1. Introduction
To acquire high-quality images from high-resolution observation satellites with sub-meter accuracy, it is essential to isolate microvibrations generated by disturbance sources, including on-board payloads of satellites featuring mechanical moving parts [
1]. Cryogenic coolers of the pulse-tube type have been extensively employed in space applications to cool the focal planes of infrared imaging sensors, offering benefits such as simplicity, cost-efficiency, enhanced reliability, and reduced mechanical vibrations compared to traditional Stirling-type coolers [
2,
3,
4]. However, this cooler also generates undesirable microvibrations during on-orbit operation, which can significantly impact the performance of microvibration-sensitive payloads on observation satellites. Future space missions, such as high-precision terrestrial and celestial observation satellites, demand stricter microvibration requirements, and effective microvibration isolation has become essential for such cooler systems. To prevent image quality degradation, one effective approach is to incorporate a vibration isolator to attenuate microvibrations transmitted to microvibration-sensitive on-board payloads.
The microvibration of the cooler can be effectively mitigated by separating its operating frequency from the natural frequency of the cooler assembly using a vibration isolator. Passive vibration isolation systems represent an effective strategy for vibration mitigation, distinguished by their robustness, simplicity, and reliability [
5,
6,
7,
8,
9,
10,
11,
12,
13,
14]. Several types of passive vibration isolation systems have been proposed in previous studies. Ellis et al. [
5] proposed a vibration isolator using a commercial wire rope that supports a cryocooler system on a cube satellite. A wire rope isolator can be readily integrated with minimal modifications to the cryocooler, effectively attenuating the microvibrations generated by the cryocooler. Richard et al. [
6] introduced a hexagonal vibration isolator featuring low stiffness intended to support spaceborne coolers. Microvibration measurement tests were conducted to validate the system design. The test results demonstrated that the vibration isolator achieved a 20 dB attenuation of harmonic disturbances generated by the cooler. Riabzev et al. [
7] designed a passive multidimensional vibration isolator that incorporates a coil spring with low lateral stiffness, utilizing a three-stage spring-mass system affixed to the cold tip of a cryogenic cooler. The effectiveness of the isolation system was assessed experimentally in conjunction with analytical models. To support micro-vibration isolation of cryogenic coolers, Kamesh et al. [
8] proposed a variety of flexible passive vibration isolators, including struts with different thicknesses and bending properties, adopting a frequency decoupling approach between the operational frequency of the cooler and the natural frequency of the isolation system. Takei et al. [
9] proposed a passive two-stage type vibration isolator intended for the cryogenic cooler of the ASTRO-H satellite. The system includes a launch vibration isolator with a cast viscoelastic bumper and an on-orbit isolator characterized by metal bending properties. It offers broadband jitter isolation during on-orbit operations and reduces vibration loads in the launch environment. The effectiveness of this design was confirmed using both numerical analyses and experimental methods. Takuma et al. [
10] proposed a flux-pinned passive microvibration isolator for applications in cryogenic cooling. This mechanism leverages flux pinning to passively sustain the relative distance and position between a permanent magnet and a cooled type-II superconductor, facilitated by the flux pinning force. The isolator’s characteristics, including spring and damping coefficients, were analyzed using a numerical model. Yang et al. [
11] proposed a passive vibration isolator comprising a double-deck leaf spring filled with silicone rubber, specifically designed for space optical payloads. This design minimizes stress on the leaf-type springs while enhancing the damping coefficient, thereby improving its effectiveness in attenuating vibrations within the optical payload. The effectiveness of the vibration isolator was validated through dynamic modeling, finite element analysis (FEA), and experimental testing, with results confirming the validity of the analytical approach and demonstrating efficient attenuation of spaceborne disturbances. Robinson et al. [
12] developed a soft mount featuring a low-stiffness passive vibration isolation system, which employs metallic flexures and viscoelastic damping materials for a Thermal Infrared Sensor (TIRS) cryogenic cooler. The stiffness of the metallic flexures was calibrated to ensure that the rigid-body mode of the TIRS cooler mounted on the flexures fell within the range of 9 to 30 Hz, leading to a tenfold improvement in vibration isolation performance. Kwon et al. [
13] introduced a superelastic shape memory alloy (SMA) blade-type vibration isolator that effectively provided the desired jitter isolation performance under both 0 g and 1 g conditions. This isolator ensures the structural integrity of the cooler assembly without necessitating an additional launch locking system, even under severe launch vibration conditions, and effectively isolates microvibrations of the cooler in the orbital environment. The results of position sensitivity tests indicated that the isolator could maintain stable jitter isolation performance, even under the influence of 1 g. Kwon et al. [
14] introduced a multilayered blade-type isolator utilizing double-sided adhesive tape to mitigate microjitter generated by cryogenic coolers in space applications. The isolator’s insensitivity to positional variations enables consistent jitter reduction performance. Furthermore, the efficacy of this design, which does not require additional launch locks, was validated through qualification-level launch vibration tests. The experimental results demonstrated that the system achieved an isolation performance of 20 dB against harmonic disturbances produced by the cooler.
In passive isolators, the use of low-stiffness components facilitates the decoupling of the cooler’s primary operating frequency from the natural frequency of the supported cooler assembly, thereby effectively reducing microvibrations. However, the structural integrity of coolers utilizing low-stiffness isolators may be insufficient to withstand the harsh conditions of the launch environment. This challenge could be addressed by integrating a hold-and-release mechanism for the cooler assembly during launch. However, this solution adds complexity to the system and increases overall mass. If the hold-and-release mechanism fails to disengage the mechanical constraints of the isolation system in orbit, the isolator may not ensure adequate performance, potentially leading to degradation of the optical system’s functionality.
To address these challenges, Oh et al. [
15] developed a passive launch and on-orbit vibration isolation system (PLOVIS-I) with space heritage as part of the KOMPSAT-3A program [
16]. PLOVIS-I effectively mitigates microvibrations from a cryogenic cooler in both launch and orbital environments, removing the necessity for an additional hold-and-release mechanism. The system achieves effective microvibration isolation through the use of three coil springs characterized by comparatively low lateral stiffness. However, position sensitivity tests indicated a normalized transmitted force ratio of 4.52 between 0 g and 1 g, suggesting that the isolation performance is significantly influenced by the precise alignment of the isolator, which is critical for optimal functioning. It is noteworthy that Oh et al. [
15] did not assess the position sensitivity of the conventional PLOVIS-I. Additionally, vibration tests conducted to evaluate the design’s effectiveness at the qualification level for launch conditions demonstrated that PLOVIS-I was insufficient for attenuating sine vibration loads due to the inadequate damping properties of the coil springs, even though the maximum acceleration experienced by the cooler remained within its design limit load.
In view of the position sensitivity of the conventional PLOVIS-I, Park et al. [
17] proposed a dual coil-spring-type passive vibration isolation system (PLOVIS-II) that exhibited improved performance in isolating micro-vibrations and the attenuation of launch vibration loads. PLOVIS-II uses coil springs with low stiffness to isolate the microjitter during on-orbit operation and coil springs with relatively higher stiffness to attenuate the launch vibration loads. The key features of PLOVIS-II are its low sensitivity to the alignment position of the isolator and reduced launch vibrations compared to the conventional PLOVIS-I. The effectiveness of the design was validated through microvibration isolation and launch environment vibration tests. Although position sensitivity was measured with respect to the aligned position of the isolator, the sensitivity was only investigated for the main excitation frequency of the cooler in a previous study [
17]. Coolers generally generate harmonic vibrations that are coupled with their main driving frequency. Therefore, for the thermal control of the cooler, it is essential to analyze the effects of dynamic coupling with the elastic vibration modes of the structure that supports the cooler, including the heat pipes. This implies that the dynamic characteristics of vibration isolators are required to be in a much wider frequency range.
In this study, to measure the force transmissibility characteristics of PLOVIS-II under 0 g simulation conditions over the frequency range from 50 Hz to 250 Hz, a test method using a non-contact-type vibration exciter consisting of a voice coil and permanent magnet was proposed and investigated. The position sensitivities of PLOVIS-II and PLOVIS-I were compared. According to the test results obtained, the dual-coil spring-type isolator of PLOVIS-II showed lower sensitivity to the aligned position of the isolation system than that shown by PLOVIS-I with a single-coil spring.
The organization of the remaining sections of this paper is as follows:
Section 2 provides an overview of previous studies on PLOVIS-II, including the results of the design and validation tests.
Section 3 and
Section 4 present the design of the force transmissibility tests and the results of the on-ground force transmissibility testing, including position sensitivity tests.
3. Experimental Setup of the Force Transmissibility Test for PLOVIS-II
To verify the effectiveness of PLOVIS-II in terms of improving microvibration isolation, taking into account the harmonic vibration characteristics of the cooler, a force transmissibility test was conducted using a 4 kg dummy cooler with PLOVIS-II. The test setup mainly consisted of a noncontact vibration exciter and a microvibration measurement system, as shown in
Figure 7. In this test, a noncontact vibration exciter was used to realize the multiaxis excitation of a dummy cooler, which is only possible with single-axis excitation (
y-axis) using a linear motor, and to overcome the difficulty in realizing the actual boundary conditions of the cooler when using a contact vibration exciter. A noncontact vibration exciter consisting of a voice coil and permanent magnet was used to simulate the microvibration characteristics of a pulse-tube-type cooler. Here, a counter mass for the permanent magnet is used to prevent the center of gravity from shifting of the dummy cooler because the magnet is directly mounted on the cooler itself. The excitation force was amplified to 5 N using a power amplifier at an excitation frequency of 50–250 Hz generated by a function generator. These frequency ranges were established to evaluate the microvibration isolation performance compared with the harmonic vibration characteristics described above. An accelerometer was mounted at the C.G (Center of Gravity) of the dummy cooler to measure the excitation force. The disturbance force transmitted from the dummy cooler to the base plate was assessed using a microvibration measurement system, which incorporated three-axis load cells (MC15-3A-100, DACELL Co., Ltd., Cheongju., Republic of Korea., 4 units). A 1 g compensation device with a rubber-type wire was applied to the dummy cooler to simulate a 0 g condition where the dummy cooler remained in the nominal position of PLOVIS-II. Using the test setup, the force transmissibility (
FT) of the cooler assembly with PLOVIS-II is expressed as follows:
where
F0 is the measured excitation force of the cooler, and
Ft is the force transmitted to the base plate.
Figure 8 shows the sequential procedure followed during the force transmissibility measurement of the PLOVIS-II isolator. Following the experimental setup described in
Figure 7, an excitation signal was generated by the function generator, amplified by the power amplifier, and applied to the dummy cooler through the non-contact vibration exciter. The excitation force and the transmitted force were simultaneously measured by the accelerometer and the microvibration measurement table, respectively. All signals were collected via the data acquisition system (DAQ) and subsequently processed to calculate the force transmissibility. This flowchart provides a clear visualization of the experimental steps undertaken to ensure the repeatability and reliability of the measurement process.
Figure 9a–c show the cooler assembly configuration of the test setup with PLOVIS-II along the
x-,
y-, and
z-axes. The
x-axis test was performed using an additional bracket that allowed the cooler to be excited along the
x-axis. The test configuration for PLOVIS-I was identical to that of PLOVIS-II.
4. Force Transmissibility Test Results of PLOVIS-II
The basic characteristics of force transmissibility for PLOVIS-II were derived using the test setup described above. A position sensitivity test was conducted to evaluate the microvibration-isolation performance when the dummy cooler was shifted from the nominal position of the vibration isolator. The vibration isolator exhibited absolute isolation performance when the dummy cooler remained in the nominal position; this guaranteed vibration isolation performance. However, if the cooler shifts from its nominal position owing to an unexpected misalignment or thermal deformation of the heat pipes integrated into the cooler to transfer heat from the cooler, there is a possibility that the vibration isolation performance can be degraded. In practice, it is difficult to precisely align a cooler integrated with a heat pipe and transfer line at the nominal position of the vibration isolator, which is necessary for obtaining optimal vibration isolation performance. Therefore, to reduce the potential risk to system reliability, we considered using an isolation system with less position-sensitive characteristics. The alignment requirements of the IR sensor module integration and heat pipe for maintaining the desired vibration isolation performance were also derived from the test.
In the test, a forced translational displacement was applied to shift the cooler position along the representative gravity axis (
x-axis). The test was conducted by shifting the dummy cooler in 0.75 mm and 1.5 mm increments, because it was difficult to perform the test with increments smaller than 0.75 mm due to the limitations of the test setup. In addition, the vibration isolation performance variation of the position sensitivity was clearly distinguishable, even with 0.75 mm increments. The test cases for measuring the force transmissibility of the cooler assembly with PLOVIS-I and PLOVIS-II were defined as follows: (A) under a simulated 0 g condition; (B) and (C) enforced displacements of 0.75 and 1.5 mm, respectively, applied to the cooler; (D) under a 1 g condition, where a static force of 37.24 N was applied along the gravitational direction as a result of the cooler’s mass. In case (A), the dummy cooler was positioned at the nominal position of the isolator using a 1 g compensation device, where the desired vibration isolation performance could be guaranteed, as shown in
Figure 10a.
Figure 10b shows a representative configuration of Case (C), in which the cooler was shifted from the nominal position of the vibration isolator to simulate the conditions in Cases (B) and (C). It should be noted that the tolerances for the cooler alignment of PLOVIS-I and PLOVIS-II were 1.5 and 1.2 mm, respectively, resulting in different support conditions for Case (C). This means that the dummy cooler with PLOVIS-II is supported by a moving plate with a 0.3 mm compressed high-stiffness coil spring, unlike PLOVIS-I, which contacts a displacement limiter. Case (D) represented an unexpected condition for on-orbit operation; however, it was included to qualitatively assess the microvibration isolation performance when the dummy cooler deviated from the low-stiffness range for the reasons previously mentioned. In such a case, without a 1 g compensation device, the coil springs with low stiffness used in PLOVIS-I and PLOVIS-II were extended and compressed by the weight of the cooler assembly. However, the two vibration isolators have different mechanical support configurations. For example, as shown in
Figure 10c, a moving plate combined with high-stiffness coil springs supports the dummy cooler with PLOVIS-II under the 1 g condition. However, the cooler with PLOVIS-I is in direct contact with the displacement limiter integrated into the support structure, as shown in
Figure 10d.
Figure 11 shows the test results for Case (A) for the
x-,
y-, and
z-axes. As can be seen, both vibration isolators have almost the same force transmissibility characteristics under the 0 g condition because both vibration isolators support the dummy cooler with the same low-stiffness configuration. The force transmissibility of PLOVIS-I and PLOVIS-II at the main excitation frequency of the cooler of 50 Hz were less than 0.05 for all axes, indicating that the microvibration level of 5 N for the dummy cooler was remarkably reduced by a factor of 25. This value closely corresponds to the value (23) predicted from the transmissibility curve of the isolation system, which has a natural frequency of 8 Hz, derived using a one-degree-of-freedom mathematical model [
17]. Moreover, because of the frequency-decoupling strategy adopted in the vibration isolator design, the disturbances as well as force transmissibility were effectively reduced in the high-frequency region on all the axes.
Figure 12a and
Figure 12b show the position sensitivity test results for Cases (B) and (C) along the
x-,
y-, and
z-axes, respectively. The test results for the force transmissibility test from 50 to 250 Hz showed that the force transmissibility increased when the cooler assembly shifted from the nominally aligned position of the vibration isolator. Both vibration isolators showed almost the same test results in Case (A) because they had similar support conditions for the low-stiffness coil springs. However, in Case (C), the force transmissibility of PLOVIS-II was approximately 1.3 times lower than that of PLOVIS-I in all excitation frequency ranges because of the different support conditions. This minimizes the high-frequency harmonic disturbances associated with the coupling to the structural modes of the cooler assembly, leading to an improvement in vibration isolation performance. This indicates that the PLOVIS-II designs supported by high-stiffness springs exhibited better microvibration reduction in terms of position sensitivity.
Figure 13 shows the test results for Case (D) for the
x-,
y-, and
z-axes. The force transmissibility characteristic of PLOVIS-II for all axes under the 1 g condition was more than 1.6 times lower than that of PLOVIS-I in all frequency ranges. This is because the cooler was supported by a moving plate with high-stiffness coil springs, unlike PLOVIS-I, where microvibrations from the cooler were directly transmitted to the base plate via the support structure.
These test results indicate that PLOVIS-II has a lower tolerance for cooler alignment compared to PLOVIS-I. Further, unlike PLOVIS-I, PLOVIS-II has unsusceptible position sensitivity, as intended by its design, even when operated under severe and unexpected conditions during on-orbit operation. Therefore, the proposed PLOVIS-II is effective in relaxing the strict heat pipe and infrared detector alignment requirements, which is desirable for reducing potential risks when considering system reliability.