Boundary Conditions of the Heliosphere

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Radiative transfer equilibrium models of nearby interstellar matter (ISM) yield the boundary conditions of the heliosphere when constrained with observations of ISM inside and outside of the heliosphere. Filtration factors for interstellar neutrals crossing the heliosheath region, from charge exchange with interstellar plasma, are given for H, He, N, O, Ar, and Ne. The best models predict n(HI)~0.2 /cc, n(e)~0.1 /cc, however if the isotropic 2 kHz emission observed by Voyager (Kurth & Gurnett 2003) is formed in the surrounding ISM, an alternate model with lower electron densities is indicated. Observations of nearby ISM, the radiative transfer models, and historical 10Be records provide information on past variations in the galactic environment of the Sun.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Boundary Conditions of the Heliosphere 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 Boundary Conditions of the Heliosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Boundary Conditions of the Heliosphere will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-186121

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.