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pro vyhledávání: '"Takeo Kosugi"'
Autor:
A. Nishida
Publikováno v:
Space Research Today. 168:46
Akademický článek
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Autor:
Nishida, A.
Publikováno v:
Space Research Today; Apr2007, Vol. 168, p46-46, 1p
Publikováno v:
Solar Physics. Jun2007, Vol. 243 Issue 1, p1-2. 2p. 1 Color Photograph.
Autor:
Aschwanden, Markus
Publikováno v:
Space Science Reviews; January 1999, Vol. 87 Issue: 3-4 p539-540, 2p
Autor:
Masumi Shimojo, George A. Doschek, Takashi Watanabe, Sumitaka Tachikawa, Kiyoshi Ichimoto, L. D. Hill, Taro Sakao, Kenji Minesugi, Leon Golub, Shigenobu Shimada, Louise K. Harra, Yoshinori Suematsu, Akira Ohnishi, Tatsuaki Hashimoto, Y. Sone, Hirohisa Hara, T. Yamada, Saku Tsuneta, Toshifumi Shimizu, A. M. Title, J. L. Culhane, Takeo Kosugi, John M. Davis, K. Matsuzaki, J. K. Owens
Publikováno v:
Solar Physics. 243:3-17
著者人数:25名
Accepted: 2007-07-30
資料番号: SA1000203000
Accepted: 2007-07-30
資料番号: SA1000203000
Autor:
Satoshi Masuda, Junko Kiyohara, J. Sato, Hiroyuki Takasaki, Ayumi Asai, Takaaki Yokoyama, Takeo Kosugi, Hiroshi Nakajima
Publikováno v:
The Astrophysical Journal. 661:1234-1241
We present an examination of multiwavelength observations of an M8.2 long-duration flare which occurred on 2000 November 25. During the flare, we can see a hard X-ray (HXR) source on one Hα flare ribbon in the HXR images obtained with the Hard X-ray
Autor:
L. Bradley, R. Hagood, Charles M. Brown, Roger J. Thomas, B. M. Shaughnessy, David L. Windt, Clarence M. Korendyke, J. Lang, K. Matsuzaki, Takashi Watanabe, Rifat A Chaudry, S. Mahmoud, M. C. R. Whillock, C. M. Castelli, John F. Seely, J. T. Mariska, Viggo Hansteen, John Shea, George A. Doschek, Takeo Kosugi, P. D. Thomas, Kenneth P. Dere, Brian J. Probyn, H. Mapson-Menard, S. H. Myers, K. Al-Janabi, J. L. Culhane, G. M. Simnett, J. Tandy, B. J. Kent, Kerrin Rees, Hirohisa Hara, A. M. James, Ø. Wikstol, Peter R. Young, Joseph M. Davila, Berend Winter, Robert W. Moye, Louise K. Harra
Publikováno v:
Solar Physics. 243:19-61
The EUV Imaging Spectrometer (EIS) on Hinode will observe solar corona and upper transition region emission lines in the wavelength ranges 170 – 210 A and 250 – 290 A. The line centroid positions and profile widths will allow plasma velocities an
Autor:
Keiji Yoshimura, Anita Joshi, Rajmal Jain, Takeo Kosugi, Wahab Uddin, M. R. Deshpande, Taro Sakao, Ramesh Chandra
Publikováno v:
Solar Physics. 239:239-256
We present the H$\alpha$ observations from ARIES, Nainital of a compact and impulsive solar flare occurred on March 10, 2001 and associated with a CME. We have also analysed HXT, SXT/Yohkoh observations as well as radio observations from Nobeyama Rad
Autor:
Takeo Kosugi, Yukari Matsumoto, Satoshi Masuda, M. Sawa, J. Sato, Keiji Yoshimura, J. Kotoku, Tetsuya Watanabe, S. Kubo, K. Suga, Masato Yoshimori
Publikováno v:
Solar Physics. 236:351-368
The flare catalogue of the Yohkoh mission is compiled and linked to this article as an electronic supplement. For showing flare characteristics over wide energy range concisely, we provide the images of Hard X-ray Telescope (HXT) and the Soft X-ray T