Regolith thickness over Sinus Iridum: Results from morphology and size-frequency distribution of small impact craters-Reference-Cited by-同舟云学术

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Regolith thickness over Sinus Iridum: Results from morphology and size-frequency distribution of small impact craters

Published:2014-08 Issue:8 Volume:119 Page:1914-1935
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Fa Wenzhe¹,Liu Tiantian¹,Zhu Meng-Hua²,Haruyama Junichi³

Affiliation:

1. Institute of Remote Sensing and Geographical Information System; Peking University; Beijing China

2. Space Science Institute; Macau University of Science and Technology; Macau China

3. Institute of Space and Astronautical Science; Japan Aerospace Exploration Agency; Sagamihara Japan

Funder

National Natural Science Foundation

Key Research Program

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference35 articles.

1. Global survey of lunar regolith depths from LROC images;Bart;Icarus,2011

2. Compositional and temporal investigation of exposed lunar basalts in the Mare Imbrium region;Bugiolacchi;Icarus,2008

3. Geologic investigation and mapping of the Sinus Iridum quadrangle from Clementine, SELENE, and Chang'E-1 data;Chen;Sci. Chin. Phys. Mech. Astron.,2010

4. Simulation for ground penetrating radar (GPR) study of the subsurface structure of the Moon;Fa;J. Appl. Geophys.,2013

5. A primary analysis of microwave brightness temperature of lunar surface from Chang-E 1 multi-channel radiometer observation and inversion of regolith layer thickness;Fa;Icarus,2010

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