Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh51a1188g&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SH51A-1188
Physics
2124 Heliopause And Solar Wind Termination, 7538 Solar Irradiance, 7549 Ultraviolet Emissions
Scientific paper
The Pioneer 10 (P10) Lyman Alpha dataset is the only dataset that is available for the study of the very local interstellar medium (VLISM) in the downstream direction relative to the incoming interstellar neutral hydrogen flow, at very large distances from the sun. Selected P10 data obtained in 1984 and 1986 at distances between 31.81 to 32.25 and 37.29 to 37.74 AU have been used to estimate the local interstellar neutral hydrogen and proton densities. State of the art, stationary neutral-plasma and radiative transfer models have been used in the interpretation of the data. No VLISM heliospheric model was found that best fitted both the P10 1984 data and the 1986 data. The most probable cause for the failure to find a single best fit model is neutral hydrogen density fluctuation due to heliospheric time-dependence. The result obtained here is in qualitative agreement with recent Voyager 1 observations.
Gangopadhyay Pradip
Gruntman Mike
Izmodenov Vladislav V.
Judge Darrell
No associations
LandOfFree
Search for Heliospheric Time-dependence in Pioneer 10 Heliospheric Lyman Alpha Glow Data 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 Search for Heliospheric Time-dependence in Pioneer 10 Heliospheric Lyman Alpha Glow Data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for Heliospheric Time-dependence in Pioneer 10 Heliospheric Lyman Alpha Glow Data will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-758906