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==Historia investigationis==
Esse ventum solarem [[siderale instrumentum exploratorium]] sovieticum ''Luna 1'' anno [[1959]] et ''Mariner 2'' ([[Civitate Foederatae|America]]) anno [[1962]] (per transitum ad planetam [[Venus (planeta)|Venerem]]) experimento confirmaverunt. Vela in superficie [[Luna (satelles)|lunae]] metata sunt copias isotoporum [[Helium|helii]], [[Neon|nei]] et [[Argon|argi]]. Sideralia instrumenta speculatoria ''Pioneer 10/11'', ''Voyager 1/2'' et missio ''Ulysses'' ventum solarem extra orbitam Terrae investigaverunt. ''Helios 1/2'' et missiones ''Mariner'' et ''Pioneer'' ad Venerem et ''Vega'' russica facta de eo intra orbitam planetae nostri suppeditaverunt. ''IMP 1-8'', ''AIMP 1/2'', ''ACE'', '' ISEE 1-3'' sideraleque observatorium solare ''SOHO'' ventum illum circum Terram scrutata sunt. Missio ''Ulysses'' etiam res de vento solari extra planitiem eclipticam suppeditavit. Missio, ut referantur exempla ''Genesis,'' in Terram anno [[2004]] redivit, sed rediens in [[aer]]a Terrae adflicta est per ruinam cum [[umbrella descensoria]] non patesceret.
{{NexInt}}
*[[Macula solaris]]
*[[Plasmasphaerium]]
*[[Velum electricum]]
*[[Velum magneticum]]
*[[Velum solare]]
==Bibliographia==
*Fox, Karen C. [[2012]]. NASA Study Using Cluster Reveals New Insights Into Solar Wind. ''NASA.''
*Cuperman, S., et N. Metzler. [[1978]]. Role of fluctuations in the interplanetary magnetic field on the heat conduction in the Solar Wind. ''J. Geophys. Res.'' 78(16): 3167–3168.
*Cuperman, S. et N. Metzler. [[1973]]. ''Astrophys. J.'' 182(3): 961–975.
*Cuperman, S., et N. Metzler. [[1975]]. Solution of 3-fluid model equations with anomalous transport coefficients for thequiet Solar Wind. ''Astrophys. J. 196(1): 205–219.
*Cuperman, S. et N. Metzler. [[1976]]. Relative magnitude of streaming velocities of alpha particles and protons at 1AU. ''Astrophys. and Space Sci.'' 45(2): 411–417.
*Cuperman, S., et N. Metzler. [[1979]]. Comments on Acceleration of Solar Wind He++3 effects of Resonant and nonresonant interactions with transverse waves. ''J. Geophys. Res.'' 84 (NA5): 2139–2140.
*Cuperman, S., N. Metzler, et M. Spygelglass. [[1975]]. Confirmation of known numerical solutions for the quiet Solar Wind equations. ''Astrophys. J.'' 198(3): 755–759.
*Metzler, N. [[1978]]. A multi-fluid model for stellar winds.Proceedings of the L. D. de Feiter Memorial Symposium on the Study of Traveling Interplanetary Phenomena. AFGL-TR-77-0309, Air Force Systems Command, USAF.
*Metzler, N., S. Cuperman, M. Dryer, et P. Rosenau. [[1979]]. A time-dependent two-fluid model with thermal conduction for Solar Wind. ''Astrophys. J.'' 231(3): 960–976.
*Metzler, N. et M. Dryer. [[1978]]. A self-consistent solution of the three-fluid model of the Solar Wind. ''Astrophys. J.'' 222(2): 689–695.
==Nexus externi==
{{CommuniaCat|Solar wind|ventos solares}}
[[Categoria:Astronomia]]<!--PRO TEM-->
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