D
David M. Smith
Researcher at University of California, Santa Cruz
Publications - 355
Citations - 19484
David M. Smith is an academic researcher from University of California, Santa Cruz. The author has contributed to research in topics: Solar flare & Terrestrial gamma-ray flash. The author has an hindex of 60, co-authored 354 publications receiving 17870 citations. Previous affiliations of David M. Smith include University of St Andrews & Veterans Health Administration.
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Journal ArticleDOI
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (Rhessi)
Robert P. Lin,Brian R. Dennis,G. J. Hurford,David M. Smith,Alex Zehnder,Peter Harvey,D. W. Curtis,David H. Pankow,Paul Turin,Manfred Bester,André Csillaghy,M. Lewis,Norman W. Madden,H. F. van Beek,M. Appleby,T. Raudorf,J. M. McTiernan,Reuven Ramaty,E. J. Schmahl,Richard A. Schwartz,Säm Krucker,R. Abiad,T. Quinn,Peter Berg,M. Hashii,R. Sterling,R. Jackson,R. Pratt,Robert Campbell,D. Malone,D. Landis,Christopher Barrington-Leigh,S. Slassi-Sennou,C.P. Cork,David C. Clark,D. Amato,Larry E. Orwig,Robert F. Boyle,I. S. Banks,K. Shirey,Anne K. Tolbert,Dominic M. Zarro,Frank Snow,Knud Thomsen,Reinhold Henneck,A. Mchedlishvili,P. Ming,M. D. Fivian,John Jordan,Richard Wanner,Jerry Crubb,J. Preble,M. Matranga,Arnold O. Benz,Hugh S. Hudson,Richard C. Canfield,Gordon D. Holman,Carol Jo Crannell,Takeo Kosugi,A. G. Emslie,N. Vilmer,John C. Brown,Christopher M. Johns-Krull,Markus J. Aschwanden,Thomas R. Metcalf,A. J. Conway +65 more
TL;DR: RHESSI as discussed by the authors is a Principal Investigator (PI) mission, where the PI is responsible for all aspects of the mission except the launch vehicle, and is designed to investigate particle acceleration and energy release in solar flares, through imaging and spectroscopy of hard X-ray/gamma-ray continua emitted by energetic electrons, and of gamma-ray lines produced by energetic ions.
Journal ArticleDOI
THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION
Fiona A. Harrison,William W. Craig,William W. Craig,Finn Erland Christensen,Charles J. Hailey,William W. Zhang,Steven E. Boggs,Daniel Stern,W. Rick Cook,Karl Forster,Paolo Giommi,Brian W. Grefenstette,Yunjin Kim,Takao Kitaguchi,Jason E. Koglin,Kristin K. Madsen,Peter H. Mao,Hiromasa Miyasaka,Kaya Mori,M. Perri,Michael J. Pivovaroff,Simonetta Puccetti,Vikram Rana,Niels Jørgen Stenfeldt Westergaard,J. L. Willis,Andreas Zoglauer,Hongjun An,Matteo Bachetti,Matteo Bachetti,Nicolas M. Barrière,Eric C. Bellm,Varun Bhalerao,Varun Bhalerao,Nicolai Brejnholt,Felix Fuerst,Carl Christian Liebe,Craig B. Markwardt,Melania Nynka,Julia Vogel,Dominic J. Walton,Daniel R. Wik,David M. Alexander,L. R. Cominsky,Ann Hornschemeier,Allan Hornstrup,Victoria M. Kaspi,Greg Madejski,Giorgio Matt,S. Molendi,David M. Smith,John A. Tomsick,Marco Ajello,David R. Ballantyne,Mislav Baloković,Didier Barret,Didier Barret,Franz E. Bauer,Roger Blandford,W. Niel Brandt,Laura Brenneman,James Chiang,Deepto Chakrabarty,Jérôme Chenevez,Andrea Comastri,Francois Dufour,Martin Elvis,Andrew C. Fabian,Duncan Farrah,Chris L. Fryer,Eric V. Gotthelf,Jonathan E. Grindlay,D. J. Helfand,Roman Krivonos,David L. Meier,Jon M. Miller,Lorenzo Natalucci,Patrick Ogle,Eran O. Ofek,Andrew Ptak,Stephen P. Reynolds,Jane R. Rigby,Gianpiero Tagliaferri,Stephen E. Thorsett,Ezequiel Treister,C. Megan Urry +84 more
TL;DR: The Nuclear Spectroscopic Telescope Array (NuSTAR) as discussed by the authors is the first focusing high-energy X-ray telescope in orbit, which operates in the band from 3 to 79 keV.
Journal ArticleDOI
The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
Fiona A. Harrison,William W. Craig,Finn Erland Christensen,Charles J. Hailey,W. W. Zhang,Steven E. Boggs,Daniel Stern,W. Rick Cook,Karl Forster,Paolo Giommi,Brian W. Grefenstette,Yunjin Kim,Takao Kitaguchi,Jason E. Koglin,Kristin K. Madsen,Peter H. Mao,Hiromasa Miyasaka,Kaya Mori,M. Perri,Michael J. Pivovaroff,Simonetta Puccetti,Vikram Rana,Niels Jørgen Stenfeldt Westergaard,J. L. Willis,Andreas Zoglauer,Hongjun An,Matteo Bachetti,Nicolas M. Barrière,Eric C. Bellm,Varun Bhalerao,Nicolai Brejnholt,Felix Fuerst,Carl Christian Liebe,Craig B. Markwardt,Melania Nynka,Julia Vogel,Dominic J. Walton,Daniel R. Wik,David M. Alexander,L. R. Cominsky,Ann Hornschemeier,Allan Hornstrup,Victoria M. Kaspi,Greg Madejski,Giorgio Matt,Silvano Molendi,David M. Smith,John A. Tomsick,Marco Ajello,David R. Ballantyne,Mislav Baloković,Diddier Barret,Franz E. Bauer,Roger Blandford,W. Niel Brandt,Laura Brenneman,James Chiang,Deepto Chakrabarty,Jérôme Chenevez,Andrea Comastri,Martin Elvis,Andrew C. Fabian,Duncan Farrah,Chris L. Fryer,Eric V. Gotthelf,Jonathan E. Grindlay,David J. Helfand,Roman Krivonos,David L. Meier,Jon M. Miller,Lorenzo Natalucci,Patrick Ogle,Eran O. Ofek,Andrew Ptak,Stephen P. Reynolds,Jand R. Rigby,Gianpiero Tagliaferri,Stephen E. Thorsett,Ezequiel Treister,C. Megan Urry +79 more
TL;DR: The Nuclear Spectroscopic Telescope Array (NuSTAR) as discussed by the authors is the first focusing high-energy X-ray telescope in orbit, which operates in the band from 3 - 79 keV.
Journal ArticleDOI
The RHESSI Imaging Concept
G. J. Hurford,Edward J. Schmahl,Edward J. Schmahl,Richard A. Schwartz,A. J. Conway,Markus J. Aschwanden,André Csillaghy,B. R. Dennis,Christopher M. Johns-Krull,Säm Krucker,Robert P. Lin,J. M. McTiernan,Thomas R. Metcalf,J. Sato,David M. Smith +14 more
TL;DR: The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) as mentioned in this paper uses nine rotating modulation collimators that time-modulate the incident flux as the spacecraft rotates.
Journal ArticleDOI
An exceptionally bright flare from SGR 1806–20 and the origins of short-duration γ-ray bursts
Kevin Hurley,Steven E. Boggs,Steven E. Boggs,David M. Smith,Robert C. Duncan,Robert P. Lin,Andreas Zoglauer,Säm Krucker,G. J. Hurford,Hugh S. Hudson,C. Wigger,Wojtek Hajdas,Christopher Thompson,I. G. Mitrofanov,A. B. Sanin,William V. Boynton,C. Fellows,A. von Kienlin,G. G. Lichti,Arne Rau,T. L. Cline +20 more
TL;DR: In this article, the authors reported the detection of a long (380's) giant flare from SGR 1806-20, which was much more luminous than any previous transient event observed in our Galaxy.