Low Geo‐Effectiveness of Fast Halo CMEs Related to the 12 X‐Class Flares in 2002-Reference-Cited by-同舟云学术

Low Geo‐Effectiveness of Fast Halo CMEs Related to the 12 X‐Class Flares in 2002

Author:

Schmieder B.¹²³^ORCID,Kim R.‐S.²⁴^ORCID,Grison B.⁵^ORCID,Bocchialini K.⁶,Kwon R.‐Y.²^ORCID,Poedts S.³⁷^ORCID,Démoulin P.¹^ORCID

Affiliation:

1. Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris Meudon France

2. Korea Astronomy and Space Science Institute Daejeon Korea

3. Department of MathematicsKU Leuven Leuven Belgium

4. Department of Science and TechnologyUniversity of Daejeon Daejeon Korea

5. Department of Space PhysicsInstitute of Atmospheric Physics of the Czech Academy of Sciences Prague Czech Republic

6. Institut d'Astrophysique SpatialeUniv. Paris‐Sud, CNRS, Université Paris‐Saclay Orsay CEDEX France

7. Group of Astrophysics, Institute of PhysicsUniversity of Maria Curie‐Skłodowska Lublin Poland

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

Reference99 articles.

2. The standard flare model in three dimensions. II. Upper limit on solar flare energy;Aulanier G.;Astrophysical Journal,2013

5. Billings D. E.(1966).A guide to the solar corona.

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