Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Miteva, R."'
The aim of this work is to summarize the main underlying assumptions, simplifications and uncertainties while studying solar energetic particles (SEPs). In general, numerous definitions are used for the evaluation of a given SEP parameter and these d
Externí odkaz:
http://arxiv.org/abs/1705.02144
Autor:
Miteva, R., Kaufmann, P., Cabezas, D. P., Cassiano, M. M., Fernandes, L. O. T., Freeland, S. L., Karlicky, M., Kerdraon, A., Kudaka, A. S., Luoni, M. L., Marcon, R., Raulin, J. -P., Trottet, G., White, S. M.
Publikováno v:
A&A 586, A91 (2016)
The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observed simultaneously in microwaves, H-alpha, EUV, and soft X-ray bands. Al
Externí odkaz:
http://arxiv.org/abs/1512.01763
Solar energetic particle (SEP) events are related to flares and coronal mass ejections (CMEs). This work is a new investigation of statistical relationships between SEP peak intensities - deka-MeV protons and near-relativistic electrons - and charact
Externí odkaz:
http://arxiv.org/abs/1411.4133
Publikováno v:
Solar Physics, 2013, Volume 282, Issue 2, pp.579-613
We study the influence of the large-scale interplanetary magnetic field configuration on the solar energetic particles (SEPs) as detected at different satellites near Earth and on the correlation of their peak intensities with the parent solar activi
Externí odkaz:
http://arxiv.org/abs/1403.0708
Publikováno v:
Central European Astrophysical Bulletin, 2013, Vol. 37, p. 541-553
We present the association rates between solar energetic particles (SEPs) and the radio emission signatures in the corona and IP space during the entire solar cycle 23. We selected SEPs associated with X and M-class flares from the visible solar hemi
Externí odkaz:
http://arxiv.org/abs/1402.6442
We explore the link between solar energetic particles (SEPs) observed at 1 AU and large-scale disturbances propagating in the solar corona, named after the Extreme ultraviolet Imaging Telescope (EIT) as EIT waves, which trace the lateral expansion of
Externí odkaz:
http://arxiv.org/abs/1402.1676
Publikováno v:
Serbian Astronomical Journal, Vol 2019, Iss 199, Pp 83-87 (2019)
Ground-based total solar eclipse observations are still the key method for coronal investigations. The question about its white-light degree of polarization remains unanswered. There are hypotheses claiming that the degree of polarization in certain
Externí odkaz:
https://doaj.org/article/8c835f1d36974157a5e98d4446ce2171
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics November 2018 180:26-34
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics November 2018 179:517-526
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics November 2018 179:1-10