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pro vyhledávání: '"S.I. Syrovatskii"'
Akademický článek
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Akademický článek
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Autor:
Zelenyi, L. M.1,2 (AUTHOR), Malova, Kh. V.1,3 (AUTHOR) hmalova@yandex.ru, Popov, V. Yu.1,4,5 (AUTHOR), Grigorenko, E. E.1,2 (AUTHOR), Büchner, J.6 (AUTHOR)
Publikováno v:
Plasma Physics Reports. Sep2021, Vol. 47 Issue 9, p857-877. 21p.
Autor:
Sarmah, Swaraj Pratim1 (AUTHOR), Goswami, Umananda Dev1 (AUTHOR) umananda2@gmail.com
Publikováno v:
European Physical Journal C -- Particles & Fields. Apr2024, Vol. 84 Issue 4, p1-22. 22p.
Autor:
Frank, Anna G.1 (AUTHOR) annfrank@fpl.gpi.ru, Savinov, Sergey A.2 (AUTHOR) s.a.savinov@mail.ru
Publikováno v:
Symmetry (20738994). Jan2024, Vol. 16 Issue 1, p103. 15p.
Autor:
Boris V. Somov, S.I. Syrovatskii
Publikováno v:
Solar Physics. 55:393-399
Observational data and theoretical arguments suggest that the heating source for an active region is the quasi-steady dissipation of magnetic field in current sheets. Effects in the solar atmosphere which are due to the presence of current sheets are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8440d2760783d38b2e6cc354c73a4e03
https://doi.org/10.1007/bf00152582
https://doi.org/10.1007/bf00152582
Publikováno v:
Symposium - International Astronomical Union. 91:491-494
Numerical solutions for problem of hydrodynamic response of the inhomogeneous (exponential) atmosphere on impulsive heating by energetic electrons or by very high-temperature thermal fluxes are discussed.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::50abfccc67e34b3d60c2aaff515da56c
https://doi.org/10.1017/s0074180900068017
https://doi.org/10.1017/s0074180900068017
Autor:
Boris V. Somov, S.I. Syrovatskii
Publikováno v:
Solar Physics. 75:237-244
A longitudinal stability is considered for the quasi-steady current sheet which is uniform along the current. In the MHD approximation, the stability problem is solved for the plane neutral sheet and small disturbances propagating along the current.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::24e498f7886d3a437d8a5d848bb0adb8
https://doi.org/10.1007/bf00153474
https://doi.org/10.1007/bf00153474
Autor:
S.I. Syrovatskii
Publikováno v:
Solar Physics. 58:89-94
Using the adiabatic approximation, it is shown that the problem of the continuous deformation of a force-free (f.f.) field, in general, has no solution. This means that f.f. fields are nonevolutionary and even small perturbations may produce drastic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::91f96760b039cffab15abb1cf06b05bc
https://doi.org/10.1007/bf00152556
https://doi.org/10.1007/bf00152556
Autor:
S.I. Syrovatskii
Publikováno v:
Solar Physics. 76:3-20
A model is presented for the penetration into the corona of a new magnetic field of a developing bipolar region and for its interaction with an old large-scale coronal field. An important feature of the model is a reconnection of the old and new fiel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c5c343316b98834afc1aa14e4ef9d82
https://doi.org/10.1007/bf00214126
https://doi.org/10.1007/bf00214126