Journal ArticleDOI
The Hinode(Solar-B)Mission: An Overview
Takeo Kosugi,K. Matsuzaki,Taro Sakao,Toshifumi Shimizu,Y. Sone,Sumitaka Tachikawa,Tatsuaki Hashimoto,Kenji Minesugi,Akira Ohnishi,T. Yamada,Saku Tsuneta,Hirohisa Hara,Kiyoshi Ichimoto,Yoshinori Suematsu,Masumi Shimojo,Takashi Watanabe,Shigenobu Shimada,John M. Davis,L. D. Hill,J. K. Owens,A. M. Title,J. L. Culhane,Louise K. Harra,George A. Doschek,Leon Golub +24 more
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TLDR
The Hinode satellite as discussed by the authors is the successor to the Yohkoh mission, which aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases.Abstract:
The Hinode satellite (formerly Solar-B) of the Japan Aerospace Exploration Agency’s Institute of Space and Astronautical Science (ISAS/JAXA) was successfully launched in September 2006. As the successor to the Yohkoh mission, it aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases. Hinode is an observatory style mission, with all the instruments being designed and built to work together to address the science aims. There are three instruments onboard: the Solar Optical Telescope (SOT), the EUV Imaging Spectrometer (EIS), and the X-Ray Telescope (XRT). This paper provides an overview of the mission, detailing the satellite, the scientific payload, and operations. It will conclude with discussions on how the international science community can participate in the analysis of the mission data.read more
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Journal ArticleDOI
Observations and simulations of longitudinal oscillations of an active region prominence
TL;DR: In this article, a multi-wavelength data analysis of the active region prominence oscillations above the western limb on 2007 February 8 was carried out and a one-dimensional hydrodynamic simulation of the longitudinal oscillations was performed.
Journal ArticleDOI
Morphology, dynamics and plasma parameters of plumes and inter-plume regions in solar coronal holes
Klaus Wilhelm,Lucia Abbo,Frederic Auchere,Nicolas Barbey,Li Feng,Alan H. Gabriel,Silvio Giordano,Shinsuke Imada,Antoine Llebaria,William H. Matthaeus,Giannina Poletto,N.-E. Raouafi,Steven T. Suess,Luca Teriaca,Y. M. Wang +14 more
TL;DR: In this paper, the structure and dynamics of coronal plumes and inter-plume regions in solar coronal holes were investigated. But the authors did not provide a detailed analysis of the plume generation process and its interaction with the solar wind.
Journal ArticleDOI
The Solar Internetwork. I. Contribution to the Network Magnetic Flux
TL;DR: In this article, the authors investigated the contribution of internetwork magnetic fields to the NE flux and found that 14% of the quiet Sun flux is in the form of IN fields with little temporal variations.
Journal ArticleDOI
Observations of a rotating macrospicule associated with an X-ray jet
TL;DR: In this paper, the authors studied the dynamics of a macrospicule and an associated coronal jet captured by multi-spacecraft observations using EIS and SUMER spectra.
Journal ArticleDOI
On the continuum intensity distribution of the solar photosphere
TL;DR: In this paper, a detailed comparison between simulations and seeing-free observations that takes into account the crucial influence of instrumental image degradation is presented, where images of quiet Sun granulation taken in the blue, green and red continuum bands of the SOT onboard Hinode are deconvolved with Point Spread Functions (PSF) that account for non-ideal contributions due to instrumental stray-light and imperfections.
References
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A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection
TL;DR: In this paper, the authors identify the reconnection region as the site of particle acceleration, suggesting that the basic physics of the magnetic reconnection process may be common to both types of flares.
Journal ArticleDOI
Sigmoidal morphology and eruptive solar activity
TL;DR: In this paper, the authors studied the Yohkoh Soft X-Ray Telescope video movie for 1993 and 1997 and found that regions are significantly more likely to be eruptive if they are either sigmoidal or large.
Journal ArticleDOI
Hot-Plasma Ejections Associated with Compact-Loop Solar Flares
Kazunari Shibata,Satoshi Masuda,Masumi Shimojo,Hirohisa Hara,Takaaki Yokoyama,Saku Tsuneta,Takeo Kosugi,Y. Ogawara +7 more
TL;DR: In this article, the authors search for plasma ejections in eight impulsive compact-loop flares near the limb, which are selected in an unbiased manner and include also the Masuda flare, 1992 January 13 flare.
Journal ArticleDOI
Statistical Study of Solar X-Ray Jets Observed with the YOHKOH Soft X-Ray Telescope
TL;DR: In this article, a statistical study of 100 X-ray jets, found from the database of full Sun images taken with the Soft X-Ray Telescope (SXT) aboard Yohkoh during the period between November 1991 and April 1992, was conducted.
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