Zobrazeno 1 - 10
of 137
pro vyhledávání: '"Kasparová, J."'
Autor:
García-Rivas, M., Kašparová, J., Berlicki, A., Švanda, M., Dudík, J., Čtvrtečka, D., Zapiór, M., Liu, W., Sobotka, M., Pavelková, M., Motorina, G. G.
Context: On 2022 May 4, an M5.7 flare erupted in the active region NOAA 13004, which was the target of a coordinated campaign between GREGOR, IRIS, Hinode, and ground-based instruments at the Ond\v{r}ejov observatory. A flare kernel located at the ed
Externí odkaz:
http://arxiv.org/abs/2408.10813
Publikováno v:
Solar Physics, (2022) 297:54
Narrowband (~5 MHz) and short-lived (~0.01 s) spikes with three different distributions on the 800-2000 MHz radio spectrum of the 13 June 2012 flare are detected and analyzed. We designate them as SB (spikes distributed in broad band or bands), SZ (s
Externí odkaz:
http://arxiv.org/abs/2204.09327
Publikováno v:
In Additive Manufacturing 5 January 2024 79
Publikováno v:
ApJ, 2020, Volume 889, Issue 2, id.72
Drifting pulsation structures (DPSs) are important radio fine structures usually observed at the beginning of eruptive solar flares. It has been suggested that DPSs carry important information on the energy release processes in solar flares. We study
Externí odkaz:
http://arxiv.org/abs/1912.12518
The Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory has provided unique observations of off-limb flare emission. White-light (WL) continuum enhancements were detected in the "continuum" channel of the Fe 6173 A line during the
Externí odkaz:
http://arxiv.org/abs/1709.06377
Flarix is a radiation-hydrodynamical (RHD) code for modeling of the response of the chromosphere to a beam bombardment during solar flares. It solves the set of hydrodynamic conservation equations coupled with non-LTE equations of radiative transfer.
Externí odkaz:
http://arxiv.org/abs/1602.00016
Recent measurements of vertical extents and positions of the chromospheric hard X-ray (HXR) flare sources based on Ramaty High-Energy Spectroscopic Imager (RHESSI) observations show a significant inconsistency with the theoretical predictions based o
Externí odkaz:
http://arxiv.org/abs/1601.07026
Mg II lines represent one of the strongest emissions from the chromospheric plasma during solar flares. In this article, we studied the Mg II lines observed during the X1 flare on March 29 2014 (SOL2014-03-29T17:48) by IRIS. IRIS detected large inten
Externí odkaz:
http://arxiv.org/abs/1511.00480
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
We study two modifications of the collisional thick-target model (CTTM) based on the global and local re-acceleration of non-thermal electrons by static and stochastic electric fields during their transport from the coronal acceleration site to the t
Externí odkaz:
http://arxiv.org/abs/1401.3329