Signs of magnetic helicity in interplanetary coronal mass ejections and associated prominences: Case study

Author:

Ruzmaikin Alexander1,Martin Sara2,Hu Qiang3

Affiliation:

1. Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA

2. Helio Research; La Crescenta California USA

3. Bartol Research Institute; University of Delaware; Newark Delaware USA

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference40 articles.

1. The magnetic nature of wide EUV filament channels and their role in the mass loading of CMEs;Aulanier;Astron. Astrophys.,2000

2. 3-D magnetic configurations supporting prominences;Aulanier;Astron. Astrophys.,1998

3. Model prediction for an observed filament;Aulanier;Astrophys. J.,2000

4. Geophys. Monogr.;Berger,1999

5. Rate of helicity production by solar rotation;Berger;J. Geophys. Res.,2000

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