Zobrazeno 1 - 10
of 129
pro vyhledávání: '"Vásquez, Alberto A."'
Autor:
Mulay, Sargam M., Sharma, Rohit, Valori, Gherardo, Vásquez, Alberto M., Del Zanna, Giulio, Mason, Helen, Oberoi, Divya
We aim to investigate the spatial location of the source of an active region (AR) jet and its relation with associated nonthermal type~III radio emission. An emission measure (EM) method was used to study the thermodynamic nature of the AR jet. The n
Externí odkaz:
http://arxiv.org/abs/2009.14581
Autor:
Long, David M., Valori, Gherardo, Pérez-Suárez, David, Morton, Richard J., Vásquez, Alberto Marcos
Publikováno v:
A&A 603, A101 (2017)
"EIT waves" are freely-propagating global pulses in the low corona which are strongly associated with the initial evolution of coronal mass ejections (CMEs). They are thought to be large-amplitude, fast-mode magnetohydrodynamic waves initially driven
Externí odkaz:
http://arxiv.org/abs/1703.10020
Autor:
López, Fernando M., Cremades, Hebe, Nuevo, Federico A., Balmaceda, Laura A., Vásquez, Alberto A.
We carry out an analysis of the evacuated mass from three coronal dimming regions observed by the {\it Atmospheric Imaging Assembly} (AIA) on board the {\it Solar Dynamics Observatory}. The three events are unambiguously identified with white-light c
Externí odkaz:
http://arxiv.org/abs/1611.00849
Akademický článek
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Autor:
STASTNY, PETER, LOVELL, ANNE m., HANNAH, JULIE, GOULART, DANIEL, VASQUEZ, ALBERTO, O’CALLAGHAN, SEANA, PŪRAS, DAINIUS
Publikováno v:
Health and Human Rights, 2020 Jun 01. 22(1), 105-120.
Externí odkaz:
https://www.jstor.org/stable/26923478
The Atmospheric Imaging Assembly (AIA) telescope on board the Solar Dynamics Observatory (SDO) provides coronal EUV imaging over a broader temperature sensitivity range than the previous generations of instruments (EUVI, EIT, and TRACE). Differential
Externí odkaz:
http://arxiv.org/abs/1503.02473
Autor:
Vásquez, Alberto Marcos
The large availability and rich spectral coverage of today's observational data of the solar corona, and the high spatial and temporal resolution of many instruments, has enabled the evolution of three-dimensional (3D) physical models to a great leve
Externí odkaz:
http://arxiv.org/abs/1503.02238
Autor:
Oran, Rona, Landi, Enrico, van der Holst, Bart, Lepri, Susan T., Vásquez, Alberto M., Nuevo, Federico. A., Frazin, Richard, Manchester IV, Ward B., Sokolov, Igor V., Gombosi, Tamas I.
Publikováno v:
ApJ, 806, 55, 2015
The higher charge states found in slow ($<$400km s$^{-1}$) solar wind streams compared to fast streams have supported the hypothesis that the slow wind originates in closed coronal loops, and released intermittently through reconnection. Here we exam
Externí odkaz:
http://arxiv.org/abs/1412.8288
Autor:
Hauser, Robert A., Sutherland, Dean, Madrid, Juan A., Rol, Maria Angeles, Frucht, Steven, Isaacson, Stuart, Pagan, Fernando, Maddux, Brian N., Li, George, Tse, Winona, Walter, Benjamin L., Kumar, Rajeev, Kremens, Daniel, Lew, Mark F., Ellenbogen, Aaron, Oguh, Odinachi, Vasquez, Alberto, Kinney, William, Lowery, Matt, Resnick, Maria, Huff, Nicole, Posner, Jerry, Ballman, Karla V., Harvey, Brian E., Camilleri, Michael, Zasloff, Michael, Barbut, Denise
Publikováno v:
In Clinical Parkinsonism & Related Disorders 2019 1:2-7
Autor:
Huang, Zhenguang, Frazin, Richard A., Landi, Enrico, Manchester IV, Ward B., Vásquez, Alberto M., Gombosi, Tamas I.
Magnetic loops are building blocks of the closed-field corona. While active region loops are readily seen in images taken at EUV and X-ray wavelengths, quiet Sun loops are seldom identifiable and therefore difficult to study on an individual basis. T
Externí odkaz:
http://arxiv.org/abs/1207.6661