ESTIMATES OF DENSITIES AND FILLING FACTORS FROM A COOLING TIME ANALYSIS OF SOLAR MICROFLARES OBSERVED WITHRHESSI-Reference-Cited by-同舟云学术

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ESTIMATES OF DENSITIES AND FILLING FACTORS FROM A COOLING TIME ANALYSIS OF SOLAR MICROFLARES OBSERVED WITHRHESSI

Published:2011-07-06 Issue:1 Volume:736 Page:75
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Baylor R. N.,Cassak P. A.,Christe S.,Hannah I. G.,Krucker Säm,Mullan D. J.,Shay M. A.,Hudson H. S.,Lin R. P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/736/i=1/a=75/pdf

Reference69 articles.

1. Parameters of the Magnetic Flux inside Coronal Holes

2. Radiative-dominated cooling of the flare corona and transition region

3. Determination of Flare Heating and Cooling Using the [ITAL]Transition Region and Coronal Explorer[/ITAL]

4. Influence of magnetic field structure on the conduction cooling of flare loops

5. Evaporative cooling of flare plasma

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1. K2 Ultracool Dwarfs Survey – VI. White light superflares observed on an L5 dwarf and flare rates of L dwarfs;Monthly Notices of the Royal Astronomical Society;2020-05-06

2. Understanding Breaks in Flare X-Ray Spectra: Evaluation of a Cospatial Collisional Return-current Model;The Astrophysical Journal;2017-12-14

3. INVESTIGATING THE DIFFERENTIAL EMISSION MEASURE AND ENERGETICS OF MICROFLARES WITH COMBINEDSDO/AIA ANDRHESSIOBSERVATIONS;The Astrophysical Journal;2014-06-20

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