Zobrazeno 1 - 10
of 43
pro vyhledávání: '"B. R. Dennis"'
Autor:
E P, Kontar, J E, Perez, L K, Harra, A A, Kuznetsov, A G, Emslie, N L S, Jeffrey, N H, Bian, B R, Dennis
Publikováno v:
Physical review letters. 118(15)
The energy released in solar flares derives from a reconfiguration of magnetic fields to a lower energy state, and is manifested in several forms, including bulk kinetic energy of the coronal mass ejection, acceleration of electrons and ions, and enh
Autor:
L. Fletcher, B. R. Dennis, H. S. Hudson, S. Krucker, K. Phillips, A. Veronig, M. Battaglia, L. Bone, A. Caspi, Q. Chen, P. Gallagher, P. T. Grigis, H. Ji, W. Liu, R. O. Milligan, M. Temmer
Publikováno v:
Space Science Reviews. 159:19-106
We present an overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era. Following an introductory discussion and overview of the status of observational capabilities, the article
Autor:
Thomas R. Metcalf, Markus J. Aschwanden, Säm Krucker, André Csillaghy, G. J. Hurford, David M. Smith, J. Sato, Richard A. Schwartz, B. R. Dennis, J. M. McTiernan, Edward J. Schmahl, Christopher M. Johns-Krull, A. J. Conway, Robert P. Lin
Publikováno v:
Solar Physics. 210:61-86
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) observes solar hard X-rays and gamma-rays from 3 keV to 17 MeV with spatial resolution as high as 2.3 arc sec. Instead of focusing optics, imaging is based on nine rotating modulation
Publikováno v:
High-Energy Aspects of Solar Flares ISBN: 9781461430728
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::172907539d73f8e168958105f45c72a2
https://doi.org/10.1007/978-1-4614-3073-5_2
https://doi.org/10.1007/978-1-4614-3073-5_2
Publikováno v:
Lecture Notes in Physics ISBN: 9783540552468
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d548e40a9a656c32c21cb0f8c760ee13
https://doi.org/10.1007/3-540-55246-4_90
https://doi.org/10.1007/3-540-55246-4_90
Autor:
Peter T. Gallagher, G. M. Mason, Terry G. Forbes, Gerald H. Share, Thomas R. Metcalf, Angelos Vourlidas, Nat Gopalswamy, B. R. Dennis, Ronald J. Murphy, Richard A. Schwartz, A. G. Emslie, Harald Kucharek, Gordon D. Holman, Thomas H. Zurbuchen, R. A. Mewaldt
Publikováno v:
Journal of Geophysical Research. 109
Using coordinated observations from instruments on the Advanced Composition Explorer (ACE), the Solar and Heliospheric Observatory (SOHO), and the Ramaty High Energy Solar Spectroscopic Imager (RHESSI), we have evaluated the energetics of two well-ob
Autor:
G. J. Hurford, E. J. Schmahl, R. A. Schwartz, A. J. Conway, M. J. Aschwanden, A. Csillaghy, B. R. Dennis, C. Johns-Krull, S. Krucker, R. P. Lin, J. Mctiernan, T. R. Metcalf, J. Sato, D. M. Smith
Publikováno v:
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) ISBN: 9789048162123
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3c8444389018b873ae31d6a9b4316e29
https://doi.org/10.1007/978-94-017-3452-3_3
https://doi.org/10.1007/978-94-017-3452-3_3
Autor:
R. P. Lin, B. R. Dennis, G. J. Hurford, D. M. Smith, A. Zehnder, P. R. Harvey, D. W. Curtis, D. Pankow, P. Turin, M. Bester, A. Csillaghy, M. Lewis, N. Madden, H. F. van Beek, M. Appleby, T. Raudorf, J. Mctiernan, R. Ramaty, E. Schmahl, R. Schwartz, S. Krucker, R. Abiad, T. Quinn, P. Berg, M. Hashii, R. Sterling, R. Jackson, R. Pratt, R. D. Campbell, D. Malone, D. Landis, C. P. Barrington-Leigh, S. Slassi-Sennou, C. Cork, D. Clark, D. Amato, L. Orwig, R. Boyle, I. S. Banks, K. Shirey, A. K. Tolbert, D. Zarro, F. Snow, K. Thomsen, R. Henneck, A. Mchedlishvili, P. Ming, M. Fivian, John Jordan, Richard Wanner, Jerry Crubb, J. Preble, M. Matranga, A. Benz, H. Hudson, R. C. Canfield, G. D. Holman, C. Crannell, T. Kosugi, A. G. Emslie, N. Vilmer, J. C. Brown, C. Johns-Krull, M. Aschwanden, T. Metcalf, A. Conway
Publikováno v:
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) ISBN: 9789048162123
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d1bf277682d3d5328eefba6f2e70eb4b
https://doi.org/10.1007/978-94-017-3452-3_1
https://doi.org/10.1007/978-94-017-3452-3_1
Publikováno v:
The Astrophysical Journal
We compare four different methods of calculating uncertainty estimates in fitting parameterized models to RHESSI X-ray spectra, considering only statistical sources of error. Three of the four methods are based on estimating the scale-size of the min
Autor:
R. Starr, J. I. Trombka, B. R. Dennis, M. H. Acuna, L. E. Orwig, T. L. Cline, Upendra D. Desai
Publikováno v:
AIP Conference Proceedings.
Two new missions will be launched in 1996 and 1997, each carrying X-ray and gamma ray detectors capable of high spectral resolution at room temperature. The Argentine Satelite de Aplicaciones Cientificas (SAC-B) and the Small Spacecraft Technology In