The UCSD kinematic IPS solar wind boundary and its use in the ENLIL 3-D MHD prediction model-Reference-Cited by-同舟云学术

The UCSD kinematic IPS solar wind boundary and its use in the ENLIL 3-D MHD prediction model

Author:

Jackson B. V.¹,Odstrcil D.²³,Yu H.-S.¹,Hick P. P.¹,Buffington A.¹,Mejia-Ambriz J. C.¹⁴,Kim J.⁵,Hong S.⁵,Kim Y.⁵,Han J.⁵,Tokumaru M.⁶

Affiliation:

1. Center for Astrophysics and Space Sciences; University of California, San Diego; La Jolla California USA

2. School of Physics, Astronomy, and Computational Sciences; George Mason University; Fairfax Virginia USA

3. NASA GSFC; Greenbelt Maryland USA

4. SCiESMEX, Instituto de Geofisica, Unidad Michoacan; Universidad Nacional Autonoma de Mexico; Morelia Mexico

5. Korean Space Weather Center, National Radio Research Agency; Jeju-si South Korea

6. Solar-Terrestrial Environment Laboratory; Nagoya University; Chikusa-ku Japan

Funder

AFOSR

NSF

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

Reference63 articles.

1. Microturbulence in solar wind streams;Ananthakrishnan;J. Geophys. Res.,1980

4. Coronal mass ejection reconstructions from interplanetary scintillation data using a kinematic model: A brief review;Bisi;Adv. Geosci.,2007

5. Solar wind and CME reconstructions in the inner heliosphere;Bisi;Adv. Geosci.,2008

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