A1 Refereed original research article in a scientific journal

Double Filament as a Fine Structure Element of Flare Configuration




AuthorsSolov'ev AA, Riehokainen A, Smirnova VV, Korol'kova OA

PublisherMAIK NAUKA/INTERPERIODICA/SPRINGER

Publication year2022

JournalGeomagnetism and Aeronomy

Journal name in sourceGEOMAGNETISM AND AERONOMY

Journal acronymGEOMAGN AERONOMY+

Volume62

Issue8

First page 1021

Last page1029

Number of pages9

ISSN0016-7932

eISSN1555-645X

DOIhttps://doi.org/10.1134/S0016793222080187

Web address https://link.springer.com/article/10.1134/S0016793222080187


Abstract
We investigate the properties of a double horizontal magnetic filament, uniform in length and located in the solar atmosphere in an external uniform magnetic field. A specific feature of current screening in this magnetic configuration is that the currents do not form a coaxial structure, like in a single magnetic bundle, but are located in two close parallel bands, so the total current in the double filament is zero. Such filaments do not tend to merge during lateral contact into a single magnetic structure. The equilibrium distributions of the plasma density and electric current density in the filament are calculated and the possibilities are shown for the electric current density in the filament to reach critical values at which "anomalous resistance " occurs due to the development of current ion-acoustic instability. The anomalous resistance turns out to be much larger than the usual Coulomb resistance. The following values have been found: the scale of the dissipation region, the electric field strength in it, which significantly exceeds the Dreiser value, and the possible energy of accelerated charged particles (up to hundreds of MeV).



Last updated on 2024-26-11 at 12:04