Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE)

Details Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE) Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE)

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1915k&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1915

Physics

Scientific paper

n this study, using spectral image data of Multiband Imager (MI) onboard
Kaguya (SELENE), we estimate both thicknesses of mare basalt and lava
flow units in Mare Humorum.

Affiliated with

Also associated with

No associations

Rating

Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE) 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 Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Layering and Thickness of Basalitic Lava Flows in Mare Humorum: New Spectral Analysis of Multiband Imager Data of Kaguya (SELENE) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1205053