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Improved forecasts of solar wind parameters using the Kalman filter

Published:2011-10 Issue:10 Volume:9 Page:
ISSN:1542-7390
Container-title:Space Weather
language:en
Short-container-title:Space Weather

Author:

Innocenti M. E.¹,Lapenta G.¹,Vršnak B.²,Crespon F.³,Skandrani C.³,Temmer M.⁴,Veronig A.⁴,Bettarini L.⁵,Markidis S.¹,Skender M.²

Affiliation:

1. Centrum voor Plasma-Astrofysica, Departement Wiskunde; Katholieke Universiteit Leuven; Leuven Belgium

2. Faculty of Geodesy; Hvar Observatory; Zagreb Croatia

3. Noveltis; Ramonville-Saint-Agne France

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

5. Solar-Terrestrial Center of Excellence-SIDC; Royal Observatory of Belgium; Brussels Belgium

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2011SW000659/fullpdf

Reference49 articles.

1. Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates;Arge;J. Geophys. Res.,2000

2. Improved method for specifying solar wind speed near the Sun;Arge;AIP Conf. Proc.,2003

3. Stream structure and coronal sources of the solar wind during the May 12th, 1997, CME (2004);Arge;J. Atmos. Sol. Terr. Phys.,2004

4. What is space weather?;Baker;Adv. Space Res.,1998

5. From the Sun to the Earth: The 13 May 2005 coronal mass ejection;Bisi;Solar Phys.,2010

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