New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust

Details New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1599b&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1599

Physics

Scientific paper

We present a mapping of slope streaks using HRSC data at Olympus Mons
aureole. We argue from these data that slope streaks are a dry-granular
avalanche which can be triggered by the accumulation of dust at hill
crests in the downstream side of the wind flow.

Affiliated with

Also associated with

No associations

Rating

New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New Insights for the Formation of Slope Streaks on Mars from a Systematic Mapping Using Mars Express HRSC Data: A Dry Granular Avalanche Controlled by Wind-Transported Dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1355824