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CORONAL MASS EJECTIONS

A. J. HUNDHAUSEN M. L. Guerrieri ; J. R. Jokipii ; C. P. Sonett ; M. S. Matthews ; M. S. Giampapa ; A. S. Ruskin

Cosmic Winds and the Heliosphere, 2018, p.259

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Título:
CORONAL MASS EJECTIONS
Autor: A. J. HUNDHAUSEN
M. L. Guerrieri ; J. R. Jokipii ; C. P. Sonett ; M. S. Matthews ; M. S. Giampapa ; A. S. Ruskin
Assuntos: Applied sciences ; Astronomy ; Astrophysics ; Average linear density ; Coronagraphs ; Coronal mass ejections ; Corpuscular radiation ; Electromagnetism ; Engineering ; Fundamental forces ; Magnetic fields ; Magnetism ; Mass ; Mechanics ; Microphysics ; Optical engineering ; Optical equipment ; Particle physics ; Physical sciences ; Physics ; Solar activity ; Solar flares ; Solar physics ; Solar wind ; Stellar phenomena ; Stellar physics ; Sunspots ; X ray flares
É parte de: Cosmic Winds and the Heliosphere, 2018, p.259
Descrição: Coronal mass ejections are the most spectacular disruptions of the solar corona and among the most energetic forms of solar activity. The thousands of examples observed with space-borne and groundbased instruments now provide a fairly thorough statistical description of mass ejection properties and relationships among those properties. Statistical analyses confirm earlier suggestions that mass ejections are disruptions oflarge-scale, magnetically closed regions of the corona. Mass ejections contribute only a minor fraction of the mass and energy in the solar wind. While their physical origins are not clearly established, there is a substantial body of observational evidence discounting solar flares
Editor: University of Arizona Press
Idioma: Inglês

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