Next Article in Journal
A SHDAViT-MCA Block-Based Network for Remote-Sensing Semantic Change Detection
Previous Article in Journal
Air–Sea Interaction During Ocean Frontal Passage: A Case Study from the Northern South China Sea
 
 
Search for Articles:
Title / Keyword
Author / Affiliation / Email
Journal
Article Type
 
 
Advanced Search
 
Section
Special Issue
Volume
Issue
Number
Page
 
Journals
Remote Sensing
Volume 17
Issue 17
10.3390/rs17173025
remotesensing-logo
Submit to this Journal Review for this Journal Propose a Special Issue
► Article Menu

Article Menu

share Share announcement Help format_quote Cite question_answer Discuss in SciProfiles
Correction to Remote Sens. 2022, 14(24), 6326.
first_page
settings
Order Article Reprints
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Correction

Correction: O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326

by
James O’Donoghue
1,* and
Tom Stallard
2
1
Department of Solar System Science, JAXA Institute of Space and Astronautical Science, Sagamihara 252-5210, Japan
2
Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle-upon-Tyne NE1 8ST, UK
*
Author to whom correspondence should be addressed.
Remote Sens. 2025, 17(17), 3025; https://doi.org/10.3390/rs17173025
Submission received: 30 July 2025 / Accepted: 30 July 2025 / Published: 1 September 2025
Versions Notes

Error in Figure

In the original publication [1], there was a mistake in Figure 2 as published. The H2 density profile in the Uranus panel and H2 and H profiles in the Neptune panel were incorrectly retrieved from the literature. This is now corrected in the figure below, and all other neutral and ion species were checked to confirm that no other similar mistakes were made. In addition, the X-axis numbering was made denser so that the values in the figure are easier to read; specifically, the tick mark spacing is now spaced to display every two orders of magnitude, instead of every three. The corrected Figure 2 appears below. The authors state that the scientific conclusions are unaffected. This correction was approved by the Academic Editor. The original publication has also been updated.
Remotesensing 17 03025 i001

Reference

  1. O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326. [Google Scholar] [CrossRef]
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content.

Share and Cite

MDPI and ACS Style

O’Donoghue, J.; Stallard, T. Correction: O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326. Remote Sens. 2025, 17, 3025. https://doi.org/10.3390/rs17173025

AMA Style

O’Donoghue J, Stallard T. Correction: O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326. Remote Sensing. 2025; 17(17):3025. https://doi.org/10.3390/rs17173025

Chicago/Turabian Style

O’Donoghue, James, and Tom Stallard. 2025. "Correction: O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326" Remote Sensing 17, no. 17: 3025. https://doi.org/10.3390/rs17173025

APA Style

O’Donoghue, J., & Stallard, T. (2025). Correction: O’Donoghue, J.; Stallard, T. What the Upper Atmospheres of Giant Planets Reveal. Remote Sens. 2022, 14, 6326. Remote Sensing, 17(17), 3025. https://doi.org/10.3390/rs17173025

Note that from the first issue of 2016, this journal uses article numbers instead of page numbers. See further details here.

Article Metrics

Back to TopTop