In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 122, No. 5 ( 2017-05), p. 800-821
Abstract:
Modeled lunar craters in the simple to complex regime to explore morphological outcomes Slow/large and fast/small impactors produce craters of same size but with different morphologies Progression from simple to complex structures is highly sensitive to the choice of acoustic fluidization constants
Type of Medium:
Online Resource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1002/2016JE005236
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2017
detail.hit.zdb_id:
1086497-0
detail.hit.zdb_id:
3094268-8
detail.hit.zdb_id:
2016810-X
SSG:
16,13