In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 122, No. 10 ( 2017-10)
Kurzfassung:
Deuterium Lyman alpha brightness in the upper atmosphere of Mars is highly variable, peaking just after southern summer solstice Martian limb D brightness varies on timescales that are similar to those of water vapor variations lower in the atmosphere Deuterium variability may be due to seasonal factors such as regional dust storm activity and subsequent lower atmospheric circulation
Materialart:
Online-Ressource
ISSN:
2169-9380
,
2169-9402
DOI:
10.1002/jgra.v122.10
DOI:
10.1002/2017JA024666
Sprache:
Englisch
Verlag:
American Geophysical Union (AGU)
Publikationsdatum:
2017
ZDB Id:
2033040-6
ZDB Id:
161665-1
ZDB Id:
3094181-7
SSG:
16,13