Model development for ULYSSES and SOHO

Details Model development for ULYSSES and SOHO Model development for ULYSSES and SOHO

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993alab.reptr....w&link_type=abstract

Final Report, 27 May - 27 Nov. 1993 Alabama Univ., Huntsville.

Physics

Lyman Alpha Radiation, Magnetohydrodynamics, Solar Corona, Solar Physics, Stellar Models, Stellar Structure, Boundary Conditions, Soho Mission, Solar Magnetic Field, Stellar Radiation, Two Dimensional Models, Ulysses Mission

Scientific paper

The purpose of this research is to provide scientific expertise in solar physics and in the development and use of magnetohydrodynamic (MHD) models of coronal structures for the computation of Lyman alpha scattered radiation in these structures. The specific objectives will be to run MHD models with new boundary conditions and compute resulting scattered solar Lyman alpha intensities, guided by results from the first series of boundary conditions.

Affiliated with

Also associated with

No associations

Rating

Model development for ULYSSES and SOHO 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 Model development for ULYSSES and SOHO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Model development for ULYSSES and SOHO will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-808012