R
Richard A. Shine
Researcher at Advanced Technology Center
Publications - 82
Citations - 7880
Richard A. Shine is an academic researcher from Advanced Technology Center. The author has contributed to research in topics: Sunspot & Photosphere. The author has an hindex of 42, co-authored 82 publications receiving 7524 citations. Previous affiliations of Richard A. Shine include Japan Aerospace Exploration Agency & National Institute of Standards and Technology.
Papers
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Journal ArticleDOI
The transition region and coronal explorer
B. N. Handy,Loren W. Acton,Charles C. Kankelborg,C. J. Wolfson,D. J. Akin,Marilyn E. Bruner,R. Caravalho,R.C. Catura,Roger A. Chevalier,Dexter W. Duncan,Christopher G. Edwards,C.N. Feinstein,Samuel L. Freeland,Frank M. Friedlaender,C. Hoffmann,Neal E. Hurlburt,B. Jurcevich,N. Katz,G. A. Kelly,James R. Lemen,M. Levay,R.W. Lindgren,D. Mathur,S.B. Meyer,S.J. Morrison,M. Morrison,R. W. Nightingale,T.P. Pope,R. Rehse,Carolus J. Schrijver,Richard A. Shine,L. Shing,Keith T. Strong,Theodore D. Tarbell,Alan M. Title,D. D. Torgerson,Leon Golub,Jay A. Bookbinder,David Caldwell,Peter Cheimets,William N. Davis,Edward E. DeLuca,R. A. McMullen,Harry P. Warren,D. Amato,Richard R. Fisher,H. Maldonado,C. Parkinson +47 more
TL;DR: In this paper, a contract for the development and flight of an experiment to study the solar atmosphere with excellent spatial and temporal resolution; and reduction and analysis of the resultant data is presented.
Journal ArticleDOI
Initial Calibration of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)
Paul Boerner,Christopher G. Edwards,James R. Lemen,A. Rausch,Carolus J. Schrijver,Richard A. Shine,L. Shing,Robert A. Stern,Theodore D. Tarbell,Alan M. Title,C. Jacob Wolfson,Regina Soufli,Eberhard Spiller,Eric M. Gullikson,David E. McKenzie,David L. Windt,Leon Golub,William A. Podgorski,Paola Testa,M. A. Weber +19 more
TL;DR: The Atmospheric Imaging Assembly (AIA) instrument onboard the Solar Dynamics Observatory (SDO) is an array of four normal-incidence reflecting telescopes that image the Sun in ten EUV and UV wavelength channels as mentioned in this paper.
Journal ArticleDOI
A Tale of Two Spicules: The Impact of Spicules on the Magnetic Chromosphere
Bart De Pontieu,Scott W. McIntosh,Scott W. McIntosh,Viggo Hansteen,Mats Carlsson,Carolus J. Schrijver,Theodore D. Tarbell,Alan M. Title,Richard A. Shine,Y. Suematsu,Saku Tsuneta,Yukio Katsukawa,Kiyoshi Ichimoto,Toshifumi Shimizu,Shin’ichi Nagata +14 more
TL;DR: In this article, high-resolution observations of the Sun in Ca II H (3968A) from the Solar Optical Telescope on Hinode were used to show that there are at least two types of spicules that dominate the structure of the magnetic solar chromosphere.
Journal ArticleDOI
Chromospheric Anemone Jets as Evidence of Ubiquitous Reconnection
Kazunari Shibata,Tahei Nakamura,Takuma Matsumoto,Kenichi Otsuji,Takenori J. Okamoto,N. Nishizuka,T. Kawate,Hiroko Watanabe,Shin’ichi Nagata,Satoru Ueno,Reizaburo Kitai,Satoshi Nozawa,Saku Tsuneta,Yoshinori Suematsu,Kiyoshi Ichimoto,Toshifumi Shimizu,Yukio Katsukawa,Theodore D. Tarbell,Thomas E. Berger,Bruce W. Lites,Richard A. Shine,Alan M. Title +21 more
TL;DR: Hinode observations of chromospheric anemone jets suggest that magnetic reconnection similar to that in the corona is occurring at a much smaller spatial scale throughout the chromosphere, and suggest that the heating of the solar chromosphere and corona may be related to small-scale ubiquitous reconnection.
Journal ArticleDOI
Polarization Calibration of the Solar Optical Telescope onboard Hinode
Kiyoshi Ichimoto,Bruce W. Lites,D. F. Elmore,Yoshinori Suematsu,Saku Tsuneta,Yukio Katsukawa,Toshifumi Shimizu,Richard A. Shine,Theodore D. Tarbell,Alan M. Title,J. Kiyohara,Kazuya Shinoda,G. Card,Alice R. Lecinski,K. V. Streander,Masao Nakagiri,Masakuni Miyashita,M. Noguchi,C. Hoffmann,T. Cruz +19 more
TL;DR: The solar optical telescope (SOT) onboard Hinode aims to obtain vector magnetic fields on the Sun through precise spectropolarimetry of solar spectral lines with a spatial resolution of 0.2 -0.3 arcsec as discussed by the authors.