Ensemble Prediction of a Halo Coronal Mass Ejection Using Heliospheric Imagers-Reference-Cited by-同舟云学术

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Ensemble Prediction of a Halo Coronal Mass Ejection Using Heliospheric Imagers

Published:2018-07 Issue:7 Volume:16 Page:784-801
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Amerstorfer T.¹^ORCID,Möstl C.¹^ORCID,Hess P.²,Temmer M.³^ORCID,Mays M. L.⁴^ORCID,Reiss M. A.¹⁴^ORCID,Lowrance P.⁵,Bourdin P.-A.¹^ORCID

Affiliation:

1. Space Research Institute; Austrian Academy of Sciences; Graz Austria

2. NRC Research Associate, U.S. Naval Research Laboratory; Washington DC USA

3. Institute of Physics; University of Graz; Graz Austria

4. Heliophysics Science Division; NASA Goddard Space Flight Center; Greenbelt MD USA

5. IPAC; California Institute of Technology; Pasadena CA USA

Funder

Austrian Science Fund

Seventh Framework Programme

Forschungsförderungsgesellschaft/ASAP

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2017SW001786/fullpdf

Reference68 articles.

1. The magnetometer instrument on MESSENGER;Anderson;Space Science Reviews,2007

2. Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME;Arge;Journal of Atmospheric and Solar-Terrestrial Physics,2004

3. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;Journal of Geophysical Research,2000

4. Radio imaging of shock-accelerated electrons associated with an erupting plasmoid on 2010 november 3;Bain;The Astrophysical Journal,2012

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4. Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager Data, and Machine Learning;The Astrophysical Journal;2023-05-01

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