DERIVING THE PROPERTIES OF CORONAL PRESSURE FRONTS IN 3D: APPLICATION TO THE 2012 MAY 17 GROUND LEVEL ENHANCEMENT-Reference-Cited by-同舟云学术

DERIVING THE PROPERTIES OF CORONAL PRESSURE FRONTS IN 3D: APPLICATION TO THE 2012 MAY 17 GROUND LEVEL ENHANCEMENT

Published:2016-12-07 Issue:1 Volume:833 Page:45
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Rouillard A. P.,Plotnikov I.,Pinto R. F.^ORCID,Tirole M.,Lavarra M.,Zucca P.,Vainio R.,Tylka A. J.,Vourlidas A.^ORCID,Rosa M. L. De,Linker J.,Warmuth A.,Mann G.,Cohen C. M. S.^ORCID,Mewaldt R. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/833/i=1/a=45/pdf

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1. PAMELA’S MEASUREMENTS OF MAGNETOSPHERIC EFFECTS ON HIGH-ENERGY SOLAR PARTICLES

2. A “breathing” source surface for cycles 23 and 24

3. Modeling of Coronal EUV Loops Observed withTRACE. I. Hydrostatic Solutions with Nonuniform Heating

4. Heliospheric plasma sheet and coronal streamers

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