Effect of Electron Pressure on the Grad–Shafranov Reconstruction of Interplanetary Coronal Mass Ejections-Reference-Cited by-同舟云学术

Effect of Electron Pressure on the Grad–Shafranov Reconstruction of Interplanetary Coronal Mass Ejections

Published:2013-03-08 Issue:1 Volume:284 Page:275-291
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Hu Qiang,Farrugia C. J.,Osherovich V. A.,Möstl C.,Szabo A.,Ogilvie K. W.,Lepping R. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-013-0259-y.pdf

Reference44 articles.

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2. Al-Haddad, N., Nieves-Chinchilla, T., Savani, N.P., Möstl, C., Marubashi, K., Hidalgo, M.A., Roussev, I.I., Poedts, S., Farrugia, C.J.: 2013, Magnetic field configuration models and reconstruction methods: a comparative study. Solar Phys., in this issue. doi: 10.1007/s11207-013-0244-5 .

3. Fainberg, J., Osherovich, V.A., Stone, R.G., MacDowall, R.J., Balogh, A.: 1996, Ulysses observations of electron and proton components in a magnetic cloud and related wave activity. In: Winterhalter, D., Gosling, J.T., Habbal, S.R., Kurth, W.S., Neugebauer, M. (eds.) American Institute of Physics Conference Series 382, 554 – 557. doi: 10.1063/1.51513 .

4. Farrugia, C.J., Fitzenreiter, R.J., Burlaga, L.F., Erkaev, N.V., Osherovich, V.A., Biernat, H.K., Fazakerley, A.: 1994, Observations in the sheath region ahead of a magnetic cloud and in the dayside magnetosheath during magnetic cloud passage. Adv. Space Res. 14, 105 – 110. doi: 10.1016/0273-1177(94)90055-8 .

5. Farrugia, C.J., Berdichevsky, D.B., Möstl, C., Galvin, A.B., Leitner, M., Popecki, M.A., Simunac, K.D.C., Opitz, A., Lavraud, B., Ogilvie, K.W., Veronig, A.M., Temmer, M., Luhmann, J.G., Sauvaud, J.A.: 2011, Multiple, distant (40∘) in situ observations of a magnetic cloud and a corotating interaction region complex. J. Atmos. Solar-Terr. Phys. 73, 1254 – 1269. doi: 10.1016/j.jastp.2010.09.011 .

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