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Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections

  • Published:2019-04 Issue:4 Volume:17 Page:498-526
  • ISSN:1542-7390
  • Container-title:Space Weather
  • language:en
  • Short-container-title:Space Weather

Author:

Kilpua E.K.J.1ORCID,Lugaz N.2ORCID,Mays M. L.3ORCID,Temmer M.4ORCID

Affiliation:

1. Department of PhysicsUniversity of Helsinki Finland

2. Space Science Center, Institute for the Study of Earth, Oceans, and SpaceUniversity of New Hampshire Durham NH USA

3. NASA Goddard Space Flight Center Greenbelt MD USA

4. Institute of PhysicsUniversity of Graz, Universitaetsplatz 5 Graz Austria

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference279 articles.

1. CORONAL MASS EJECTION INITIATION BY CONVERGING PHOTOSPHERIC FLOWS: TOWARD A REALISTIC MODEL

2. Characterizing and predicting the magnetic environment leading to solar eruptions

3. A Model for Solar Coronal Mass Ejections

4. Modeling the corona and solar wind using ADAPT maps that include far‐side observations;Arge C. N.;Solar Wind 13,2013

5. Air force data assimilative photospheric flux transport (ADAPT) Model;Arge C. N.;Twelfth International Solar Wind Conference,2010

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