Introduction of RSTAR Model for Akatsuki Data Analysis

George HASHIMOTO; Miho Sekiguchi; Takao M. Sato; Makiko Hashimoto; Seiko Takagi; Naohiro Manago; Takashi Nakajima; Teruyuki Nakajima; Takehiko Satoh

Presentation information

[EE] Oral

P (Space and Planetary Sciences) » P-PS Planetary Sciences

[P-PS04] Results from Akatsuki and advances in Venus science

Tue. May 22, 2018 10:45 AM - 12:15 PM A01 (Tokyo Bay Makuhari Hall)

convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Takeshi Horinouchi(Faculty of Environmental Earth Science, Hokkaido University), Masaru Yamamoto(九州大学応用力学研究所, 共同), Kevin McGouldrick(University of Colorado Boulder), Chairperson:Horinouchi Takeshi, Satoh Takehiko

11:10 AM - 11:25 AM

[PPS04-07] Introduction of RSTAR Model for Akatsuki Data Analysis

*George HASHIMOTO¹, Miho Sekiguchi², Takao M. Sato³, Makiko Hashimoto³, Seiko Takagi⁴, Naohiro Manago³, Takashi Nakajima⁵, Teruyuki Nakajima³, Takehiko Satoh³ (1.Department of Earth Sciences, Okayama University, 2.Tokyo University of Marine Science and Technology, 3.JAXA, 4.Hokkaido University, 5.Tokai University)

Keywords:Akatsuki, radiative transfer

RSTAR7-Akatsuki is a package for calculating the radiance observed by cameras onboard Akatsuki. Libraries are provided to users under the condition that they are used only for non-profit scientific or educational purposes (OpenCLASTR project http://157.82.240.167/~clastr/). Now we are ready to calculate the radiance observed by IR1, IR2, and LIR.