Faculty Profiles - MASUDA, Satoshi

Papers - MASUDA, Satoshi

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Coronal electron distribution in solar flares: drift kinetic model Reviewed

Minoshima, T., S. Masuda, Y. Miyoshi, and K. Kusano

Astrophys. J. Vol. 732 page： 111-117 2011.5

Magnetic Transport on the Solar Atmosphere by Laminar and Turbulent Ambipolar Diffusion Reviewed

Hiraki,Y., V. Krishan, and S. Masuda

Astrophys. J. Vol. 720 page： 1311-1317 2010.9

Trans-equatorial Loop System Comes from Coronal Hole Boundary through Interactions between Active Region and Coronal Hole Reviewed

Yokoyama, M. and S. Masuda

Solar Physics Vol. 263 page： 135-152 2010.5

Measurements of the Coronal Acceleration Region of a Solar Flare Reviewed

Krucker S., H. S. Hudson, L. Glesener, S. M. White, S. Masuda, J.-P. Wuelser, and R. P. Lin

Astrophys. J. Vol. 714 page： 1108-1119 2010.5

G-band and Hard X-ray emissions of the 2006 December 14 Flare Observed by Hinode/SOT and RHESSI Reviewed

Watanabe, K., S. Krucker, T. Shimizu, S. Masuda, and K. Ichimoto

Astrophys. J. Vol. 715 page： 651-655 2010.5

Drift-Kinetic Modeling of Particle Acceleration and Transport in Solar Flares Reviewed

Minoshima, T., S. Masuda, and Y. Miyoshi

Astrophys. J. Vol. 714 page： 332-342 2010.5

*Formation Mechanism of Soft X-ray Transient Trans-Equatorial Loop System Reviewed

Yokoyama, M. and S. Masuda

Solar Phys. Vol. 254 page： 285-296 2009

The Focusing Optics X-ray Solar Imager (FOXSI) Reviewed

Krucker, S., S. Christe, L. Glesener, S. McBride, P. Turin, D. Glaser, P. Saint-Hilaire, G. Delory, R. P. Lin, M. Gubarev, B. Ramsey, Y. Terada, S. Ishikawa, M. Kokubun, S. Saito, T. Takahashi, S. Watanabe, K. Nakazawa, H. Tajima, S. Masuda, T. Minoshima, and M. Shomojo

Proc. SPIE Vol. 7437 page： 743705 2009

Multi-Wavelength Observation of Electron Acceleration in the 2006 December 13 Flare Reviewed

Minoshima T., S. Imada, T. Morimoto, T. Kawate, H. Koshiishi, M. Kubo, S. Inoue, H. Isobe, S. Masuda, S. Krucker, and T. Yokoyama

Astrophys. J. Vol. 697 page： 843-849 2009

Imaging Spectroscopy on Preflare Coronal Nonthermal Sources Reviewed

Asai, A., H. Nakajima, M. Shimojo, T. Yokoyama, S. Masuda, and S. Krucker

Astrophys. J. Vol. 695 page： 1623-1630 2009

Magnetic Transport On The Solar Atmosphere By Turbulent Ambipolar Diffusion Reviewed

Krishan, V. and S. Masuda

Asian Journal of Physics Vol. 17 page： 479-488 2008

*Looptop impulsive hard X-ray source in solar flares observed with Yohkoh/HXT Invited Reviewed

Masuda, S.

Asian Journal of Physics Vol. 17 page： 411-421 2008

Three-Dimensional Structure Analysis of Coronal Magnetic Field in AR NOAA 10930 Based on Vector Magnetogram Observations with Hinode/SOT Reviewed

Inoue, S., K. Kusano, S. Masuda, T. Miyoshi, T. Yamamoto, T. Magara, S. Tsuneta, T. Sakurai, T. Yokoyama, and the US/Japan SOT team

ASP conference series Vol. 397 page： 110 2008

*Hard X-ray emission from the solar corona Reviewed

Krucker, S., M. Battaglia, P. J. Cargill, L. Fletcher, H. S. Hudson, A. L. MacKinnon, S. Mausda, L. Sui, M. Tomczak, A. M. Veronig, L. Vlahos, and S. M. White

Astron. and Astrophys. Review Vol. 16 page： 155-208 2008

Detection of High-Energy Solar Neutrons and Protons by Ground Level Detec tors on April 15 Reviewed

Muraki, Y., Y. Matsubara, S. Masuda, S. Sakakibara, T. Sako, K. Watanabe, R. Buetikofer, E. O. Flueckiger, A. Chilingarian, G. Hovsepyan, F. Kakimoto, T. Terasawa, Y. Tsunesada, H. Tokuno, A. Velarde, P. Evenson, J. Poirier, and T. Sakai

Astroparticle Physics Vol. 29 page： 229-242 2008

Evolution of H-alpha Kernels and Energy Release in an X-Class Flare Reviewed

Asai, A., T. Yokoyama, M. Shimojo, S. Masuda, and K. Shibata

ASP Conference Series Vol. 369 page： 461-468 2007

Imaging Spectroscopy of a Gradual Hardening Flare on 2000 November 25 Reviewed

Takasaki, H., J. Kiyohara, A. Asai, H. Nakajima, T. Yokoyama, S. Masuda, J. Sato, and T. Kosugi

Astrophysical Journal Vol. 661 page： 1234-1241 2007

*Micro-Type-III Radio Bursts Reviewed

Morioka, A., Y. Miyoshi, S. Masuda, F. Tsuchiya, H. Misawa, H. Matsumoto, K. Hashimoto, and H. Oya

Astrophys. J. Vol. 657 page： 567-576 2007

Language：English Publishing type：Research paper (scientific journal)

We present a detailed description of the features of solar "micro–type III" radio bursts, which are elements of the so-called type III storms, using long-term observations made by the Geotail and Akebono satellites. Micro–type III bursts are characterized by short-lived, continuous, and weak emission. Their average power is estimated to be well below that of the largest type III bursts, by 6 orders of magnitude. When they occur, these bursts have a distribution of emitted power flux that is different from that of ordinary type III bursts, indicating that they are not just weaker versions of the ordinary bursts. Micro–type III burst activity is not accompanied by significant solar soft X-ray activity. We identify the active regions responsible for micro–type III bursts by examining the concurrence of their development and decay with the bursts. It is found that both micro and ordinary type III bursts can emanate from the same active region without interference, indicating the coexistence of independent electron acceleration processes. It is suggested that the active regions responsible for micro–type III bursts generally border on coronal holes.

A solar neutron telescope in Tibet and its capability examined by the 1998 November 28th event Reviewed

Muraki, Y., H. Tsuchiya, K. Fujiki, S. Masuda, Y. Matsubara, H. Menjo, T. Sako, K. Watanabe, M. Ohnishi, A. Shiomi, M. Takita, T. Yuda, Y. katayose, N. Hotta, S. Ozawa, T. Sakurai, Y. H. Tan, and J. L. Zhang

Astroparticle Physics Vol. 28 page： 119-131 2007

Flare Ribbon Expansion and Energy Release Reviewed

Asai, A., T. Yokoyama, M. Shimojo, S. Masuda, and K. Shibata

Journal of Astrophysics and Astronomy Vol. 27 page： 167-173 2006

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Papers - MASUDA, Satoshi