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The Sun and the Heliosphere as an Integrated System pp 201–251Cite as

A Global Picture of CMEs in the Inner Heliosphere

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 317))

Abstract

This is an overview of Coronal mass ejections (CMEs) in the heliosphere with an observational bias towards remote sensing by coronagraphs. Particular emphasis will be placed on the results from the Solar and Heliospheric Observatory (SOHO) mission which has produced high quality CME data uniform and continuos over the longest stretch ever. After summarizing the morphological, physical, and statistical properties of CMEs, a discussion on the phenomena associated with them is presented. These are the various manifestations of CMEs observed at different wavelengths and the accompanying phenomena such as shocks and solar energetic particles that provide information to build a complete picture of CMEs. Implications of CMEs for the evolution of the global solar magnetic field are presented. CMEs in the heliosphere are then discussed including out-of-the-ecliptic observations from Ulysses and the possibility of a 22-year cycle of cosmic ray modulation by CMEs. After outlining some of the outstanding questions, a summary of the chapter is provided.

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  1. Laboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, MD, 20771, USA

    N. Gopalswamy

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  1. INAF — Osservatorio di Arcetri, Firenze, Italy

    Giannina Poletto

  2. NASA Marshall Space Flight Center, National Space & Technology Center/Solar Physics, Huntsville, AL, USA

    Steven T. Suess

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Gopalswamy, N. (2004). A Global Picture of CMEs in the Inner Heliosphere. In: Poletto, G., Suess, S.T. (eds) The Sun and the Heliosphere as an Integrated System. Astrophysics and Space Science Library, vol 317. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2831-1_8

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