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Mariani, F., Bavassano, B., Villante, U. (1983) A statistical study of MHD discontinuities in the inner solar system: Helios 1 and 2. Solar Physics, 83 (2). 349-365 doi:10.1007/bf00148285

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Reference TypeJournal (article/letter/editorial)
TitleA statistical study of MHD discontinuities in the inner solar system: Helios 1 and 2
JournalSolar Physics
AuthorsMariani, F.Author
Bavassano, B.Author
Villante, U.Author
Year1983 (March)Volume83
Issue2
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00148285Search in ResearchGate
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Mindat Ref. ID8917459Long-form Identifiermindat:1:5:8917459:9
GUID0
Full ReferenceMariani, F., Bavassano, B., Villante, U. (1983) A statistical study of MHD discontinuities in the inner solar system: Helios 1 and 2. Solar Physics, 83 (2). 349-365 doi:10.1007/bf00148285
Plain TextMariani, F., Bavassano, B., Villante, U. (1983) A statistical study of MHD discontinuities in the inner solar system: Helios 1 and 2. Solar Physics, 83 (2). 349-365 doi:10.1007/bf00148285
In(1983, March) Solar Physics Vol. 83 (2) Springer Science and Business Media LLC

See Also

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Mariani, F., Villante, U., Bruno, R., Bavassano, B., Ness, N.F. (1979) An extended investigation of Helios 1 and 2 observations: The interplanetary magnetic field between 0.3 and 1 AU. Solar Physics, 63 (2). doi:10.1007/bf00174545
Bavassano, B., Dobrowolny, M., Fanfoni, G., Mariani, F., Ness, N. F. (1982) Statistical properties of MHD fluctuations associated with high-speed streams from Helios-2 observations. Solar Physics, 78 (2). 373-384 doi:10.1007/bf00151617
Bruno, R., Villante, U., Bavassano, B., Schwenn, R., Mariani, F. (1986) In-situ observations of the latitudinal gradients of the solar wind parameters during 1976 and 1977. Solar Physics, 104 (2). 431-445 doi:10.1007/bf00159093
Mariani, F., Bavassano, B., Villante, U. (1985) Comment on “A reexamination of rotational and tangential discontinuities in the solar wind” by M. Neugebauer et al. Journal of Geophysical Research, 90. 5363 doi:10.1029/ja090ia06p05363
Mariani, F., Ness, N. F., Burlaga, L. F., Bavassano, B., Villante, U. (1978) The large-scale structure of the interplanetary magnetic field between 1 and 0.3 AU during the primary mission of Helios 1. Journal of Geophysical Research, 83. 5161 doi:10.1029/ja083ia11p05161
Bruno, R., Bavassano, B., Villante, U. (1985) Evidence for long period Alfvén waves in the inner solar system. Journal of Geophysical Research, 90. 4373 doi:10.1029/ja090ia05p04373
Burlaga, L. F., Ness, N. F., Mariani, F., Bavassano, B., Villante, U., Rosenbauer, H., Schwenn, R., Harvey, J. (1978) Magnetic fields and flows between 1 and 0.3 AU during the primary mission of Helios 1. Journal of Geophysical Research, 83. 5167 doi:10.1029/ja083ia11p05167
Mariani, F., Bavassano, B., Villante, U., Ness, N. F. (1973) Variations of the occurrence rate of discontinuities in the interplanetary magnetic field. Journal of Geophysical Research, 78 (34) 8011-8022 doi:10.1029/ja078i034p08011
Dobrowolny, M., Bavassano, B., Mariani, F., Ness, N. (1979) Magnetic dips in the solar wind. Solar Physics, 62 (1). 203-220 doi:10.1007/bf00150144
Villante, U., Bruno, R., Mariani, F., Burlaga, L.F., Ness, N.F. (1979) The shape and location of the sector boundary surface in the inner solar system. Journal of Geophysical Research, 84. 6641 doi:10.1029/ja084ia11p06641
Bavassano, B. (1994) Recent observations of MHD fluctuations in the solar wind. Annales Geophysicae, 12 (2) 97 doi:10.1007/s005850050039
 
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