Japan Geoscience Union Meeting 2014

Presentation information

International Session (Poster)

Symbol P (Space and Planetary Sciences) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM08_2PO1] Space Weather and Space Climate

Fri. May 2, 2014 4:15 PM - 5:30 PM Poster (3F)

Convener:*Kataoka Ryuho(National Institute of Polar Research), Yusuke Ebihara(Research Institute for Sustainable Humanosphere, Kyoto University), Kanya Kusano Kanya(Solar-Terrestrial Environment Laboratory, Nagoya University), Toshifumi Shimizu(Institute of Space and Astronautical Science, JAXA), Yoshizumi Miyoshi(Solar-Terrestrial Environement Laboratory, Nagoya University), Ayumi Asai(Unit for Synergetic Studies of Space, Kyoto University), Tatsuhiko Sato(Japan Atomic Energy Agency), Hidekatsu Jin(National Institude of Information and Communications Technology), Kiminori Itoh(Graduate School of Engineering, Yokohama National University), Hiroko Miyahara(College of Art and Design, Musashino Art University)

4:15 PM - 5:30 PM

[PEM08-P04] Solar cell degradation of Akebono satellite due to space radiation and effect of temperature variation

*Wataru MIYAKE1, Yoshizumi MIYOSHI2, Ayako MATSUOKA3 (1.Tokai University, 2.Solar Terrestrial Environment Laboratory, Nagoya University, 3.Institute of Space and Astronautical Science)

Keywords:Akebono satellite, proton radiation belt

Solar cells on any satellite degrade gradually due to severe space radiation environment. We have analyzed the degradation of the solar cells of the Akebono satellite, and found a fair correlation between the decrease rate of the solar cell output current and the trapped proton flux between 1989 and 1996. The previous studies demonstrated that we can deduce information of proton radiation belt from degradation of solar cells of the Akebono satellite. The relationship cannot be discernible after 1996. The previous studies suggested more prominent temperature effect in the later years because of progress of the degradation. In order to expand studies by using solar cells as a radiation monitor, we must separate exactly the contribution of temperature and of proton radiation. Since the sensor for solar cell temperature failed in 1991 and no temperature is available after 1991, we try to model the temperature variation at solar cells from the temperature of other surface parts. Once we establish the method, we correlate the temperature with solar cell output current and deduce the contribution of proton radiation.