Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid model

Details Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid model Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid model

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...64h&link_type=abstract

NASA Goddard Space Flight Center, International Solar Wind 8 Conference, p. 64

Statistics

Computation

1

Solar Corona, Coronal Holes, Solar Wind, Flow Characteristics, Interplanetary Space, Plasma Density, Temperature Profiles, Line Of Sight, Two Fluid Models, Magnetohydrodynamic Flow, Plasma Temperature, Solar Protons, Coronagraphs, Ulysses Mission, Spartan Satellites, Light Emission, Stellar Models, Scale Height, Proton Energy, Density Measurement, Lyman Alpha Radiation

Scientific paper

Using the empirical constraints provided by observations in the inner corona and in interplanetary space. we derive the flow properties of the solar wind using a two fluid model. Density and scale height temperatures are derived from White Light coronagraph observations on SPARTAN 201-1 and at Mauna Loa, from 1.16 to 5.5 R, in the two polar coronal holes on 11-12 Apr. 1993. Interplanetary measurements of the flow speed and proton mass flux are taken from the Ulysses south polar passage. By comparing the results of the model computations that fit the empirical constraints in the two coronal hole regions, we show how the effects of the line of sight influence the empirical inferences and subsequently the corresponding numerical results.

Affiliated with

Also associated with

No associations

Rating

Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid 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 Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Flow properties of the solar wind obtained from white light data, ULYSSES observations and a two-fluid model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-759953