Zobrazeno 1 - 10
of 96
pro vyhledávání: '"MORIOKA, Akira"'
Autor:
Iwai, Kazumasa, Miyoshi, Yoshizumi, Masuda, Satoshi, Tsuchiya, Fuminori, Morioka, Akira, Misawa, Hiroaki
The fine spectral structures of solar radio type-I bursts were observed by the solar radio telescope AMATERAS. The spectral characteristics, such as the peak flux, duration, and bandwidth, of the individual burst elements were satisfactorily detected
Externí odkaz:
http://arxiv.org/abs/1405.0708
Autor:
Nakamura, Yuki, Kasaba, Yasumasa, Kimura, Tomoki, Lamy, Laurent, Cecconi, Baptiste, Fischer, Georg, Sasaki, Ayumu, Tao, Chihiro, Tsuchiya, Fuminori, Misawa, Hiroaki, Kumamoto, Atsushi, Morioka, Akira
Publikováno v:
In Planetary and Space Science 15 November 2019 178
Publikováno v:
In Planetary and Space Science 2008 56(15):1967-1976
Investigation of local time dependence of Mercury's sodium exosphere based on a numerical simulation
Publikováno v:
In Planetary and Space Science 2008 56(13):1681-1687
Publikováno v:
In Planetary and Space Science 2008 56(8):1155-1168
Autor:
Morioka, Akira, Miyoshi, Yoshizumi, Kurita, Satoshi, Kasaba, Yasumasa, Angelopoulos, Vassilis, Misawa, Hiroaki, Kojima, Hirotsugu, McFadden, James P.
Publikováno v:
Journal of Geophysical Research: Space Physics. 118(3):1123-1131
Auroral kilometric radiation (AKR) is known to be transient emissions generated by rapidly accelerated electrons together with sudden auroral activation in the polar magnetosphere. In contrast, the characteristics and relationship with the auroral ac
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :25-28
For the purpose of confirming the plasma condition of the topside ionosphere, we have investigated spectra of Jupiter's radio emissions observed with the Cassini spacecraft to derive the Faraday rotation for the period of Cassini's Jupiter swing-by a
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :45-48
Saturn's outer magnetosphere is considered to be one of sources of auroral particles, inducing the complex interaction between magnetospheric particles and Titan. In 1980s, Voyager 1 and 2 had revealed the existence of high energy (approximately keV)
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :33-36
The Jovian Synchrotron Radiation (JSR) is a radio wave emitted from the relativistic electrons in the Jovian radiation belt, which has information of dynamics of high-energy particles and electromagnetic disturbances in the Jovian inner magnetosphere
Autor:
Imai, Kota, Misawa, Hiroaki, Tsuchiya, Fuminori, Morioka, Akira, Watanabe, Takuo, Kudo, Riichi
Publikováno v:
第39回月・惑星シンポジウム = Proceedings of the 39th ISAS Lunar and Planetary Symposium. :37-40
We have made regular observations of the Jovian Synchrotron Radiation (JSR) with the Iitate Planetary Radio Telescope (IPRT) at 325 MHz since 2003. As a further project of IPRT, we have developed a new dual frequency receiver system which enables sim