Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Iizima, Masahide"'
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics 2006 68(12):1340-1351
Publikováno v:
Journal of Plasma and Fusion Research SERIES. 8:165-168
資料番号: SA1001038000
Autor:
Suzuki, Tomonori, Ono, Takayuki, Iizima, Masahide, Uemoto, Jyunpei, Kumamoto, Atsushi, Nishimura, Yukitoshi, Wakabayashi, Makoto
Publikováno v:
スペース・プラズマ研究会: 平成19年度 = Proceedings of Space Plasma Conference FY2007. :40-43
平成19年度スペースプラズマ研究会 (2008年3月27日-28日. 宇宙航空研究開発機構宇宙科学研究本部(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県
Space Plasma Conference FY2007 (March 27-28, 2008. I
Space Plasma Conference FY2007 (March 27-28, 2008. I
Publikováno v:
Advances in polar upper atmosphere research. 20:27-37
Solar zenith angle and solar activity dependences of electron number density in the nightside auroral region from the topside ionosphere to the magnetosphere within a geocentric radial distance of 2.6 R_E were statistically investigated based on anal
Publikováno v:
Advances in polar upper atmosphere research. 19:10-20
Seasonal and solar cycle dependences of the correlation between auroral kilometric radiation (AKR) and the auroral electrojet (AE) index have been investigated based on the plasma wave data obtained by the Akebono satellite. Under any seasonal and so
Publikováno v:
Advances in polar upper atmosphere research. 17:60-76
Plasma wave phenomena associated with sudden commencements (SCs) were analyzed using the database of Akebono satellite observations that has been contributed to for more than 13 years, since March 1989. The plasma wave data from 263 satellite passage
Publikováno v:
Advances in polar upper atmosphere research. 17:146-154
The second harmonic wave properties of auroral kilometric radiation(AKR) were examined using data obtained by the Akebono satellite. The results of our statistical analysis indicate that the probability of a harmonic event occurrence is more than 60%
Publikováno v:
Advances in polar upper atmosphere research. 17:48-59
Solar cycle variations of auroral kilometric radiation (AKR) observed by the Akebono satellite have been compared with the variations of F10.7 and solar wind dynamic pressure. F10.7 and solar wind dynamic pressure show different solar cycle variation
Autor:
Kitamura, Naritoshi, Nishimura, Yukitoshi, Ono, Takayuki, Kumamoto, Atsushi, Shinbori, Atsuki, Iizima, Masahide, Matsuoka, Ayako, Hairston, M. R.
Publikováno v:
Journal of Geophysical Research. A: Space Physics. 115
Accepted: 2010-03-15
資料番号: SA1001044000
資料番号: SA1001044000
Publikováno v:
Journal of Geophysical Research. A: Space Physics. 115
Accepted: 2009-09-02
資料番号: SA1001041000
資料番号: SA1001041000