MAVEN SEP Observations of Scorpius X‐1 X‐Rays at Mars: A Midatmosphere Occultation Analysis Technique
Author:
Affiliation:
1. Space Sciences Laboratory University of California Berkeley CA USA
2. Department of Physics and Astronomy University of Kansas Lawrence KS USA
Funder
National Aeronautics and Space Administration
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020GL088927
Reference40 articles.
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4. Extensive MRO CRISM observations of 1.27μm O2airglow in Mars polar night and their comparison to MRO MCS temperature profiles and LMD GCM simulations
5. Variability of D and H in the Martian upper atmosphere observed with the MAVEN IUVS echelle channel
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2. Precision Ephemerides for Gravitational-wave Searches – IV. Corrected and refined ephemeris for Scorpius X-1;Monthly Notices of the Royal Astronomical Society;2023-02-02
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4. High-Resolution X-Ray Spectroscopy of Supernova Remnants;High-Resolution X-ray Spectroscopy;2023
5. Methods of Planetary Atmospheric Density Retrieval Based on X-ray Occultation;Chinese Journal of Space Science;2023
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