(PDF) Solar Wind Properties and Geospace Impact of Coronal

Solar Wind Properties and Geospace Impact of Coronal Mass Ejection‐driven Sheath Regions: Variation and Driver Dependence

Space Weather - United States

doi 10.1029/2019sw002217

Full Text

Abstract

Available in full text

Categories

Atmospheric Science

Date

August 1, 2019

Authors

E. K. J. Kilpua

M. M. H. Kalliokoski

Publisher

American Geophysical Union (AGU)

Related search

Sheath-Accumulating Propagation of Interplanetary Coronal Mass Ejection

Astrophysical Journal Letters

Planetary Science

English

Characteristic Magnetic Field and Speed Properties of Interplanetary Coronal Mass Ejections and Their Sheath Regions

Journal of Geophysical Research

Planetary Sciences

Atmospheric Science

Aquatic Science

Earth-Surface Processes

Planetary Science

English

Transport and Acceleration of Solar Energetic Particles From Coronal Mass Ejection Shocks

Proceedings of the International Astronomical Union

Planetary Science

English

Low Coronal Signatures of a Coronal Mass Ejection

Proceedings of the International Astronomical Union

Planetary Science

English

Coronal Mass Ejection: Key Issues

Proceedings of the International Astronomical Union

Planetary Science

English

Solar Wind-Magnetosphere Coupling Efficiency During Ejecta and Sheath-Driven Geomagnetic Storms

Journal of Geophysical Research: Space Physics

English

Coronal "Wave": Magnetic Footprint of a Coronal Mass Ejection?

Astrophysical Journal

Planetary Science

English

Dependence of 100 MeV Solar Proton Events on the Solar Activities: Flares and Coronal Mass Ejections

English

Solar Energetic Particles Produced by a Slow Coronal Mass Ejection at ∼0.25 Au

Astrophysical Journal, Supplement Series

Planetary Science

English