Improved input to the empirical coronal mass ejection (CME) driven shock arrival model from CME cone models-Reference-Cited by-同舟云学术

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Improved input to the empirical coronal mass ejection (CME) driven shock arrival model from CME cone models

Published:2006-10 Issue:10 Volume:4 Page:n/a-n/a
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Xie H.¹²,Gopalswamy N.²,Ofman L.¹²,St. Cyr O. C.²,Michalek G.³,Lara A.⁴,Yashiro S.¹²

Affiliation:

1. Department of Physics; Catholic University of America; Washington, D. C. USA

2. NASA Goddard Space Flight Center; Greenbelt Maryland USA

3. Astronomical Observatory of Jagiellonian University; Cracow Poland

4. Instituto de Geofisica; Universidad Nacional Autónoma de México; Mexico City Mexico

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference26 articles.

1. Compound streams, magnetic clouds, and major geomagnetic storms;Burlaga;J. Geophys. Res.,1987

2. Successive CMEs and complex ejecta;Burlaga;J. Geophys. Res.,2002

3. Reply to comment on “Coronal mass ejections, interplanetary ejecta and geomagnetic storms” by Gopalswamy et al.;Cane;Geophys. Res. Lett.,2003

4. Coronal mass ejections, interplanetary ejecta and geomagnetic storms;Cane;Geophys. Res. Lett.,2000

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1. ICME Evolution in the Inner Heliosphere;Solar Physics;2020-04

2. Operational Modeling of Heliospheric Space Weather for the Parker Solar Probe;The Astrophysical Journal Supplement Series;2020-02-01

3. Formation of Coronal Mass Ejections in the Solar Corona and Propagation of the Resulting Plasma Streams in the Heliosphere;Plasma Physics Reports;2019-10

4. Effective Acceleration Model for the Arrival Time of Interplanetary Shocks driven by Coronal Mass Ejections;Solar Physics;2017-11-24

5. Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations;Proceedings of the International Astronomical Union;2017-07

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