Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model

Details Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40..131b&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, Jan. 1992, p. 131-138.

Computer Science

5

Mars Atmosphere, Planetary Ionospheres, Solar Planetary Interactions, Solar Wind, Venus Atmosphere, Ions, Plasma Turbulence, Space Plasmas, Two Fluid Models

Scientific paper

A two-fluid hydrodynamic (HD) model with anomalous friction between ion species (protons and O+ ions) due to turbulence in the magnetosheath is suggested for solar wind (SW) interactions with Venus and Mars. The method of calculation and results are given for both planets. The results are compared with experimental data from the Pioneer-Venus and PHOBOS-2 spacecraft and also with the results of the one-fluid HD model with mass-loading. The results of the two-fluid HD model are in better agreement with the experimental data than those obtained earlier.

Affiliated with

Also associated with

No associations

Rating

Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Turbulent pick-up of new-born ions near Venus and Mars and problems of numerical modelling of the solar wind interaction with these planets. II - Two-fluid HD model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-939521