@inproceedings{oai:jaxa.repo.nii.ac.jp:00005047,
 author = {川中, 宣太 and 加藤, 成晃 and 嶺重, 慎 and Kawanaka, Norita and Kato, Yoshiaki and Mineshige, Shin},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, In explaining the spectral properties of active galactic nuclei (AGNs) and X-ray binaries, it is often assumed that they consists of a geometrically thin, optically thick disk and hot, optically thin corona surrounding the thin disk. As for a model of a corona, we adopt the simulation data of three-dimensional MHD accretion flows, while for a thin disk we assume a standard disk. We perform Monte Carlo radiative transfer simulations in the corona, taking into account the Compton scattering of the soft photons from the thin disk by hot thermal electrons. We can reproduce the emergent spectra which are consistent with those of typical Seyfert galaxies, and we also find the rapid time variability in X-ray emission spectra, originating from the density fluctuation in the corona., Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574115, レポート番号: JAXA-SP-09-008E},
 pages = {304--305},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Theoretical Interpretation of X-ray Spectra from Active Galactic Nuclei and Low/Hard State of X-ray Binaries with an Accretion Disk-Corona Model},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}