The Solar Wind Speed Expansion Factor [${v}$–$f _{\text{s}}$] Relationship at the Inner Boundary (18 $\text{R}_{\odot }$) of the Heliosphere
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-019-1576-6.pdf
Reference58 articles.
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3. Arge, C.N., Odstrcil, D., Pizzo, V.J., Mayer, L.R.: 2003, Improved method for specifying solar wind speed near the Sun. In: Velli, M., Bruno, R., Malara, F. (eds.) Proc. Tenth Internat. Solar Wind Conf.CP-679, Am. Inst. Phys., Melville, 190. DOI .
4. Arge, C.N., Luhmann, J.G., Schrijver, C.J., Li, Y.: 2004, Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME. J. Atmos. Solar-Terr. Phys.66, 1295. DOI .
5. Detman, T.R., Dryer, M., Yeh, T., Han, S.M., Wu, S.T.: 1991, A time-dependent, three-dimensional MHD numerical study of interplanetary magnetic draping around plasmoids in the solar wind. J. Geophys. Res.96, 9531. DOI .
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