Research Project
Grant-in-Aid for Young Scientists (B)
Toward the realization of the "backside illuminated type CMOS detector" necessary for constructing a "photon-counting imaging type" solar X-ray telescope capable of directly observing the particle acceleration region considered to be present in the solar corona, we performed a study to estimate the performance required for this detector from previous observations. We analyzed limb flares observed by the Hinode/EIS that observes extreme ultraviolet close to soft X-rays that can be observed the acceleration region. However, there is only one flare event that observed near the acceleration region, and which was already reported in other paper (Imada et al., 2013) . Therefore, we estimated the intensity of accelerated particles during solar flares statistically by using other flare radiation (white-light, hard X-ray, ultraviolet), and obtained the flare characteristics at the time of particle acceleration.
All 2018 2017 2016 2015
All Journal Article (15 results) (of which Int'l Joint Research: 10 results, Peer Reviewed: 7 results, Open Access: 2 results, Acknowledgement Compliant: 2 results) Presentation (20 results) (of which Int'l Joint Research: 13 results, Invited: 4 results)
The Astrophysical Journal
Volume: 850 Issue: 2 Pages: 204-204
10.3847/1538-4357/aa9659
Volume: 851 Issue: 2 Pages: 91-91
10.3847/1538-4357/aa9b34
Memoirs of the National Defence Academy of Japan
Volume: 55 Pages: 9-16
120006358374
Proceedings of the 35th International Cosmic Ray Conference (ICRC2017)
Volume: 150
Volume: 136
Volume: 103
Volume: 101
Volume: 53
Volume: 52
Volume: 51
Volume: 836 Issue: 2 Pages: 150-150
10.3847/1538-4357/aa5b8b
Publications of the Astronomical Society of Japan
Volume: 69 Issue: 1 Pages: 7-7
10.1093/pasj/psw111
Solar Physics
Volume: 291 Issue: 4 Pages: 1241-1265
10.1007/s11207-016-0887-0
Advances in Space Research
Volume: 58 Issue: 10 Pages: 2018-2025
10.1016/j.asr.2016.02.008
第59回宇宙科学技術連合講演会論文集
Volume: OS6
40020617202
