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Autor:
Orger, Necmi Cihan, Rodrigo, Cordova Alarcon Jose, Anh, Minh Pham, Kim, Sangkyun, Kitamura, Kentaro, Teramoto, Mariko, Nakayama, Daisuke, Kishimoto, Makiko, Nishinaga, Kounosuke, Oboshi, Akihiro, Sawa, Kenta, Masui, Hirokazu, Sano, Kei, Toyoda, Kazuhiro, Cho, Mengu
Lunar horizon glow (LHG) has been seen as an excessive brightness to be monitored in order to estimate the abundance of the exospheric dust grains near the lunar terminator. Monitoring the LHG could reveal critical information on the dust particles n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::ab12c64d79b800488b642e3b562e3117
https://kyutech.repo.nii.ac.jp/records/7929
https://kyutech.repo.nii.ac.jp/records/7929