Abstract
Solar wind flow quantities such as matter flux, momentum flux and energy flux, may be closely related to the mechanism responsible for the evolution of the solar wind. In the highly supersonic flow regime their study is facilitated by the fact that the contribution of thermal motions to the momentum and energy fluxes is negligibly small, and thus all three quantities are expressible in terms of proton density n and flow velocity u. If a relation between n, u and heliocentric distance r can be established, the study of these quantities is further simplified. In the following we point out that such a relation does in fact exist, and comment on its implications.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Reference
Rosenbauer, H., Schwerin, R., Marsch, E., Meyer, B., Miggenrieder, H., Montgomery, M.D., Mühlhäuser, K.H., Pilipp, W., Voges, W., and Zink, S.M.: 1977, J. Geophys., 42, pp. 561–580.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1980 IAU
About this chapter
Cite this chapter
Eyni, M., Steinitz, R. (1980). An Empirical Relation Between Density, Flow Velocity and Heliocentric Distance in the Solar Wind. In: Dryer, M., Tandberg-Hanssen, E. (eds) Solar and Interplanetary Dynamics. International Astronomical Union / Union Astronomique Internationale, vol 91. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9100-2_21
Download citation
DOI: https://doi.org/10.1007/978-94-009-9100-2_21
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1163-2
Online ISBN: 978-94-009-9100-2
eBook Packages: Springer Book Archive