Zobrazeno 1 - 10
of 26
pro vyhledávání: '"B. Calvo-Mozo"'
Autor:
Juan Carlos Martinez Oliveros, Stuart D. Bale, Saida Milena Diaz Castillo, B. Calvo-Mozo, Marc Pulupa, Vratislav Krupar
We report and examine the observation of an unusual and rare in-situ electron observation associated with a solar type III radio burst on 24 December 1996. This radio event was accompanied by high energy electrons, measured by the Solid State Telesco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d36962aa616e437b7a09de4bf41f0747
http://arxiv.org/abs/1910.04306
http://arxiv.org/abs/1910.04306
Publikováno v:
Proceedings of the International Astronomical Union. 12:134-139
We present a database of 11 interplanetary shocks associated to coronal mass ejections (CMEs) observed by STEREO and Wind missions between 2006 and 2011 that show evidence of Type II radio burst. For all events, we calculated the principal characteri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e324883797407e7b48605ab3cd2a6258
https://doi.org/10.1017/s1743921317004008
https://doi.org/10.1017/s1743921317004008
Publikováno v:
Proceedings of the International Astronomical Union. 12:16-19
Solar radio astronomy is a fast developing research field in Colombia. Here, we present the scientific goals, specifications and current state of the First Colombian Solar Radio Interferometer consisting of two log-periodic antennas covering a freque
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46cb74004be5eb1b6821b0cb2b330d49
https://doi.org/10.1017/s1743921317000084
https://doi.org/10.1017/s1743921317000084
Autor:
Angel D. Martínez, Valeria Quintero Ortega, Juan Carlos Martinez Oliveros, Alina-Catalina Donea, Juan Camilo Buitrago-Casas, Charles Lindsey, Douglas Braun, B. Calvo-Mozo
Publikováno v:
The Astrophysical Journal Letters. 901:L9
We report the discovery of ultra-impulsive acoustic emission from a solar flare, emission with a seismic signature that indicates submersion of its source approximately a Mm beneath the photosphere of the active region that hosted the flare. Just ove
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::43165bacda038b2024a01e74f35ba144
https://doi.org/10.3847/2041-8213/abad2a
https://doi.org/10.3847/2041-8213/abad2a
Autor:
Juan Camilo Buitrago-Casas, Charles Lindsey, Juan Carlos Martinez Oliveros, Valeria Quintero Ortega, Angel D. Martínez, B. Calvo-Mozo
Publikováno v:
The Astrophysical Journal. 895:L19
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d5929223a5b550de23e14408008f8cb6
https://doi.org/10.3847/2041-8213/ab9173
https://doi.org/10.3847/2041-8213/ab9173
Autor:
S. Zharkov, J. Martinez Oliveros, Juan Camilo Buitrago-Casas, Lindsay Glesener, C. Lindsey, Säm Krucker, B. Calvo-Mozo
Publikováno v:
Solar Physics. 290:3151-3162
Several mechanisms have been proposed to explain the transient seis- mic emission, i.e., sunquakes, from some solar flares. Some theories associate high-energy electrons and/or white-light emission with sunquakes. High-energy charged particles and th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b00d846a34d8a5f278597a55406d0c7f
https://doi.org/10.1007/s11207-015-0786-9
https://doi.org/10.1007/s11207-015-0786-9
Abrupt and permanent changes of photospheric magnetic fields have been observed during solar flares. The changes seem to be linked to the reconfiguration of magnetic fields, but their origin is still unclear. We carried out a statistical analysis of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd83c0de0e78cfdb3a37d2528c62a27a
http://arxiv.org/abs/1711.08631
http://arxiv.org/abs/1711.08631
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
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