Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Pascal Saint Hilaire"'
Autor:
Natasha L. S. Jeffrey, Säm Krucker, Morgan Stores, Eduard P. Kontar, Pascal Saint-Hilaire, Andrea F. Battaglia, Laura Hayes, Hannah Collier, Astrid Veronig, Yang Su, Srikar Paavan Tadepalli, Fanxiaoyu Xia
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 2, p 145 (2024)
The Spectrometer/Telescope for Imaging X-rays (STIX) on board Solar Orbiter (SolO) provides a unique opportunity to systematically perform stereoscopic X-ray observations of solar flares with current and upcoming X-ray missions at Earth. These observ
Externí odkaz:
https://doaj.org/article/1c1ad2a794714d5585511dc927dff187
Publikováno v:
The Journal of the Astronautical Sciences. 67:1391-1411
We present the general concept of a telescope with optics and detectors mounted on two separate spacecrafts, in orbit around the telescope’s target (scopocentric or target-centric orbit), and using propulsion to maintain the Target-Optics-Detector
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a01087ae46b06ed00d0256c961b56038
https://doi.org/10.1007/s40295-020-00231-2
https://doi.org/10.1007/s40295-020-00231-2
Publikováno v:
Handbook of X-ray and Gamma-ray Astrophysics ISBN: 9789811645440
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a8b148ecfc1be95f08c293ffd1c58e9a
https://doi.org/10.1007/978-981-16-4544-0_170-1
https://doi.org/10.1007/978-981-16-4544-0_170-1
Publikováno v:
Handbook of X-ray and Gamma-ray Astrophysics ISBN: 9789811645440
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cf4edb7c9d4ae6b304fcb9bff79eafa6
https://doi.org/10.1007/978-981-16-4544-0_169-1
https://doi.org/10.1007/978-981-16-4544-0_169-1
Autor:
Juan Carlos Martínez Oliveros, Juan Camilo Guevara Gómez, Pascal Saint-Hilaire, Hugh Hudson, Säm Krucker
Publikováno v:
The Astrophysical Journal. 936:56
We describe observations of the white-light structures in the low corona following the X8.2 flare SOL2017-09-10, as observed in full Stokes parameters by the Helioseismic and Magnetic Imager (HMI) of the Solar Dynamics Observatory. These data show bo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0334dbed9ac07be3c756f1f2ca03c8ec
https://doi.org/10.3847/1538-4357/ac83b7
https://doi.org/10.3847/1538-4357/ac83b7
Solar flare electron acceleration is an extremely efficient process, but the method of acceleration is not well constrained. Two of the essential diagnostics: electron anisotropy (velocity angle to the guiding magnetic field) and the high energy cuto
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::552ae92717792346951f4fac62dbfa28
https://eprints.gla.ac.uk/224208/2/224208.pdf
https://eprints.gla.ac.uk/224208/2/224208.pdf
Publikováno v:
The Astrophysical Journal. 923:276
Polarized scattered light from low (few tens of megameter altitudes) coronal transients has been recently reported in Solar Dynamics Observatory/Helioseismic and Magnetic Image (HMI) observations. In a classic paper, Minnaert (1930) provided an analy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2ec3636bf3078f9a0a07b4316b928f67
https://doi.org/10.3847/1538-4357/ac2f9b
https://doi.org/10.3847/1538-4357/ac2f9b
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. 294
The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) provides hard X-ray spectral observations with ${\approx}\,1~\mbox{keV}$ resolution to study flare-accelerated ( ${>}\,10~\mbox{keV}$ ) electrons through their bremsstrahlung emission.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1112f87dfa37135f54bb97f429c854ea
https://doi.org/10.1007/s11207-019-1495-6
https://doi.org/10.1007/s11207-019-1495-6
Publikováno v:
Solar Physics, 226 (1)
The radio emission during 201 X-ray selected solar flares was surveyed from 100 MHz to 4 GHz with the Phoenix-2 spectrometer of ETH Zurich. The selection includes all RHESSI flares larger than C5.0 jointly observed from launch until June 30, 2003. De
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::241b3587e85132ad601ee04a9e635352
http://doc.rero.ch/record/319789/files/11207_2005_Article_5254.pdf
http://doc.rero.ch/record/319789/files/11207_2005_Article_5254.pdf