Silica Sinter and the Evolution of Hot Springs in the Alvord/Pueblo Valleys, Southeast Oregon, USA

Hot springs in the Alvord/Pueblo valleys in southeastern Oregon are analogous to Basin-and-Range hydrothermal systems where heat source and permeable pathways are met through crustal thinning. Silica sinter deposition at Mickey Springs, Alvord Valley, predates the late Pleistocene high stand of pluvial Lake Alvord. At Borax Lake, Pueblo Valley, sinter deposition occurred during the Holocene. This study examines the evolution of springs at Mickey Springs, where three morphologies of sinter are present: (1) basalt clasts surrounded by sinter in interbedded conglomerate and sandstone, (2) pool-edge and aprons of sinter surrounding depressions (12–32 m diameter), and (3) quaquaversal sinter mounds with pool-edge sinter. The oldest sinter occurs in silica-cemented conglomerate and sandstone, where deposition occurred prior to 30 kya. Deposition around broad depressions and mounds occurred after 30 kya but before water levels began to rise in pluvial Lake Alvord. Thermoluminescence dates suggest sinter deposition ceased before 18 kya when silt and clay filled inactive vents and buried aprons. A few mounds hosted active springs after sinter deposition ceased but while submerged in pluvial Lake Alvord. Now, high-temperature springs, steam vents, and mud pots are concentrated in a 50 × 50 m area near the southern edge of the spring area.


Introduction
Surface and subsurface hydrogeological conditions of geothermal systems are recorded in silica sinters. However, the timing of sinter deposition relative to ongoing geological processes in the surrounding environment and the duration of conditions that allowed amorphous silica to be delivered to the surface environment are difficult to constrain.
Three hot spring areas in the Alvord and Pueblo valleys of southeastern Oregon (Figure 1) have silica sinter deposits, but none are currently depositing sinter. At two relatively pristine sites, Borax Lake [1-3] and Mickey Springs [4,5], stratigraphy, structure, hydrogeochemistry, and age dates provide insight into the time of silica sinter deposition during the evolution of these hot spring systems. Remote locations, designated as Area of Critical Environmental Concern (ACEC) by the Bureau of Land Management, and ownership of Borax Lake by The Nature Conservancy protect the hot spring deposits and provide opportunities to investigate the timing and duration of silica sinter deposition relative to the evolution of the geothermal systems and Late Pleistocene pluvial Lake Alvord. These temporal relations are within context of the tectonic evolution of the northwestern Basin-and-Range Province [6], ongoing deformation of the Alvord/Pueblo valleys [7][8][9][10], dynamics of fluid flow along active faults [11][12][13][14][15], and chronology and deformation of pluvial lake shorelines [9,10].  While many studies have explored the micro-scale dynamics of silica sinter deposition and diagenesis (e.g., [16][17][18][19]), this study examines the meso-scale lifespan and migration of spring features at Mickey Springs. The objectives of this study were to (1) refine the stratigraphy and structure of the Mickey Springs site relative to the pluvial and neotectonic history of the Alvord/Pueblo valleys, and (2) interpret the duration and timing of sinter

Pluvial Lake Alvord
Late Pleistocene lakes, including pluvial Lake Alvord, were widespread in the Basinand-Range Province. Sparse datable materials in the Alvord/Pueblo valleys forces a reliance on studies in neighboring basins to reconstruct the Pleistocene history. Benson and Thompson [33] reported lake levels for Lake Lahontan, the most studied lake 15 km to the south, dating back to 50 kya. They showed a gradual deepening of the lake until 15 kya, and a sharp increase in the lake level lasting from 15-12 kya, after which the lake quickly dried. Many of these pluvial lakes, including Lake Lahontan, may have had a dry period of little or no standing water from 35-20 kya [34].
Pleistocene pluvial Lake Alvord formed wave-cut terraces in the Alvord/Pueblo valleys that are summarized by Oldow and Singleton [10]. Their study grouped central Alvord Valley paleoshorelines into older Serrano terraces (elevation from 1320 to 1280 m) and younger Alvord terraces (elevations from 1294 to 1256 m), both of which have been offset by faults. The ages of the three older Serrano terraces are estimated by correlation with the better-studied Eetza highstand of Lake Lahontan, and loosely constrained between 200 and 130 kya [35].
Age estimates of the younger Alvord terraces vary (e.g., [10,36]). The age of the highest shoreline of the Alvord terraces is constrained by luminescence dating of shorelines in Bog Hot Valley [37] as 17.8 ± 1 kya. The lake level may have retreated to as low as 15 m above the floor of the Alvord Valley by 10-12 kya, as determined through arrowhead analysis at archaeological sites [38].
At least one episode of a rapid lake-level decrease has been documented [36] when the lake overtopped Big Sand Gap (Figure 1). The overtopping water incised Big Sand Gap from 1292 to 1280 m, draining 11.3 km 3 of water to the east and into Coyote Basin, eventually draining into the Owyhee River. Chemical correlation of an ash layer at 1243 m with deposition of Mt. St. Helens ash (set Sg tephra, age of 13-14 kya) suggests deep-water conditions at the time of deposition, but it is not determined by the authors if it was deposited before or after the overtopping and incision, which lowered the lake level to 1280 m.
Archaeological evidence from Alvord Valley indicates a pattern of drying through the Holocene. After a possible lake-level minimum at around 11.5 kya [39], basin lakes are known to have been habitation centers for native people. The Western Pluvial Lakes Tradition [40] was marked by continuous habitation around pluvial lakes from 9 to 5 kya. Beck [41] argues that the period from 5 to 3 kya saw location-dependent alternating periods of wet and dry in eastern Oregon with shallow lakes or seasonal wetlands occupying the valleys of the former deeper pluvial lakes. Today, the Alvord Desert is the driest area in Oregon, receiving less than 17 cm of precipitation a year [42].

Mickey Springs
The Alvord Valley bifurcates to the north with a western fault-bounded valley along the Steens Mountain front and an eastern fault-bounded valley, which extends with a north/northeast trend to Mickey Basin ( Figure 2). The horst block between the two valleys includes Mickey Butte, which lies northwest of Mickey Springs. Fault data are from [43,44].
Mickey Springs, Borax Lake, and Alvord Hot Springs ( Figure 1) are in the Alvord Valley Known Geothermal Resource Area (KGRA). Anadarko Petroleum Company announced the discovery of a thermal aquifer in a 451-m-deep exploration well located 2.3 km southwest of Borax Lake (press release 7 November 1989) in the Pueblo Valley. The well was flow tested for 22 h and yielded flow rates of 1500 Lm -1 with temperature measured at 152 °C. The discovery well was within an ACEC designated by the Bureau of Land Management (BLM) in 1983. The ACEC adjoins 65 hectares including Borax Lake owned by The Nature Conservancy to protect the habitat of the endemic Borax Lake chub (Gila boraxobius). Anadarko Petroleum Company dropped leases on public land in December 1996. The legal status of the chub was reviewed by Echelle and Echelle [45]. The Steens Mountain Cooperative Management and Protection Act of 2000 (Public Law 106-399) declared the Alvord Valley KGRA off limits for geothermal development. As part of the agreement, Mickey Springs in the Alvord Valley was designated an ACEC inside a Wilderness Area on public land managed by the BLM. Alvord Hot Springs is located on private land but has seen limited development for recreational purposes.
The relatively pristine Mickey Springs consists of a tight cluster of active and inactive springs in an area smaller than 4 hectares. Over 50 active vents are present at Mickey Springs. While several high-temperature mud pots and steam vents are currently active, only one spring's outflow is near boiling [1, 2,46]. Other lower-temperature springs (30-60 A third sub-basin, here called Mickey playa (MP), is southwest of Mickey Springs. Several Quaternary faults have been mapped (red lines), and some have offset shorelines from pluvial Lake Alvord (1280 m shoreline indicated by black line). Several other faults have been mapped in the vicinity of varying age (green lines). Fault data are from [43,44].
Mickey Springs, Borax Lake, and Alvord Hot Springs (Figure 1) are in the Alvord Valley Known Geothermal Resource Area (KGRA). Anadarko Petroleum Company announced the discovery of a thermal aquifer in a 451-m-deep exploration well located 2.3 km southwest of Borax Lake (press release 7 November 1989) in the Pueblo Valley. The well was flow tested for 22 h and yielded flow rates of 1500 Lm −1 with temperature measured at 152 • C. The discovery well was within an ACEC designated by the Bureau of Land Management (BLM) in 1983. The ACEC adjoins 65 hectares including Borax Lake owned by The Nature Conservancy to protect the habitat of the endemic Borax Lake chub (Gila boraxobius). Anadarko Petroleum Company dropped leases on public land in December 1996. The legal status of the chub was reviewed by Echelle and Echelle [45]. The Steens Mountain Cooperative Management and Protection Act of 2000 (Public Law 106-399) declared the Alvord Valley KGRA off limits for geothermal development. As part of the agreement, Mickey Springs in the Alvord Valley was designated an ACEC inside a Wilderness Area on public land managed by the BLM. Alvord Hot Springs is located on private land but has seen limited development for recreational purposes.
The relatively pristine Mickey Springs consists of a tight cluster of active and inactive springs in an area smaller than 4 hectares. Over 50 active vents are present at Mickey Springs. While several high-temperature mud pots and steam vents are currently active, only one spring's outflow is near boiling [1, 2,46]. Other lower-temperature springs   • C) are present and have a visually estimated combined outflow volume less than the single high-temperature area.
Oestreicher [46] studied the micro-scale textures of pool edge sinter at Mickey Springs and compared them to current microbial colonies in spring outflow channels. He determined the outflow fluid temperatures at the time of sinter deposition to be 40-60 • C, and supersaturated with amorphous silica. This silica precipitated from the thermal water onto the microbial communities present at the time, preserving the texture of the silicified microfossils.
Nicholson et al. [47] analyzed the microcrystaline structure of silica sinter at Mickey Springs and Borax Lake. The samples analyzed from Borax Lake were predominantly amorphous silica (opal-A), while the silica sinter at Mickey Springs has a significant portion of paracrystaline silica (opal-CT). As both spring systems have similar water chemistry, the primary deposits of silica were assumed to be amorphous, with the transition to the microcrystalline structure taking place over time after deposition. This led the authors to conclude, based on the silica phase, that the sinter at Mickey Springs was older (up to 30 kya) than at Borax Lake (4 kya).
Anderson and Fairley [15] modelled the heat flux at Mickey Springs using temperature probes to assess the structural context of the spring system. Their work sought to classify the type of structural setting for the springs based on the conceptual models of Curewitz and Karson [48] and favored a model of interacting fault tips, with areas of shear and extension. Further, the authors compared this finding to an unpublished fault map ( Figure 3) of the Mickey Springs area by J.S. Oldow (unpublished data, 2006). The authors correlated the areas of high heat flux to the areas of extension expected in a releasing fault step. At Borax Lake, the 100+ springs north of the lake are categorized as fault trace hot springs and geothermal fluid flow in this setting was investigated by Fairley et al. [11] and Fairley and Hinds [12,13].   [15]). Dashed box is the study area of Anderson and Fairley [15], and the approximate extent of the current study.
Silica sinter at Mickey Springs occurs in three morphologies: (1) mounds with narrow central depressions, (2) broad depressions, and (3) sinter-bearing silica-cemented sandstone and conglomerate. The distribution of these morphologies is presented in Figure 4.  [15]). Dashed box is the study area of Anderson and Fairley [15], and the approximate extent of the current study. Cummings and St. John [2] determined that fluids from the three major hydrothermal systems in the Alvord and Pueblo Valleys (Alvord Hot Springs, Borax Lake, and Mickey Springs) are meteoric in origin. They estimated a minimum aquifer temperature for Mickey Springs of 168 • C based on oxygen-sulfate isotope geothermometry. The 87 Sr/ 86 Sr ratios of thermal water and bedrock units suggest the thermal aquifer is stratigraphically beneath Steens Basalt in the Steens Mountain volcanics at a depth of 1 to 2 km. The estimated minimum reservoir temperature for the aquifer feeding springs north of Borax Lake is 203 • C. The 87 Sr/ 86 Sr ratios for springs north of Borax Lake are consistent with deeperseated welded tuff and basalt [1, 2,49].
Silica sinter at Mickey Springs occurs in three morphologies: (1) mounds with narrow central depressions, (2) broad depressions, and (3) sinter-bearing silica-cemented sandstone and conglomerate. The distribution of these morphologies is presented in Figure 4.

Mounds with Narrow Depressions
Several mounds with pool-edge sinter and quaquaversal aprons lie on a topographic bench between 1235 and 1240 m ( Figure 5). The more southern of these typically have aprons elongated along the south-dipping slope toward the lower-elevation high-temperature spring area (Q7, Q8, Q10). Brief descriptions are provided in Table 1.

Mounds with Narrow Depressions
Several mounds with pool-edge sinter and quaquaversal aprons lie on a topographic bench between 1235 and 1240 m ( Figure 5). The more southern of these typically have aprons elongated along the south-dipping slope toward the lower-elevation hightemperature spring area (Q7, Q8, Q10). Brief descriptions are provided in Table 1.

D3
Two overlapping depressions, both with sinter blocks exposed in depression floor. No sinter is exposed in walls of the depression. Slope break at edge of depression floor consistent with transition to uniform exterior blanket of fine-grained silt and clay. Many of the sinter mounds have narrow shallow central depressions, but some have no identifiable central depression. Feature Q4 ( Figure 5) has typical morphology but is unique in that it has over 3 m of relief in the central depression ( Figure 6). The central depression is rimmed with inward-dipping pool-edge sinter from the highest point on the sinter apron down to 90 cm within the vertical wall of the depression. Below this, laminar sinter is exposed from 90 cm to 2 m. Moderately sorted, subangular to rounded, coarse-grained sand is present between sheets of sinter, and silicified root casts are common. Below the laminar sinter, un-cemented, moderately sorted, subangular to rounded, coarsegrained sand is exposed ( Figure 6, 1A-DT). Silicified root-casts are also present in this sediment down to 2.9 m. The depression widens below 2 m and some cavities extend at least 2 m horizontally under the laminar sinter and above the floor of the depression (see Figure 6c). The sediment below 2.9 m is well sorted, subrounded to rounded fine-grained sand and silt ( Figure 6, 1C-DT). A large block of pool-edge sinter, broken from the rim, lies on the floor of the depression.

Broad Depressions
Several broad depressions are present in the ACEC (Figures 5 and 7). The largest of these features, D1, has pool-edge sinter exposed around much of the rim surrounding the depression (Figure 8). These depressions are 12 to 32 m in diameter, with an average depth of 1.1 m. The depressions are aligned E/NE at an elevation of 1237 m. The floors of the depressions are typically dry loose sediment, but blocks of sinter up to 1 m are present in some. A 0.6 cm × 1.5 m metal rod was used to probe the subsurface to identify areas of loose sediment (rod will penetrate when pushed by hand) and sinter (rod will not penetrate). Probing in the depression floor varied from smooth to gritty-sounding and easily inserted, to meeting refusal at as little as a few centimeters below the surface. In areas of the rim where sinter is exposed, probing laterally with a metal rod beneath the sinter is able to penetrate to the length of the rod. The sinter apron here does not have great vertical thickness but overlies loose sediment in a similar stratigraphic relation as exposed in the depression of feature Q4 ( Figure 6). coarse-grained sand is exposed ( Figure 6, 1A-DT). Silicified root-casts are also present in this sediment down to 2.9 m. The depression widens below 2 m and some cavities extend at least 2 m horizontally under the laminar sinter and above the floor of the depression (see Figure 6c). The sediment below 2.9 m is well sorted, subrounded to rounded finegrained sand and silt ( Figure 6, 1C-DT). A large block of pool-edge sinter, broken from the rim, lies on the floor of the depression. (c) Stratigraphy exposed in the central depression of feature Q4, looking north while standing on the floor of the central depression. Inward-dipping pool-edge sinter is exposed at the surface down to 90 cm. Laminar sinter interbedded with un-cemented coarse-grained sand is present from 90 cm to 2 m. Silicified root-casts are present between layers of laminar sinter and in underlying coarse-grained sand to 2.9 m. Location of the TL sample W4823 indicated by an arrow. Grain size charts of two sediment samples are shown in the center of the image, with the sample location indicated by the corresponding colored symbols.

Broad Depressions
Several broad depressions are present in the ACEC (Figures 5 and 7). The largest of these features, D1, has pool-edge sinter exposed around much of the rim surrounding the depression (Figure 8). These depressions are 12 to 32 m in diameter, with an average depth of 1.1 m. The depressions are aligned E/NE at an elevation of 1237 m. The floors of the depressions are typically dry loose sediment, but blocks of sinter up to 1 m are present in some. A 0.6 cm × 1.5 m metal rod was used to probe the subsurface to identify areas of loose sediment (rod will penetrate when pushed by hand) and sinter (rod will not penetrate). Probing in the depression floor varied from smooth to gritty-sounding and easily (c) Stratigraphy exposed in the central depression of feature Q4, looking north while standing on the floor of the central depression. Inward-dipping pool-edge sinter is exposed at the surface down to 90 cm. Laminar sinter interbedded with un-cemented coarse-grained sand is present from 90 cm to 2 m. Silicified root-casts are present between layers of laminar sinter and in underlying coarse-grained sand to 2.9 m. Location of the TL sample W4823 indicated by an arrow. Grain size charts of two sediment samples are shown in the center of the image, with the sample location indicated by the corresponding colored symbols.
Sediments in the depression floor are fine-grained silt and clay with blocks of pooledge sinter and silicified root casts ( Figure 9c). The ground surface is often crunchy underfoot when dry but makes a thick sticky mud when moistened by precipitation. A sample was collected from the surface in dry conditions from a thin (<1 cm) crust dissolved in HCl. This crust overlies loose powdery silt and clay. An auger was used to sample sediments in the southwest part of the depression, where probing with the metal rod met no refusal. The sediment was reassembled for the photo in Figure 9d. The top 27 cm consisted of 70% well-sorted brown silt and clay. The coarse portion (larger than fine sand) of the near-surface sediment was composed primarily (60%) of angular to rounded sinter fragments that did not effervesce with HCl ( Figure 9b). Fragments of root casts were also common in the coarse portion (40%). Both the root and sinter fragments are coated by carbonate, which dissolves in HCl. Less than 1% of this sample comprised lithic fragments.
inserted, to meeting refusal at as little as a few centimeters below the surface. In areas of the rim where sinter is exposed, probing laterally with a metal rod beneath the sinter is able to penetrate to the length of the rod. The sinter apron here does not have great vertical thickness but overlies loose sediment in a similar stratigraphic relation as exposed in the depression of feature Q4 ( Figure 6). Figure 7. Area of sinter mounds and broad depressions. The aprons surrounding broad depressions are blanketed with silt and clay (gray area) that effervesces with HCl. White areas in the photo are exposed sinter or broken sinter gravel and sediment. Typical sediment outside of this area is poorly sorted coarse-to fine-grained sand (blue, teal, and green dots).  . Area of sinter mounds and broad depressions. The aprons surrounding broad depressions are blanketed with silt and clay (gray area) that effervesces with HCl. White areas in the photo are exposed sinter or broken sinter gravel and sediment. Typical sediment outside of this area is poorly sorted coarse-to fine-grained sand (blue, teal, and green dots). inserted, to meeting refusal at as little as a few centimeters below the surface. In areas of the rim where sinter is exposed, probing laterally with a metal rod beneath the sinter is able to penetrate to the length of the rod. The sinter apron here does not have great vertical thickness but overlies loose sediment in a similar stratigraphic relation as exposed in the depression of feature Q4 ( Figure 6).

Figure 7.
Area of sinter mounds and broad depressions. The aprons surrounding broad depressions are blanketed with silt and clay (gray area) that effervesces with HCl. White areas in the photo are exposed sinter or broken sinter gravel and sediment. Typical sediment outside of this area is poorly sorted coarse-to fine-grained sand (blue, teal, and green dots). showing a relatively sharp interior slope of the depression. Apron surrounding the depression gradually slopes away from the depression where sinter is exposed (northeast portion) and is relatively horizontal where blanketed with fine-grained silt and clay (southwest portion). Pool-edge sinter outcrops at high-slope areas around the edge of the depression. ments in the southwest part of the depression, where probing with the metal rod met no refusal. The sediment was reassembled for the photo in Figure 9d. The top 27 cm consisted of 70% well-sorted brown silt and clay. The coarse portion (larger than fine sand) of the near-surface sediment was composed primarily (60%) of angular to rounded sinter fragments that did not effervesce with HCl ( Figure 9b). Fragments of root casts were also common in the coarse portion (40%). Both the root and sinter fragments are coated by carbonate, which dissolves in HCl. Less than 1% of this sample comprised lithic fragments. Grain size decreased with depth, while uniformity and rounding of grains increased down to 40 cm. Below 40 cm, sediment was 85% well-sorted green silt and clay, which did not react with HCl ( Figure 9b). Sand grains are subrounded to rounded. The coarse portion was 80% sinter and 20% lithic fragments (mostly basalt), and the lithic and crystal content increased to 50% of the total at the finest sand-grain sizes. This auger hole was dug to 113 cm, where the sediment was saturated and too fine grained to be brought up in the auger. The water table was at 35 cm. The temperature probe was inserted into the Grain size decreased with depth, while uniformity and rounding of grains increased down to 40 cm. Below 40 cm, sediment was 85% well-sorted green silt and clay, which did not react with HCl ( Figure 9b). Sand grains are subrounded to rounded. The coarse portion was 80% sinter and 20% lithic fragments (mostly basalt), and the lithic and crystal content increased to 50% of the total at the finest sand-grain sizes. This auger hole was dug to 113 cm, where the sediment was saturated and too fine grained to be brought up in the auger. The water table was at 35 cm. The temperature probe was inserted into the auger hole, and pushed easily further into the saturated soil to a total depth of 165 cm. Soil temperature increased with depth, from 28 • C at 40 cm to 47 • C at 165 cm.
Sinter is seldom exposed in the higher ground surrounding the depressions. Instead, the sinter aprons are buried by loose fine-grained well-sorted silt that effervesces with HCl. The coarse-grained portion contains primarily rounded sand-size grains of sinter. The extent of the silt is indicated in Figure 7. The sediment blanket was probed with a metal rod to depths up to 1.5 m before meeting refusal. Sediments outside the area of blanketing silt are typically poorly sorted coarse-to fine-grained sand (Figure 7).

Conglomerate Cemented with Silica Sinter
Silica-cemented sandstone and conglomerate crops out in the area shown in Figure 4. The location of a topographic ridge oriented roughly N/S at an elevation of~1247 m is west of the left-stepping normal faults that offset the ridge ( Figure 5). These faults separate east-dipping blocks of cemented sandstone/conglomerate from flat-lying beds of similar material. The outcrops vary between fine-grained well-sorted sandstone to poorly sorted conglomerate, typically in beds~10 cm thick. Ripple marks, trough cross-beds, and root casts are common in the finer-grained beds. Sparse petrified wood is locally preserved. In the conglomerate beds, clast sizes are up to 5 cm. Clasts are mainly basalt with rare andesite and rhyolite [1]. The coarser-grained conglomerates are exposed to the north and east, and maximum grain size decreases toward the southwest. No outcrop of the silicacemented sandstone/conglomerate is present east of the outflow channel from feature Q5 (Figure 7). In outcrops of the conglomerate and sandstone north of the parking area (Figure 4), bedding along an incised valley dips to the north. Loosely cemented sand is present in slope wash at and below~1247 m northeast of the parking area.
Locally, coarse-grained sand and small pebbles are suspended in opaline silica, suggesting coeval deposition of silica sinter and lithic clasts. Uranium series disequilibrium age dating at Argonne National Labs yielded a date of <16,000 ybp [2]. This poorly constrained date influenced interpretations of time of deposition of the sandstone/conglomerate and sinter mounds [2,4] (see Section 4).

Current Hydrothermal Activity
Active springs are present in two settings: (1) high-temperature springs at lower elevation, and (2) warm springs located within sinter features.
High-temperature springs at lower elevation occur in a 50 m × 50 m roughly circular area at an elevation of 1230 m and south of the sinter mounds and depressions ( Figure 4). Mud pots, the highest temperature springs, steam vents, and hot ground ( Figure 10) are present in this area. The morphology of these thermal features is diverse and changes frequently. Within this area, (1) a mud pot (MP in Figure 10) erupted mud sometime between March and May, 2014; (2) geysering from the persistently highest temperature spring is reported by St. John and Cummings [50], Cross [51], and Kipple [52,53]; and (3) steam vents from small diameter orifices to the north and at slightly higher elevation form the highest temperature springs.
There is no evidence of current or past silica sinter deposition in this area. Water discharged from the high-temperature springs travels south toward dug-out ponds for watering cattle outside the ACEC fence. Carbonate is deposited in outflow channels where effluent temperatures are approximately 73 • C. Oestreicher [46] examined the microbiota within the temperature gradient found in these outflow channels.
The mud pots are typically 1-2-m-diameter depressions with a floor of wet bubbling mud. They are located near the southern edge of the high-temperature area and are flanked to the south by a 1.0-to 1.5-m-high berm of very poorly sorted sediment ( Figure 11). Between March and May, 2014, a mud pot exploded and resurfaced the surrounding area (3 m radius) with sediments that were 70 % moderately sorted silt and clay (see the grain size chart in Figure 11). The coarse portion was primarily basalt clasts but contained no silica sinter fragments.
The area of high-temperature springs, steam vents, and mud pots is bounded by ground that is warm to the touch on the north and west (10 cm probe recorded a temperature between 67 and 95 • C), by a 1.5-m-high berm on the southwest (Figure 11), and a distinct change in sediment type on the east ( Figure 10, right side of image). Together, the hot ground, berm, and sediment change encircle the high-temperature area and mark its outer extent. There is no evidence of current or past silica sinter deposition in this area. Water discharged from the high-temperature springs travels south toward dug-out ponds for watering cattle outside the ACEC fence. Carbonate is deposited in outflow channels where effluent temperatures are approximately 73 °C. Oestreicher [46] examined the microbiota within the temperature gradient found in these outflow channels.
The mud pots are typically 1-2-m-diameter depressions with a floor of wet bubbling mud. They are located near the southern edge of the high-temperature area and are flanked to the south by a 1.0-to 1.5-m-high berm of very poorly sorted sediment ( Figure  11). Between March and May, 2014, a mud pot exploded and resurfaced the surrounding area (3 m radius) with sediments that were 70 % moderately sorted silt and clay (see the grain size chart in Figure 11). The coarse portion was primarily basalt clasts but contained no silica sinter fragments.   There is no evidence of current or past silica sinter deposition in this area. Wate discharged from the high-temperature springs travels south toward dug-out ponds fo watering cattle outside the ACEC fence. Carbonate is deposited in outflow channe where effluent temperatures are approximately 73 °C. Oestreicher [46] examined the m crobiota within the temperature gradient found in these outflow channels.
The mud pots are typically 1-2-m-diameter depressions with a floor of wet bubblin mud. They are located near the southern edge of the high-temperature area and ar flanked to the south by a 1.0-to 1.5-m-high berm of very poorly sorted sediment (Figur 11). Between March and May, 2014, a mud pot exploded and resurfaced the surroundin area (3 m radius) with sediments that were 70 % moderately sorted silt and clay (see th grain size chart in Figure 11). The coarse portion was primarily basalt clasts but containe no silica sinter fragments. Figure 11. TL sample W4828 was collected from an auger hole in the berm southwest of the hightemperature area. The grain size chart for sample TL-HS (red dot) collected at the TL sample depth. The grain size chart HS-MPC (blue triangle) is for debris ejected from the mud pot betwee The pool-edge sinter was sampled for uranium series disequilibrium dating [2] but was found unsuitable for dating. The relief between the apron rim and the depression is 1 m. A muddy spring is present on the north edge of the floor of the depression. The water surface is continually rippling, presumably from gas discharge, which circulates microbial mats around the pool. Probing this pool with a metal rod revealed that the pool extends north under the sinter apron for at least the length of the rod (1.5 m). outer extent.
Warm springs located within sinter features are within the central depressions of feature D1 and a few sinter mounds (e.g., Q9). Spring temperatures in the central depression of D1 are included in Figure 8. Only one spring (Q5) supports a pool and has surface outflow.
Feature Q9 (Figure 12) is rimmed by up to 1 m (measured vertically) of inward dipping pool-edge sinter, with an apron diameter of 25 m and central depression diameter of 5 m. The pool-edge sinter was sampled for uranium series disequilibrium dating [2] but was found unsuitable for dating. The relief between the apron rim and the depression is 1 m. A muddy spring is present on the north edge of the floor of the depression. The water surface is continually rippling, presumably from gas discharge, which circulates microbial mats around the pool. Probing this pool with a metal rod revealed that the pool extends north under the sinter apron for at least the length of the rod (1.5 m).    Figure 12, at the maximum thickness of the sediment) is 80% subangular to rounded lithic fragments, and 20% angular to subangular sinter. Cummings and St. John [2] report similar resurfacing at this site.
An auger hole in the depression (stratigraphic column right side of Figure 12) reached the rooted zone from the grass previously growing in the depression at a depth of 13 cm.
Below this rooted zone, sediment was primarily silty sand and sorting increased with depth down to 60 cm. From 60 to 78 cm was another rooted zone, with poorer sorting and a higher percentage of coarse sand. Below this rooted zone, grain size decreased to 85% well-sorted silt and clay, green in color, and similar to the deeper sediment in D1. The water table was at 72 cm. At a depth of 105 cm, the auger broke through several gravel-sized sinter clasts. The total depth reached was 127 cm, where saturation prevented the recovery of material.

Thermoluminescence Dating
The sampling strategy for thermoluminescence (TL) dating was to constrain the age of sinter deposition while respecting ACEC restrictions and, due to dangerously high ground temperatures, samples were limited to the shallow (<1 m) subsurface. Six sample sites were selected for TL dating and the results are summarized in Table 2, Figure 13, and Appendix A.  Feature Q9 was resurfaced by a mud eruption that occurred between March an May, 2014, emanating from the spring in the depression. The eruption deposited moder ately sorted silt and clay over an area of ~50 m 2 to a maximum thickness of 13 cm. Th coarse-grained portion of this sediment (3C-MB, collected, as the arrow indicates in Figur  12, at the maximum thickness of the sediment) is 80% subangular to rounded lithic frag ments, and 20% angular to subangular sinter. Cummings and St. John [2] report simila resurfacing at this site.
An auger hole in the depression (stratigraphic column right side of Figure 12 reached the rooted zone from the grass previously growing in the depression at a dept of 13 cm. Below this rooted zone, sediment was primarily silty sand and sorting increase with depth down to 60 cm. From 60 to 78 cm was another rooted zone, with poorer sortin and a higher percentage of coarse sand. Below this rooted zone, grain size decreased t 85% well-sorted silt and clay, green in color, and similar to the deeper sediment in D1 The water table was at 72 cm. At a depth of 105 cm, the auger broke through severa gravel-sized sinter clasts. The total depth reached was 127 cm, where saturation prevente the recovery of material.

Thermoluminescence Dating
The sampling strategy for thermoluminescence (TL) dating was to constrain the ag of sinter deposition while respecting ACEC restrictions and, due to dangerously hig ground temperatures, samples were limited to the shallow (<1 m) subsurface. Six sampl sites were selected for TL dating and the results are summarized in Table 2, Figure 13, an Appendix A. Figure 13. Barplot of TL ages, showing the age (triangle) and uncertainty (lines) of each sample Material beneath the laminar sinter of Q4 is the oldest dated sample at 30 kya. Well-sorted fine grained sediment from depressions and blanketing sinter aprons range in age from 18-12 kya. Th age of the sediment from near the current high-temperature springs is ~9 kya. The youngest TL dat is from poorly sorted sand in feature Q3. Material beneath the laminar sinter of Q4 is the oldest dated sample at 30 kya. Well-sorted finegrained sediment from depressions and blanketing sinter aprons range in age from 18-12 kya. The age of the sediment from near the current high-temperature springs is~9 kya. The youngest TL date is from poorly sorted sand in feature Q3.
Potential underestimation of the true time of deposition by the TL process as used here may emerge from the heating of sediments by the hydrothermal water, cosmic ray contamination, or moisture content of the sample at time of processing. Appendix A contains information on the sample characteristics, analytical procedures, and results for these TL analyses. Sufficient heating can excite electrons, allowing them to escape from the crystal lattice, effectively reducing the TL age. Since all plateau and analysis temperatures were at or above 275 • C, it is assumed here that near-boiling spring water did not provide sufficient heating to bleach the samples. Despite the shallow sample depth used in this study, it is assumed that samples were sufficiently deep such that cosmic ray contamination did not significantly bleach the samples. Finally, the presence of moisture in sediment acts as radiation shielding, slowing the accumulation of electrons in the traps. The moisture content of the sample during the dating process is assumed to be constant through time; if the moisture content was higher in the past, then the actual age of sediments would be older than those determined by the TL process. Therefore, the ages reported here are considered the minimum ages.
At Q4 (Figure 6; sample W4823), a sinter mound, a sample was collected from unconsolidated sediment underlying laminated sinter. Sinter from two sources is present in the the Q4 sinter mound. The oldest, the laminated sinter, is part of the apron from a neighboring broad depression. The younger, the pool-edge sinter and thick-bedded sinter, was deposited when the Q4 mound vent was active. Sample W4823 was collected by augering horizontally into the wall of the central depression immediately below the laminated sinter ( Figure 6) and from a horizontal auger distance of 30 cm. The soil temperature was 29 • C and the laboratory-measured moisture content was 22.2%. The grain size of these sediments is presented in Figure 6. TL age is 30.7 ± 7.9 kya. Low TL sensitivity led to a temperature plateau comparison between 275 and 350 • C, resulting in scattered TL data and an unusually large age uncertainty.
Sample W4828 was collected from the berm that circles the southwest portion of the high-temperature area ( Figure 11) and near the rim of the mud pot that erupted between March and May, 2014. The sample was 40 cm below the surface. The soil temperature was 84 • C and the moisture content was reported as 10.1%. The sample included a large rock approximately half the volume of the total sample. This can distort the results of the TL process, but the grain size analysis and local observations show poor sorting of the sediments and therefore the sample was not considered anomalous for TL age determination. The age of this sample was 9.2 ± 1.0 kya.
Three samples were collected from the floors of the central depressions rimmed by sinter. Samples collected from two sites, Q12 ( Figure 14) and D1 (Figure 8), were fine-grained sand, silt, and clay. At Q3 (Figure 15), the sample was very poorly sorted, sinter-bearing sand to gravel. These samples constrain the age of sediments that infill the vents.
Sample W4829 was collected at sinter mound Q12 ( Figure 14) from an auger hole 27 cm below the surface of the central depression. The soil temperature was 59 • C and the laboratory-measured moisture content was 34.3%. Sediments from 0-56 cm were poorly sorted, loose, sandy silt, with sparse clasts of sinter up to 4 cm, but the sample sent for TL analysis was primarily sand and silt. TL output plateaued between 300 and 500 • C, with a resulting age of 18.1 ± 2.1 kya.
Sample W4831 was collected at a depth of 53 cm from the central depression of the sinter mound Q3 (Figure 15). A sinter apron surrounds this feature and pool-edge sinter is visible immediately surrounding an area of loose, poorly sorted silty sand with pebbles, flush with the sinter elevation. In the portion of the TL dating process that involved cleaning the grains with hydrofluoric acid (after treatment with HCl), the sample reacted violently to the acid, indicating a high feldspar content. The coarse portion of the sediment contained~75% angular clasts of sinter up to 6 cm brought up in the auger and~25% coarse basalt sand up to 2 mm. The soil temperature was 36 • C at 50 cm below the surface. The moisture content was reported as 4.1%. The TL age was 0.8 ± 0.4 kya.  Sample W4829 was collected at sinter mound Q12 ( Figure 14) from an auger hole 27 cm below the surface of the central depression. The soil temperature was 59 °C and the laboratory-measured moisture content was 34.3%. Sediments from 0-56 cm were poorly sorted, loose, sandy silt, with sparse clasts of sinter up to 4 cm, but the sample sent for TL Figure 14. Image looking north at feature Q12, location of TL sample W4829. The fracture in the sinter is oriented N/NE and continuation is indicated by the linear orientation of bushes in the image. The grain size chart is shown for sample TL-CH, which was collected immediately above the TL sample depth of 27 cm.  Sample W4829 was collected at sinter mound Q12 ( Figure 14) from an auger hole 27 cm below the surface of the central depression. The soil temperature was 59 °C and the laboratory-measured moisture content was 34.3%. Sediments from 0-56 cm were poorly sorted, loose, sandy silt, with sparse clasts of sinter up to 4 cm, but the sample sent for TL Figure 15. Location of TL sample W4831 in Q3. The sinter apron is relatively flat, with a central area of loose sediment level with the pool-edge sinter surrounding it. Sediment from the auger hole immediately above the TL sample depth (corresponding red dot) was 30% fine sand, poorly sorted with gravel-size pieces of angular sinter and pebbles of sub-rounded basalt (inset top left).
Sample W4832 was collected in the broad depression of feature D1 (Figure 8) from 24 cm below the surface near the south edge of the central depression. This auger hole was adjacent to the hole for the sediment core shown in Figure 9d. The sample depth was 27-37 cm, and was selected initially for practicality, as soil saturation made acquiring a deeper intact sample problematic with the tools used. However, this depth is at the transition from the surface sediment containing root fragments and the lower well-sorted silt and clay. The laboratory-measured moisture content was reported as 47.0%. TL sensitivity was again low, leading to an above-average TL age uncertainty. The age of this sample was 12.8 ± 4.4 kya.
Sample W4830 was collected from fine-grained sediments blanketing the sinter apron of the broad depression D1, 47 cm below the surface (Figure 16). The sediment at the TL sample depth was well-sorted, subrounded to rounded, sandy silt with 65% fine silt and clay. The soil temperature was 33 • C. The moisture content was reported as 32.2%. The TL age of this sample was 17.9 ± 3.0 kya. TL sensitivity was similar to sample W4829, and the TL ages overlap within one standard deviation ( Figure 13).
ing the grains with hydrofluoric acid (after treatment with HCl), the sample reacted violently to the acid, indicating a high feldspar content. The coarse portion of the sediment contained ~75% angular clasts of sinter up to 6 cm brought up in the auger and ~25% coarse basalt sand up to 2 mm. The soil temperature was 36 °C at 50 cm below the surface. The moisture content was reported as 4.1%. The TL age was 0.8 ± 0.4 kya.
Sample W4832 was collected in the broad depression of feature D1 (Figure 8) from 24 cm below the surface near the south edge of the central depression. This auger hole was adjacent to the hole for the sediment core shown in Figure 9 d. The sample depth was 27-37 cm, and was selected initially for practicality, as soil saturation made acquiring a deeper intact sample problematic with the tools used. However, this depth is at the transition from the surface sediment containing root fragments and the lower well-sorted silt and clay. The laboratory-measured moisture content was reported as 47.0%. TL sensitivity was again low, leading to an above-average TL age uncertainty. The age of this sample was 12.8 ± 4.4 kya.
Sample W4830 was collected from fine-grained sediments blanketing the sinter apron of the broad depression D1, 47 cm below the surface (Figure 16). The sediment at the TL sample depth was well-sorted, subrounded to rounded, sandy silt with 65% fine silt and clay. The soil temperature was 33 °C. The moisture content was reported as 32.2%. The TL age of this sample was 17.9 ± 3.0 kya. TL sensitivity was similar to sample W4829, and the TL ages overlap within one standard deviation ( Figure 13).

Ground Penetrating Radar
The preliminary GPR study reported by Mowbray and Cummings [4] used 250 MHz shielded antennas spaced 0.5 m apart operating at 165 Volts with a horizontal resolution of 20 cm and a 2 m penetration depth. The track passed through the four broad depressions ( Figure 5D1-D4) and extended onto the silica-cemented sandstone/conglomerate unit outcrops to the southwest. At the depth attained with the 250 MHz antennas, the sandstone/conglomerate unit continued and is interpreted to underlie thin sinter deposits.
In May, 2014, three transects were surveyed with 1000 volt antennas ( Figure 5). With these antennas, the top meter of the surface is noisy from the strength of the GPR signal extending in all directions, and only resolves subsurface features greater than 1-2 m below the surface, below the maximum thickness of most sinter aprons. Two tracks (1 and 3) were made from west to east, and one track (2) was made from north to south. Both 50 and 100 MHz antennas were deployed on track 1, while only 50 MHz antennas were deployed on track 2 and 3. The 50 MHz antennas were able to penetrate to a depth of approximately 17 m, while the 100 MHz antennas penetrated to a depth of approximately 10 m. All GPR tracks are shown with and without topographic correction in Figure S1: GPR raw data and topographically corrected data.
Track 1 (Figure 17) was surveyed using the 50 MHz ( Figure S1: GPR raw data and topographically corrected data for Track 1, 50 MHz) and the 100 MHz ( Figure S2: GPR raw data and topographically corrected data for Track 1, 100 MHz) antennas, over a distance of 222 m. The track started at the high point of the silicified sandstone, passed just north of the central depression of feature Q4, crossed the center of feature D1, and terminated before the east fence of the ACEC. A 5-m gap in the 50 MHz track on the crest of Q4 was caused by temporary disconnection of the antennas from the recording computer.
In May, 2014, three transects were surveyed with 1000 volt antennas ( Figure 5). With these antennas, the top meter of the surface is noisy from the strength of the GPR signal extending in all directions, and only resolves subsurface features greater than 1-2 m below the surface, below the maximum thickness of most sinter aprons. Two tracks (1 and 3) were made from west to east, and one track (2) was made from north to south. Both 50 and 100 MHz antennas were deployed on track 1, while only 50 MHz antennas were deployed on track 2 and 3. The 50 MHz antennas were able to penetrate to a depth of approximately 17 m, while the 100 MHz antennas penetrated to a depth of approximately 10 m. All GPR tracks are shown with and without topographic correction in Figure S1: GPR raw data and topographically corrected data.
Track 1 (Figure 17) was surveyed using the 50 MHz ( Figure S1: GPR raw data and topographically corrected data for Track 1, 50 MHz) and the 100 MHz ( Figure S2: GPR raw data and topographically corrected data for Track 1, 100 MHz) antennas, over a distance of 222 m. The track started at the high point of the silicified sandstone, passed just north of the central depression of feature Q4, crossed the center of feature D1, and terminated before the east fence of the ACEC. A 5-m gap in the 50 MHz track on the crest of Q4 was caused by temporary disconnection of the antennas from the recording computer. Figure 17. GPR transect 1 from west to east, descending from the silicified sandstone outcrop, across feature Q4 and D1, and terminating at the east fence of the ACEC. ( Figure S1: GPR raw data and topographically corrected data for Track 1, 50 MHz. Figure S2: GPR raw data and topographically corrected data for Track 1, 100 MHz). Track 2 (Figure 18) was surveyed using 50 MHz ( Figure S3: GPR raw data and topographically corrected data for Track 2, 50 MHz) antennae over a distance of 265 m. This track traversed feature D1, crossed the west flank of the sinter apron of Q9, passed west of Q12, crossed the center of the high-temperature spring area, and terminated at the south fence of the ACEC.  Figure S1: GPR raw data and topographically corrected data for Track 1, 50 MHz. Figure S2: GPR raw data and topographically corrected data for Track 1, 100 MHz). Track 2 (Figure 18) was surveyed using 50 MHz ( Figure S3: GPR raw data and topographically corrected data for Track 2, 50 MHz) antennae over a distance of 265 m. This track traversed feature D1, crossed the west flank of the sinter apron of Q9, passed west of Q12, crossed the center of the high-temperature spring area, and terminated at the south fence of the ACEC.
Track 3 (Figure 19) was surveyed using the 50 MHz ( Figure S4: GPR raw data and topographically corrected data for Track 3, 50 MHz) antennae over a distance of 180 m. The track began west of the sandstone ridge over sparsely vegetated soil, where no outcrop was present, crossed the high-temperature area just north of the mud pots and high-temperature spring outflows, and over a small rise east of the high-temperature springs, terminating at the east fence of the ACEC. Track 3 (Figure 19) was surveyed using the 50 MHz ( Figure S4: GPR raw data and topographically corrected data for Track 3, 50 MHz) antennae over a distance of 180 m. The track began west of the sandstone ridge over sparsely vegetated soil, where no outcrop was present, crossed the high-temperature area just north of the mud pots and hightemperature spring outflows, and over a small rise east of the high-temperature springs, terminating at the east fence of the ACEC.  Track 3 (Figure 19) was surveyed using the 50 MHz ( Figure S4: GPR raw data and topographically corrected data for Track 3, 50 MHz) antennae over a distance of 180 m. The track began west of the sandstone ridge over sparsely vegetated soil, where no outcrop was present, crossed the high-temperature area just north of the mud pots and hightemperature spring outflows, and over a small rise east of the high-temperature springs, terminating at the east fence of the ACEC. Broad parabolic reflections are visible in all three GPR tracks before the addition of topography (Figures S1-S4). Once topography was added, the parabolic reflectors are distorted. The width of the parabola indicates the presence of a zone rather than a point feature. These broad parabolas can be produced by zones of material with a different density or electrical properties to that of the surrounding area. Possible causes for these Common features visible in the 50 and 100 MHz images are (1) the dipping beds of the silicified sandstone, (2) deterioration of the signal due to thick silt at the ground surface, and (3) alteration of the signal due to shallow groundwater. All three GPR transects terminated near the fence line of the ACEC. Strong reflectors in the GPR tracks rise toward the termination point of each track and are interpreted as air-wave signals from the fence posts, and determined not to be indicative of the subsurface structure. Topography-corrected raw data for the transects are reproduced here (Figures 17-19) and the stratigraphic interpretations based on these data are illustrated below each transect.
The dominant texture in the GPR tracks is sub-horizontal to gently dipping lines, found primarily in the lower two-thirds of the imaged areas. This is interpreted to be a relatively uniform unit of underlying sediment, indicating that all sinter precipitated at Mickey Springs is near the surface and forms a relatively thin capping unit.
The silica-cemented sandstone/conglomerate unit was exposed at the surface on the western portion of track 1 (Figure 17). The GPR image shows some thick (compared to the thin sub-horizontal bedding of the underlying sediment) horizontal bedding accompanied by east-dipping lines. The thick horizontal bedding extends 5-10 m in depth and is thicker than the thin horizontal lines of the bottom two-thirds of the transect. Because these lines are coincident with the sandstone outcrop, they are interpreted to trace the subsurface extent of the sandstone and indicate the sandstone/conglomerate unit is only~10 m thick. Similar texture is not visible in the GPR data from the eastern portion of track 1, nor in track 2 or 3.
The east-dipping lines in the sandstone/conglomerate unit in track 1 continue at depth in the thinner-bedded sediment as discontinuities in bedding. These discontinuities are interpreted as faults, and are in proximity to many parabolics, indicating a damage zone ( Figures S1-S4). Three faults are also interpreted from track 2 ( Figure 18) at discontinuities in bedding. These faults are coincident with the slope break between the topographic bench containing the sinter mounds and depressions at 1235 m, dipping toward the current high-temperature springs to the southeast.
Areas below sinter aprons have non-uniform bedding planes and discontinuities, typically approximating the width of the apron or depression and narrowing downward. From the exposure in the depression of Q4, the planar-bedded sediments below the laminar sinter appear as primary deposition that remains unaltered by the thermal waters that deposited the sinter; however, the GPR data suggests a zone of alteration underlying each feature.
The area of the high-temperature springs in the E/W transect of track 3 ( Figure 19) appears blocky and undulating down to 10 m, while the N/S transect of track 2 does not have similar blocky features. Both transects indicate a discontinuity of bedding at 5-10 m beneath the high-temperature area. Some of the largest blocky light and dark zones in track 3 coincide with the main high-temperature springs, which flow from cracks primarily oriented N/S. The blocky features are therefore likely showing the shallow subsurface structure on which the fluid is rising. Several parabolics are also present just beneath the blocky area and may indicate the continuation of the conduit at depth ( Figure S4: GPR raw data and topographically corrected data for Track 3, 50 MHz).

Discussion
Silica sinter deposition requires the discharge of hot water with colloidal silica suspended in the effluent. Deposition of the colloidal silica occurs as the solution cools to form pool-edge sinter and outflow channels across the surrounding apron. Encrustation of algae in the pool and outflow channels and vegetation growing on the apron are well documented (e.g., [17][18][19]46]). These conditions were met before the Alvord Valley was inundated by late Pleistocene pluvial Lake Alvord at Mickey Springs and during the Holocene at Borax Lake [3]. In this discussion, the stratigraphic, age, and structural relations are examined, and a timeline presented for the sinter deposits at Mickey Springs.

Stratigraphic Relations
GPR applied to geothermal systems with siliceous sinter deposits was introduced by Dougherty and Lynne [54] and Lynne and Dougherty [55]. The technique has been applied to siliceous sinters at Opal Mound, Utah, Steamboat Springs, Nevada, and Horohoro and Pukemoremore in the Taupo Volcanic Zone, New Zealand [56] and at Old Faithful Geyser in Yellowstone National Park [57] to examine the thickness of sinter deposits (to about 10 m) and the distribution of fracture systems associated with hot springs and sinter deposits.
GPR surveys and SfM photogrammetry helped resolve two questions at Mickey Springs: (1) What is the stratigraphic relation between the sinter mounds/broad depressions and the sinter-bearing silica-cemented sandstone/conglomerate unit? (2) What are the characteristics of the subsurface environment beneath the sinter deposits?
East-dipping bedding in the sinter-bearing silicified sandstone/conglomerate unit has been interpreted either as foreset beds or tilted fault blocks. Cummings and St. John [2] interpreted the dipping beds in these outcrops as the foreset beds of a delta that prograded into pluvial Lake Alvord. The uranium series disequilibrium date of <16,000 ybp [2] available at that time was consistent with this interpretation of coeval sedimentation and sinter deposition. This interpretation suggested that subaerial sinter deposition in the mounds and depressions had occurred at Mickey Springs after the pluvial Lake Alvord dried.
This interpretation also guided the thinking in Mowbray and Cummings [4] as they presented a climate-driven model for the evolution of the Mickey Springs site. In this model, sinter deposition ceased during the Holocene as a lagged response to the warming climate and drying of pluvial Lake Alvord. When Pluvial Lake Alvord was present, it provided recharge to the deep heat source below the Steens Basalt. Although fault slip continued through the Holocene to maintain permeable pathways [8,10], the meteoric water available to the system diminished with the drying of the lake. The preliminary GPR study [4] at the depth attained with the 250 MHz antennas seemed to confirm that the foresets of the silicified delta continued and underlie the sinter deposits.
Reinterpretation of these outcrops based on SfM photogrammetry ( Figure 5), additional field work, and 50 MHz and 100 MHz GPR transects (Figures 17-19) supported tilted blocks along left-stepping, down-to-the-east, north-striking normal faults to explain these east-dipping blocks of sinter-bearing silica-cemented sandstone and conglomerate. In Figure 5, left-stepping normal faults are shown separating the sinter-bearing silicacemented sandstone/conglomerate unit from the area of sinter mounds/broad depressions. This reinterpretation aligns better with sedimentological details in outcrops where the depositional architecture of bedding and relations between sandstone and conglomerate layers are more consistent with deposition on an alluvial fan rather than deposition on a delta front. The GPR data are consistent with this reinterpretation. However, the deeper resolution of the 50 MHz antennas shows that the sandstone/conglomerate unit is not continuous at depth under the sinter mounds/broad depressions and spring area.
The GPR data and outcrops at sites, such as Q4, Q9, and D1, indicate that the sinter aprons around springs are thin. At Q4, the total sinter thickness exposed in the vent walls is 2 m. This is similar to direct and indirect observations at other sinter mounds and sinter rims around broad depressions. There is no evidence from observation or in the GPR transects of stacking of sinter deposits at several levels beneath the features observed at the modern surface. The GPR data are consistent with areas of stratigraphic disruption (faults/fractures) and potentially hydrothermal alteration underlying hot spring vents.

Timing of Sinter Deposition
The ages of the silica sinter deposits at the three hot springs in the Alvord/Pueblo valleys are reported for Borax Lake [3,47,58] and at Mickey Springs [2,5,47]. The age of the sinter deposits at Alvord Hot Springs has not been determined.
At Borax Lake in the Pueblo Valley, a seismic refraction study [3,58] indicated that the 8.3-m-thick biomorphic mound overlies silt-and clay-rich sediment deposited in pluvial Lake Alvord. Pool-edge sinter rims the 4-hectare lake, which commands the crest of the shield-shaped mound. The mound is comprised of diatom frustules, silt-size opal-A silica particles, silica-encrusted and permineralized vascular plant fragments, sinter fragments, discontinuous carbon-rich plant layers, charcoal layers, and sparse hard sinter layers. A 1.2 m long, 0.64 cm diameter wooden dowel was used to probe the flanks of the mound below the sinter apron that surrounds the lake. Resistance was rarely encountered and locally, the dowel would sink under its own weight. An AMS radiocarbon date for a discontinuous charcoal layer below the sinter apron that extends northward from the lake shore is BC 3775 to 3655 calibrated calendar years (4930 ± 60 RCYBP, ±1 S.D.; elevation = 1242.93 m). A calibrated calendar age of AD 1420 to 1455 (470 ± 50 RCYBP; elevation = 1237.81 m) was obtained from charred plant material immediately above hard silica sinter on the east flank of the mound. A normal fault displaced silica sinter and a charred layer with a calibrated calendar age of AD 685 to 800 (1270 ± 50 RCYBP; elevation = 1236.73 m) north of Borax Lake [3]. This fault is one of the active left-stepping normal faults that control hot springs north of Borax Lake and was included in an investigation of fluid flow and distribution of permeability in an active fault zone [11][12][13][14]. Based on the microcrystallinity of sinter at Borax Lake, Nicholson et al. [43] interpreted the age of sinter deposition to be 4 kya.
At Mickey Springs, the age of coeval deposition of silica sinter, sand, and conglomerate is poorly constrained. Cross bedding, root casts, fragments of petrified wood, and subangular pebbles and cobbles suggest these coarse-grained sediments accumulated on an alluvial fan. The extent of sinter-bearing silica-cemented sandstone and conglomerate ( Figure 4) suggests the discharge of thermal water may have been relatively diffuse. At best, sinter deposition is constrained within the long time span between the high stands of pluvial Lake Alvord that produced the Serrano terraces (~130 kya, [10]) and the 30 kya TL date for unconsolidated sand beneath sinter at Q4.
Deposition of sinter mounds and broad depressions started at approximately 30 kya and persisted until late Pleistocene pluvial Lake Alvord occupied the Alvord basin. This history was constructed using TL dating, GPR surveys, SfM photogrammetry, granulometry, and stratigraphic relations. Sinter deposition at the sinter mounds and broad depressions based on the crystallinity of the sinter (opal-CT) was estimated at 30 kya [43]. This is consistent with the TL date presented in this study for feature Q4 (Figure 6), where a sample collected beneath the laminated sinter deposit and underlying un-cemented sediment yielded an age of 30 kya but with relatively large error (Sample W4823, Table 2).
Sinter deposition had ceased at Mickey Springs prior to submersion in pluvial Lake Alvord. Two lines of evidence support this interpretation: (1) sinter sand, cobbles, and pool-edge sinter ensconced in silt and clay; and (2) the TL dates for the infilling sediments.
First, the sediment that infills the vents of the sinter mounds and broad depressions is dominated by silt and clay. The fine-grain size and sorting are consistent with lacustrine deposition. Sand to cobbles and blocks of pool-edge sinter are ensconced in the infilling fine-grained material. The buried sinter cobbles and blocks require the sinter to have been present before sedimentation.
Second, TL dates from the Q12 (sample W4829, Figure 14) vent and sediment covering the apron of the D1 broad depression correspond to the determined age of the early filling stage of pluvial Lake Alvord. The materials submitted for TL dating from the sinter mounds and broad depressions were opportunistically collected at the depth where sediment return in the hand auger was successful. Thus, the dates do not mark specific horizons within the filling sediment. However, the oldest date from this setting, 18.1 kya, from the Q12 site (sample W4829) is consistent with age determinations for the times when pluvial Lake Alvord occupied the Alvord basin [37]. Sediment covering the aprons of broad depressions and sinter mounds postdates sinter deposition. At the D1 broad depression, this material near the contact between silty sediment that overlies the silica sinter apron was dated at  Figure 16). Uncertainty of the age of this sample and that from the central depression of Q12 (W4829) overlap within the precision of the technique (Figure 13).
The younger age for infilling materials at the D1 site was for a sample collected near the contact between rooted sediment characteristic of the upper part of this auger hole and underlying clayey silt deposits (Figure 9). This age, 12.8 kya, suggests deposition during the late stages of pluvial Lake Alvord.
The berm located southwest of the high-temperature area is interpreted to be ejecta from the high-temperature mud pot/springs area and to have been constructed after the drying of pluvial Lake Alvord. An age date for sediment near the mud pots, 9.2 kya (W4831, Figure 11), was collected from a site with no known sinter deposits. Clasts of sinter were not present in the debris that blanketed part of this area from the mud pot explosion between March and May 2014. The GPR image suggests a discontinuity in bedding of sediments within the high-temperature area, and the berm delineates the boundary of this area.
The youngest TL age was determined for sandy sediment including basalt lithics (~25%) and angular silica sinter clasts (75%) at the Q3 site ( Figure 15). The Q3 site is one of the northernmost sinter deposits and is at an elevation similar to the landscape that lies north and northwest of the sinter deposits. This age, 0.8 kya, may reflect inundation of this sinter deposit by sheet wash from a flash flood event originating on Mickey Butte.
TL dates and crystallinity of sinter (opal-CT) [47] suggest hydrothermal discharge has occurred at the Mickey Springs site for at least 30,000 years. However, sinter deposition that formed the sinter mounds and broad depressions commenced sometime after 30 kya and ended sometime around 18 kya before the filling of pluvial Lake Alvord. The grain size data and TL dates are consistent with sedimentation from late Pleistocene pluvial Lake Alvord infilling vents of hot springs that had previously produced sinter deposits. The TL age dates are consistent with the span of ages reported for late Pleistocene pluvial Lake Alvord and the grain sizes are consistent with those likely produced from the glacial flour released into the basin from melting glaciers on Steen Mountain.
The thin sinter deposits suggest that deposition of sinter at the sinter mounds and broad depressions was short lived. GPR data suggest there is no stacking of sinter deposits one upon the other, at least within the 17 m resolved by the 50 MHz antenna surveys. The TL dates suggest that deposition occurred over a relatively short period of time bracketed by the 30 kya date at Q4 and the ages of lacustrine silt deposited in inactive vents by at least 18 kya.

Structural Interpretation
The field-based structure map by J.S. Oldow (fide [15]; Figure 3) placed Mickey Springs at interacting fault tips in a system of northeast-striking normal faults. The analysis of temperature data [15] suggest that the Mickey Springs site is located "in a fault tip-line region or in a releasing step within an obliquely slipping fault intersection area." SfM photogrammetry, additional field investigations, and GPR were used to refine the model presented in Figure 20. The changes to the map of J.S. Oldow (fide [15]) include the addition of (1) north-striking, left-stepping, down-to-the-east, normal faults and (2) a down-to-the south, northeast-striking normal fault. Reinterpretation of the east-dipping beds in the sandstone/conglomerate unit at the west edge of the area of sinter mounds from a delta front [2] to tilted fault blocks changed the age relations and structural interpretation of Mickey Springs. Taking the 30 kya TL age of the sediments that underlie sinter at Q4 as a minimum age for the sandstone/conglomerate unit, and a total fault offset of 35 m (from the highest point on the sandstone ridge to the lowest point in the GPR transects) gives a loosely approximated slip rate of 1.2 mm/year, which is plausible for the area given the slip rate estimates [10] of up to 4 mm/year. The north-striking faults shown in Figure 5 roughly align with a Quaternary fault shown in Figure 2. The persistent discharge of hot water at the Mickey Springs site for at least 30,000 years may have started at fault tip transfer points on faults shown by J.S. Oldow (fide [15]; Figure 3) but became trapped in this location as faulting occurred on the north-striking, left-stepping normal faults.
The east-north-east-striking fault added to the map of J.S. Oldow (fide [15]) in Figure  20 follows the slope break between the main area of sinter mounds and broad depressions and the high-temperature area located at lower elevation. Slope-conforming sinter aprons  [15]) constrained the location of hydrothermal activity during cementation of sandstone and conglomerate unit (blue lines). All sinter at Mickey Springs is contained within this area. Development of a north-striking left-stepping fault before 30 kya offset the sandstone and further constrained the fluid pathways in the subsurface (orange lines). All sinter mounds and depressions are east of this fault. Most sinter mounds and all depressions are on a topographic bench between 1235 and 1240 m, which is bound to the south by a northeast-striking down to the south normal fault (red line). Elongate sinter aprons along this fault indicate it was present before or during sinter deposition. Currently, the majority of high-temperature springs are constrained in a 50 × 50 m area east of the left-stepping fault and south of the sinter mounds and depressions.
Reinterpretation of the east-dipping beds in the sandstone/conglomerate unit at the west edge of the area of sinter mounds from a delta front [2] to tilted fault blocks changed the age relations and structural interpretation of Mickey Springs. Taking the 30 kya TL age of the sediments that underlie sinter at Q4 as a minimum age for the sandstone/conglomerate unit, and a total fault offset of 35 m (from the highest point on the sandstone ridge to the lowest point in the GPR transects) gives a loosely approximated slip rate of 1.2 mm/year, which is plausible for the area given the slip rate estimates [10] of up to 4 mm/year. The north-striking faults shown in Figure 5 roughly align with a Quaternary fault shown in Figure 2. The persistent discharge of hot water at the Mickey Springs site for at least 30,000 years may have started at fault tip transfer points on faults shown by J.S. Oldow (fide [15]; Figure 3) but became trapped in this location as faulting occurred on the north-striking, left-stepping normal faults. The east-north-east-striking fault added to the map of J.S. Oldow (fide [15]) in Figure 20 follows the slope break between the main area of sinter mounds and broad depressions and the high-temperature area located at lower elevation. Slope-conforming sinter aprons at sinter mounds Q7, Q8, and Q10 ( Figure 5) suggest these vents were actively depositing sinter after displacement on the northeast-striking fault generated the topography. Sinter mound Q9 experienced explosive activity reported by Cummings and St. John [2] and between site visits in March and May, 2014 reported by Mowbray [5]. The alignment of four broad depressions (sinter-lined pools) along this trend ( Figure 5, D1, D2, D3, and D4) suggest additional faults of this orientation are present where the sinter mounds and broad depressions are concentrated. The parabolic patterns in GPR transects before topographic correction ( Figures S1-S4) are consistent with fault zones that serve as conduits for rising hot water.

Timeline of Deposits
A chronology of activity at Mickey Springs is presented in Figure 21. The earliest evidence of silica sinter deposition is clasts of basalt suspended in opaline silica in the sandstone/conglomerate unit. Sedimentary structures, petrified wood, fossils of vascular plants [2], and GPR profiles suggest the basalt-rich sand and gravel were locally sourced (probably Mickey Butte) and deposited on a relatively thin (~10 m) alluvial fan. This activity was occurring prior to 30 kya, but how long before is not known. The most intense silica cementation occurs immediately west of the main sinter mound area ( Figure 4). Less intense cementation occurs to the north-northwest and weakly to un-cemented sand and conglomerate forms of low hills immediately north of Mickey Springs on the uplifted side of the north-east-striking fault (Figure 4). Based on the distribution of cementation and sinter, the focus of hot spring activity prior to 30 kya was in the area near modern Mickey Springs. The faults along which hot water rose to the surface have not been identified. However, the conduits were likely controlled by the fault tip intersections of northeast-striking faults. Deformation on the left-stepping north-striking faults that separate the outcrops of the sandstone/conglomerate unit from the area underlain by sinter mounds and sinter-rimmed broad depressions occurred in rocks that had already been silica cemented. at sinter mounds Q7, Q8, and Q10 ( Figure 5) suggest these vents were actively depositing sinter after displacement on the northeast-striking fault generated the topography. Sinter mound Q9 experienced explosive activity reported by Cummings and St. John [2] and between site visits in March and May, 2014 reported by Mowbray [5]. The alignment of four broad depressions (sinter-lined pools) along this trend ( Figure 5, D1, D2, D3, and D4) suggest additional faults of this orientation are present where the sinter mounds and broad depressions are concentrated. The parabolic patterns in GPR transects before topographic correction (Figures S1-S4) are consistent with fault zones that serve as conduits for rising hot water.

Timeline of Deposits
A chronology of activity at Mickey Springs is presented in Figure 21. The earliest evidence of silica sinter deposition is clasts of basalt suspended in opaline silica in the sandstone/conglomerate unit. Sedimentary structures, petrified wood, fossils of vascular plants [2], and GPR profiles suggest the basalt-rich sand and gravel were locally sourced (probably Mickey Butte) and deposited on a relatively thin (~10 m) alluvial fan. This activity was occurring prior to 30 kya, but how long before is not known. The most intense silica cementation occurs immediately west of the main sinter mound area ( Figure 4). Less intense cementation occurs to the north-northwest and weakly to un-cemented sand and conglomerate forms of low hills immediately north of Mickey Springs on the uplifted side of the north-east-striking fault (Figure 4). Based on the distribution of cementation and sinter, the focus of hot spring activity prior to 30 kya was in the area near modern Mickey Springs. The faults along which hot water rose to the surface have not been identified. However, the conduits were likely controlled by the fault tip intersections of northeaststriking faults. Deformation on the left-stepping north-striking faults that separate the outcrops of the sandstone/conglomerate unit from the area underlain by sinter mounds and sinter-rimmed broad depressions occurred in rocks that had already been silica cemented. The lack of cementation in poorly sorted lithic-rich fluvial sediments that directly underlie sinter mounds may suggest a time when sinter was not being deposited or that The lack of cementation in poorly sorted lithic-rich fluvial sediments that directly underlie sinter mounds may suggest a time when sinter was not being deposited or that the vent walls were sealed by silica, preventing cementation in the surrounding sediment. At Borax Lake, the walls of the carrot-shaped~29-m-deep vent are lined by banded opaline silica, which separates easily eroded fine-grained material of the biomorphic mound from the turbulent waters in the vent [1- 3,59]. The sinter-rimmed broad depressions are interpreted as forming first. This is suggested by exposures in the walls of Q4, where gently dipping sinter layers interbedded with lithic-rich sand of an apron of a neighboring broad depression underlie more robust wavy sinter and pool-edge sinter of the Q4 sinter mound. The sinter mounds flank the sinter-rimmed broad depressions ( Figure 5).
Sinter deposition ceased prior to the onset of pluvial lake conditions. Late Pleistocene pluvial Lake Alvord began to fill as the climate warmed and melted glaciers on Steens Mountain. The lake eventually submerged Mickey Springs. When the elevation of the shoreline coincided with the elevation of the springs, wave action broke the sinter aprons, lodging blocks of sinter in the spring vents. As the depth of water increased, silt-and claysize sediment was deposited in the vents along with minor amounts of sand-size fragments of angular sinter. Most vents had ceased discharging water by this time. However, a few, such as Q4 and Q5, apparently were active while submerged in the lake and flushed the fine-grained sediment from their vents.
As the climate dried and the lake level dropped, wave action again broke blocks of sinter from the pool edges and scattered them on the now filled pool floors. The TL dates for silt-and clay-size sediment within the pools and overlying the sinter aprons are between 18 and 12 kya. The lake sediment was largely eroded either during the receding stage of the lake or by subsequent fluvial activity.
Since the drying of pluvial Lake Alvord, the locations of high-temperature springs, mud pots, and steam vents have emerged in their current location, probably in a zone of extension associated with the southern fault. However, low-volume warm springs are still active within the ancestral vents of the sinter mounds and sinter-rimmed broad depressions.

Conclusions
Hot springs have been active within a 4-hectare area at Mickey Springs for over 30,000 years and are localized at interacting fault tips of northeast-striking faults as proposed by Anderson and Fairley [15]. Left-stepping north-striking normal faults that separate the area of sinter mounds and broad depressions from the sinter-bearing sandstone/conglomerate unit may have localized up flow to a relatively small area. Movement on an east-northeast-striking normal fault within the area of sinter mounds (Q7, Q8, and Q10) occurred while sinter deposition was active and pre-dates the late Pleistocene rise of lake levels in pluvial Lake Alvord. Evidence of eruptions from the Q9 sinter mound in Figure 12 and [2] suggest this fault continues to be an active zone of up flow.
Silica sinter mounds and broad depressions at Mikey Springs were deposited after 30 kya but prior to late Pleistocene filling of pluvial Lake Alvord, starting at about 18 kya. Coeval deposition of silica sinter and conglomerate occurred before 30 kya, but the age is poorly constrained. The biomorphic mound and silica sinter deposits at Borax Lake in the Pueblo Valley were deposited during the Holocene after the drying of pluvial Lake Alvord [3].
Silica sinter at Mickey Springs is 1 to 2 m thick and overlies un-cemented lithic-rich sand (e.g., Q4, Figure 6). Sinter was no longer being deposited and most springs were inactive when Late Pleistocene water levels were rising in pluvial Lake Alvord. Spring vents and aprons were buried by silt-and clay-sized sediment sourced from melting glaciers on Steens Mountain. Clasts of sinter were buried by the fine-grained sediment. A few vents continued to be active and remained clear of sediments (e.g., Q4 and Q5).
The location of high-temperature springs shifted south to a 50 × 50 m area during the Holocene. Calcite deposition, starting where effluent in the outflow channel decreases to 73 • C, and geysering characterize a near-boiling spring. Eruptions from mud pots contributed to the construction of a 1.0-to 1.5-m-high berm. A TL date at 40 cm depth is 9.2 ± 1 kya. Sinter-free ejecta from a mud pot sometime between March and May 2014 indicates sinter is not present in the shallow subsurface.

Sample W4823
The temperature plateau comparison for this sample extended only between 275 and 350 • C due to low TL sensitivity. This resulted in widely scattered TL data and a larger than usual associated age uncertainty. The more easily reset electron trap level at a temperature of 325 • C was selected for this sample.
Sample W4828 The sample tube contained a large rock fragment occupying about 50% of the tube itself. This may have distorted the radiation flux received by the sample undergoing analysis and hence distorting the resultant TL age. If the fragment contains the same uranium, thorium, and potassium as the sediment, then no correction to the final age would be necessary.
Sample W4829 The sample consisted of a loose gritty sand with only a very few, if any, small pebbles. The TL output proved reasonable with a plateau comparison extending between 300 and 500 • C, lending confidence in the final depositional age determined.
Sample W4830 The sample exhibited a reasonable plateau comparison extending between 275 and 450 • C and similar TL sensitivity as Sample W4829. The ages of these two samples overlap at the one standard deviation level.
Sample W4831 TL sensitivity of this sample was low and there was a violent reaction when treated in hydrofluoric acid possibly due to a high feldspar content. The temperature comparison exhibited by the sample proved shortened and the resultant age of only 0.8 ka, the most recent of all samples analyzed but with a large associated age uncertainty.
Sample W4832 TL sensitivity of this sample proved low, and the TL data scattered, leading to a large associated TL age uncertainty.