Precise timing of solar flare footpoint sources from mid-infrared observations

Autor: Simões, Paulo J. A., Fletcher, Lyndsay, Hudson, Hugh S., Kerr, Graham S., Penn, Matt, Lopez, Karla F.

Solar flares are powerful particle accelerators, and in the accepted standard flare model most of the flare energy is transported from a coronal energy-release region by accelerated electrons which stop collisionally in the chromosphere, heating and

Externí odkaz: http://arxiv.org/abs/2406.11361

Precise timing of solar flare footpoint sources from mid-infrared observations

Autor: Simões, Paulo J.A., Fletcher, Lyndsay, Hudson, Hugh S., Kerr, Graham S., Penn, Matt, Lopez, Karla F.

Publikováno v: Simões, Paulo J.A. Fletcher, Lyndsay Hudson, Hugh S. Kerr, Graham S. Penn, Matt Lopez, Karla F. . Precise timing of solar flare footpoint sources from mid-infrared observations. Monthly notices of the Royal Astronomical Society. 2024, 532(1), 705-718
Monthly notices of the Royal Astronomical Society

Externí odkaz: http://hdl.handle.net/10852/113793