Zobrazeno 1 - 10
of 18
pro vyhledávání: '"J. C. Martínez Oliveros"'
Publikováno v:
Astronomy & Astrophysics. 672:A32
Context: White-light continuum observations of solar flares often have coronal counterparts, including the classical ``white-light prominence'' (WLP) phenomenon. Aims: Coronal emissions by flares, seen in white-light continuum, have only rarely been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fce715106b39030bc6e42fca2d8063c6
https://doi.org/10.1051/0004-6361/202245788
https://doi.org/10.1051/0004-6361/202245788
Autor:
Tadayuki Takahashi, Gregory Kyle, Jessie Duncan, Noriyuki Narukage, Steven Christe, Hunter Kanniainen, J. C. Martínez-Oliveros, Daniel F. Ryan, Shin-nosuke Ishikawa, Sophie Musset, Christine A. Jhabvala, Yixian Zhang, Lindsay Glesener, Amy Winebarger, Juan Camilo Buitrago-Casas, Aruna N. Ramanayaka, Eliad Peretz, S. Bongiorno, Athanasios Pantazides, J. T. Vievering, Savannah Perez-Piel, Brian Ramsey, Säm Krucker, Sabrina Savage, Patrick Champey, Jeff McCracken, Kelsey Gilchrist, Shin Watanabe, Gregory Dalton, P. S. Athiray, Wayne H. Baumgartner, Ikuyuki Mitsuishi, Sasha Courtade
Publikováno v:
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII.
The FOXSI-4 sounding rocket will fly a significantly upgraded instrument in NASA's first solar are campaign. It will deploy direct X-ray focusing optics which have revolutionized our understanding of astrophysical phenomena. For example, they have al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::14999fa00465c282baad236b7d28bb2a
https://doi.org/10.1117/12.2594701
https://doi.org/10.1117/12.2594701
Autor:
Vladimir Krasnoselskikh, Säm Krucker, C. Fong, D. J. McComas, James A. Klimchuk, Tai Phan, Michel Moncuquet, N.-E. Raouafi, Marco Velli, Anthony W. Case, C. C. Chaston, Justin C. Kasper, John W. Bonnell, Melvyn L. Goldstein, David Burgess, John R. Wygant, Gregory G. Howes, Christopher H. K. Chen, Trevor A. Bowen, David Stansby, Robert E. Ergun, R. Laker, Samuel T. Badman, Stuart D. Bale, T. Dudok de Wit, F. S. Mozer, Robert J. MacDowall, Keith Goetz, David M. Malaspina, Nicole Meyer-Vernet, Jonathan Eastwood, Davin Larson, Katherine Goodrich, Michael L. Stevens, Adam Szabo, William M. Farrell, Marc Pulupa, Benjamin D. G. Chandran, Kelly E. Korreck, Paul J. Kellogg, Milan Maksimovic, James Drake, J. C. Martínez-Oliveros, Timothy S. Horbury, Cynthia A Cattell, T. Woolley, Chadi Salem, Peter Harvey
Publikováno v:
Nature
Nature, Nature Publishing Group, 2019, 576 (7786), pp.237-242. ⟨10.1038/s41586-019-1818-7⟩
Nature, Nature Publishing Group, 2019, 576 (7786), pp.237-242. ⟨10.1038/s41586-019-1818-7⟩
During the solar minimum, when the Sun is at its least active, the solar wind1,2 is observed at high latitudes as a predominantly fast (more than 500 kilometres per second), highly Alfvenic rarefied stream of plasma originating from deep within coron
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3816853070fe07658b9ba054b4282b28
https://doi.org/10.1038/s41586-019-1818-7
https://doi.org/10.1038/s41586-019-1818-7
Autor:
Milan Maksimovic, N. Carruth, Trevor A. Bowen, D. Seitz, Michel Moncuquet, Keith Goetz, J. C. Martínez-Oliveros, David Sundkvist, Peter Harvey, Marc Pulupa, Pascal Saint-Hilaire, Stuart D. Bale, John W. Bonnell, D. Gordon
Publikováno v:
Journal of Geophysical Research Space Physics
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2017, 122 (3), pp.2836-2854. ⟨10.1002/2016JA023345⟩
Journal of Geophysical Research Space Physics, 2017, 122 (3), pp.2836-2854. ⟨10.1002/2016JA023345⟩
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2017, 122 (3), pp.2836-2854. ⟨10.1002/2016JA023345⟩
Journal of Geophysical Research Space Physics, 2017, 122 (3), pp.2836-2854. ⟨10.1002/2016JA023345⟩
The Radio Frequency Spectrometer (RFS) is a two channel digital receiver and spectrometer, which will make remote sensing observations of radio waves and in situ measurements of electrostatic and electromagnetic fluctuations in the solar wind. A part
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2e3b5c281c54eefb12a9a1f5e150322
https://doi.org/10.1002/2016ja023345
https://doi.org/10.1002/2016ja023345
Publikováno v:
Solar Physics. 245:121-139
We carried out an electromagnetic acoustic analysis of the solar flare of 14 August 2004 in active region AR10656 from the radio to the hard X-ray spectrum. The flare was a GOES soft X-ray class M7.4 and produced a detectable sun quake, confirming ea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dee45826c4be801f2a7a331d8a8e12fd
https://doi.org/10.1007/s11207-007-9004-8
https://doi.org/10.1007/s11207-007-9004-8
Publikováno v:
The Astrophysical Journal. 818:56
Three phases are typically observed during solar flares: the preflare, impulsive, and decay phases. During the impulsive phase, it is believed that the electrons and other particles are accelerated after the stored energy in the magnetic field is rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5323a6c1dc31754ba32a940d41d3b27d
https://doi.org/10.3847/0004-637x/818/1/56
https://doi.org/10.3847/0004-637x/818/1/56
Autor:
Stuart D. Bale, Dusan Odstrcil, J. C. Martínez-Oliveros, Ying Liu, Christian Möstl, Manuela Temmer, Robert P. Lin, Richard A. Harrison, Janet G. Luhmann, David F. Webb
The successive coronal mass ejections (CMEs) from 2010 July 30 - August 1 present us the first opportunity to study CME-CME interactions with unprecedented heliospheric imaging and in situ observations from multiple vantage points. We describe two ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d485c7c71f0494079a99db86b908c947
Autor:
Juan Camilo Buitrago-Casas, Charles Lindsey, B. Calvo-Mozo, Hugh S. Hudson, Julián D. Alvarado-Gómez, J. C. Martínez-Oliveros
Multi--wavelength studies of energetic solar flares with seismic emissions have revealed interesting common features between them. We studied the first GOES X--class flare of the 24th solar cycle, as detected by the Solar Dynamics Observatory (SDO).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8aaacaebae219bf24ac2196e90e263b2
Publikováno v:
Helioseismology, Asteroseismology, and MHD Connections ISBN: 9780387894812
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::357486ee824ca2da13280a8943ab7acb
https://doi.org/10.1007/978-0-387-89482-9_40
https://doi.org/10.1007/978-0-387-89482-9_40
Publikováno v:
Astrophys J
We study the correlation between abrupt permanent changes of magnetic field during X-class flares observed by the GONG and HMI instruments, and the hard X-ray (HXR) emission observed by RHESSI, to relate the photospheric field changes to the coronal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a38db9a80223ecaa426f4fa14f2cc16
https://doi.org/10.1088/0004-637x/806/2/173
https://doi.org/10.1088/0004-637x/806/2/173