Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations

Details Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1742b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1742

Physics

Scientific paper

We report on the late summer evolution of the the NPLD. We used CRISM
data to identify an increase in VNIR albedo that we attribute to a
decrease in ice grain size from L_s = 132-167 in MY28. MARCI data
indicate this is not likely due to clouds or dust.

Affiliated with

Also associated with

No associations

Rating

Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations 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 Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Water Ice Grain Size Evolution on Martian North Polar Residual Layered Deposits for Late Summer MY28 AND 30 from CRISM/MARCI Observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1037366