In:
Geophysical Research Letters, American Geophysical Union (AGU), Vol. 49, No. 18 ( 2022-09-28)
Abstract:
Emirates Ultraviolet Spectrometer (EMUS) observations provide large scale, high cadence, synoptic views of carbon monoxide (CO) relative column abundance in the lower thermosphere of Mars Significant variability in CO brightness and relative column abundance is regularly observed in EMUS disk images Observed variability of CO relative column abundance in local time, latitude, and solar longitude is inconsistent with model predictions
Type of Medium:
Online Resource
ISSN:
0094-8276
,
1944-8007
DOI:
10.1029/2022GL099615
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2022
detail.hit.zdb_id:
2021599-X
detail.hit.zdb_id:
7403-2
SSG:
16,13