Počet záznamů: 1
Nonequilibrium Processes in the Solar Corona, Transition Region, Flares, and Solar Wind (Invited Review)
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SYSNO ASEP 0482498 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Nonequilibrium Processes in the Solar Corona, Transition Region, Flares, and Solar Wind (Invited Review) Tvůrce(i) Dudík, Jaroslav (ASU-R) RID, ORCID
Dzifčáková, Elena (ASU-R) RID, ORCID
Meyer-Vernet, N. (FR)
Del Zanna, G. (GB)
Young, P. R. (US)
Giunta, A. (GB)
Sylwester, B. (PL)
Sylwester, J. (PL)
Oka, M. (US)
Mason, H. E. (GB)
Vocks, C. (DE)
Matteini, L. (GB)
Krucker, S. (CH)
Williams, D.R. (GB)
Mackovjak, Š. (SK)Zdroj.dok. Solar Physics. - : Springer - ISSN 0038-0938
Roč. 292, č. 8 (2017), 100/1-100/72Poč.str. 72 s. Forma vydání Tištěná - P Jazyk dok. eng - angličtina Země vyd. NL - Nizozemsko Klíč. slova energetic particles ; electrons ; flares Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP GA17-16447S GA ČR - Grantová agentura ČR Institucionální podpora ASU-R - RVO:67985815 UT WOS 000410918200001 EID SCOPUS 85026776960 DOI 10.1007/s11207-017-1125-0 Anotace We review the presence and signatures of the non-equilibrium processes, both non-Maxwellian distributions and non-equilibrium ionization, in the solar transition region, corona, solar wind, and flares. Basic properties of the non-Maxwellian distributions are described together with their influence on the heat flux as well as on the rates of individual collisional processes and the resulting optically thin synthetic spectra. Constraints on the presence of high-energy electrons from observations are reviewed, including positive detection of non-Maxwellian distributions in the solar corona, transition region, flares, and wind. Occurrence of non-equilibrium ionization is reviewed as well, especially in connection to hydrodynamic and generalized collisional-radiative modeling. Predicted spectroscopic signatures of non-equilibrium ionization depending on the assumed plasma conditions are summarized. Finally, we discuss the future remote-sensing instrumentation that can be used for the detection of these non-equilibrium phenomena in various spectral ranges. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2018
Počet záznamů: 1