Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Charalambos Kanella"'
Autor:
Boris V. Gudiksen, Charalambos Kanella
Context. One candidate model for heating the solar corona is magnetic reconnection that embodies Ohmic dissipation of current sheets. When numerous small-scale magnetic reconnection events occur, then it is possible to heat the corona; if ever observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bce5631369ae4b5c205db622c050c40e
http://hdl.handle.net/10852/66106
http://hdl.handle.net/10852/66106
Autor:
Charalambos Kanella, Boris V. Gudiksen
The solar coronal heating problem is an open question since 1939. One proposed model for the transport and release of mechanical energy generated in the sub-phorospheric layers and photosphere is the nanoflare model that incorporates Ohmic heating wh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::84467a627027903463d794b63c8db339
http://arxiv.org/abs/1703.02808
http://arxiv.org/abs/1703.02808
Autor:
Charalambos Kanella, Boris V. Gudiksen
Publikováno v:
Astronomy & Astrophysics. 621:A95
Context. Nanoscale events in cooperation with steady heating from a slow heating mechanism, such as slow-burning current-sheets, could be able to heat the corona; however, their observational traces are hard to detect via current instrumentation. Aft
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf046a0348a5087fb9e9531e50a9d1eb
https://doi.org/10.1051/0004-6361/201833634
https://doi.org/10.1051/0004-6361/201833634
Publikováno v:
Journal of Physics: Conference Series. 642:012021
© Published under licence by IOP Publishing Ltd. An alternative approach to the coronal heating problem, based on the theory of drift waves, has been proposed. The drift mode is the only mode that is able to survive the drastically different (collis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bcf29e1e21b8bb6186c24ea92883465
https://doi.org/10.1088/1742-6596/642/1/012021
https://doi.org/10.1088/1742-6596/642/1/012021