Zobrazeno 1 - 10
of 81
pro vyhledávání: '"T. D. Tarbell"'
Autor:
Frédéric Auchère, Andrei Zhukov, Vincenzo Andretta, Louise K. Harra, Sami K. Solanki, Yukio Katsukawa, Kiyoshi Ichimoto, Shinsuke Imada, Luca Teriaca, Giampiero Naletto, Shin Toriumi, Tomoko Kawate, Takaaki Yokoyama, Hirohisa Hara, T. D. Tarbell, Harry P. Warren, Masahito Kubo, Yoshinori Suematsu, Toshifumi Shimizu, Sarah A. Matthews, Udo Schühle, Tetsuya Watanabe, Andrzej Fludra, Bart De Pontieu, Clarence M. Korendyke
Publikováno v:
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXI.
Solar-C EUVST (EUV High-Throughput Spectroscopic Telescope) is a solar physics mission concept that was selected as a candidate for JAXA competitive M-class missions in July 2018. The onboard science instrument, EUVST, is an EUV spectrometer with sli
Autor:
Carolus J. Schrijver, T. D. Tarbell, Viggo Hansteen, A. M. Title, Paul Boerner, B. De Pontieu, Scott W. McIntosh, Juan Martinez-Sykora, Mats Carlsson
Publikováno v:
Science. 331:55-58
The Sun's outer atmosphere, or corona, is heated to millions of degrees, considerably hotter than its surface or photosphere. Explanations for this enigma typically invoke the deposition in the corona of nonthermal energy generated by magnetoconvecti
Publikováno v:
Solar Physics. 267:75-94
We study dynamics of quiescent prominences using several data sets taken with the Solar Optical Telescope (SOT) on Hinode. We find a number of processes occurring at different stages of prominence evolution that are common for all of our chosen cases
Autor:
Takenori J. Okamoto, Z. Frank, R. A. Shine, A. M. Title, Thomas E. Berger, M. Kubo, T. D. Tarbell, Bruce W. Lites, Kenichi Otsuji
Publikováno v:
The Astrophysical Journal. 718:474-487
We present comprehensive observations of the formation and evolution of a filament channel within NOAA Active Region (AR) 10978 from Hinode/Solar Optical Telescope and TRACE. We employ sequences of Hinode spectro-polarimeter maps of the AR, accompany
Publikováno v:
The Astrophysical Journal. 859:121
We analyze and discuss an example of prominence barbs observed on the limb on 2016 January 7 by the Hinode/Solar Optical Telescope in Ca II and H alpha, the Interface Region Imaging Spectrograph, with slit jaw images and Mg II spectral data, and the
Autor:
R. A. Shine, T. D. Tarbell, M. Nagase, Kazuhide Kodeki, Shin Nagata, Yoshinori Suematsu, Christopher G. Edwards, Kiyoshi Ichimoto, E. Thomas, Toshifumi Shimizu, Osamu Ito, K. Kobayashi, S. Sour, Masaki Tabata, Saku Tsuneta, Yasuhiro Kashiwagi, R. Rehse, K. Matsuzaki, C. Hoffmann
Publikováno v:
Solar Physics. 249:221-232
The Hinode Solar Optical Telescope (SOT) is the first space-borne visible-light telescope that enables us to observe magnetic-field dynamics in the solar lower atmosphere with 0.2 – 0.3 arcsec spatial resolution under extremely stable (seeing-free)
Publikováno v:
Solar Physics. 243:87-92
All of the Hinode telemetry data are to be reformatted and archived in the DARTS system at ISAS and mirrored to data centers around the word. The archived data are distributed to users through the Internet. This paper gives an overview of the files i
Publikováno v:
The Astrophysical Journal. 641:1197-1209
We exploit a rare joint set of high-resolution, very high cadence TRACE UV images and high-resolution magnetograms from SOHO MDI to investigate the dynamical properties of flare ribbons in a GOES M1 class flare from NOAA active region 9236 on 2000 No
Autor:
L. Golub, Juan Martinez-Sykora, Lucia Kleint, Sean McKillop, Viggo Hansteen, Neal E. Hurlburt, Hardi Peter, B. De Pontieu, M. P. Miralles, Patrick I. McCauley, Steven H. Saar, James R. Lemen, Paola Testa, Scott W. McIntosh, Mats Carlsson, Katharine K. Reeves, Paul Boerner, Steven R. Cranmer, Edward E. DeLuca, S. Jaeggli, Jean-Pierre Wuelser, T. D. Tarbell, Hui Tian, M. Weber, Nicholas A. Murphy, A. M. Title, Charles C. Kankelborg
Publikováno v:
Science
As the interface between the Sun's photosphere and corona, the chromosphere and transition region play a key role in the formation and acceleration of the solar wind. Observations from the Interface Region Imaging Spectrograph reveal the prevalence o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea3be15272bef986b4d9f4230a928d68
http://arxiv.org/abs/1410.6143
http://arxiv.org/abs/1410.6143
Autor:
A. M. Title, Charles C. Kankelborg, Fabio Reale, James R. Lemen, Edward E. DeLuca, Paola Testa, Katharine K. Reeves, Jean-Pierre Wuelser, Sean McKillop, Steven H. Saar, Mats Carlsson, Joel C. Allred, S. Jaeggli, B. De Pontieu, Wei Liu, Neal E. Hurlburt, Viggo Hansteen, Paul Boerner, Lucia Kleint, Adrian N. Daw, Juan Martinez-Sykora, L. Golub, T. D. Tarbell, Hui Tian
Publikováno v:
Science
The physical processes causing energy exchange between the Sun's hot corona and its cool lower atmosphere remain poorly understood. The chromosphere and transition region (TR) form an interface region between the surface and the corona that is highly