In:
Journal of Geophysical Research: Space Physics, American Geophysical Union (AGU), Vol. 122, No. 3 ( 2017-03), p. 3815-3836
Abstract:
Photochemical O escape fluxes from dissociative recombination of O 2 + are calculated from MAVEN in situ data Escape rates of 1.2 to 5.5 × 10 25 s −1 are derived and depend on season, solar zenith angle, and EUV flux, consistent with previous models We find a power law exponent of 2.6 for the EUV dependence of escape rate, implying 100 s of mbar of oxygen loss over 3.5 Gyr
Type of Medium:
Online Resource
ISSN:
2169-9380
,
2169-9402
DOI:
10.1002/2016JA023525
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2017
detail.hit.zdb_id:
2033040-6
detail.hit.zdb_id:
161665-1
detail.hit.zdb_id:
3094181-7
SSG:
16,13
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