In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 123, No. 2 ( 2018-02), p. 322-334
Abstract:
Boulder halos form on surfaces with a high abundance of shallow subsurface ice and suggest ice‐rich mantles tens of meters thick Abundant halos in the north and rare halos in the south are attributed to differences in surface processes, not differences in substrate Boulder halos persist through multiple orbitally controlled ice deposition events and are persistent feature of Martian high latitudes
Type of Medium:
Online Resource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1002/2017JE005470
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2018
detail.hit.zdb_id:
1086497-0
detail.hit.zdb_id:
3094268-8
detail.hit.zdb_id:
2016810-X
SSG:
16,13