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Coronal Mass Ejections: Models and Their Observational Basis
DOI: 10.12942/lrsp-2011-1 Bibcode: 2011LRSP....8....1C

Chen, P. F.

Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar system, expanding from active region-sized nonpotential magnetic structure to a much larger size. The bulk of plasma with a mass of ∼ 1011,1013 kg is hauled up all the way out to the interplanetary space with a typical velocity of several hun…

2011 Living Reviews in Solar Physics
SOHO 643
Magnetic Structure of Sunspots
DOI: 10.12942/lrsp-2011-4 Bibcode: 2011LRSP....8....4B

Ichimoto, Kiyoshi; Borrero, Juan M.

In this review we give an overview about the current state-of-knowledge of the magnetic field in sunspots from an observational point of view. We start by offering a brief description of tools that are most commonly employed to infer the magnetic field in the solar atmosphere with emphasis in the photosphere of sunspots. We then address separately…

2011 Living Reviews in Solar Physics
Hinode 143