Astrophys. Space Sci. Trans., 1, 29-34, 2005
www.astrophys-space-sci-trans.net/1/29/2005/
doi:10.5194/astra-1-29-2005
© Author(s) 2005. This work is licensed under the
Creative Commons Attribution-NonCommercial-ShareAlike 2.5 License.
 
09 Dec 2005
Interpretation of Pioneer 10 heliospheric Ly α glow data obtained beyond 30 AU
D. L. Judge1, V. V. Izmodenov2,3,4, M. Gruntman1, and P. Gangopadhyay1
1University of Southern California, Los Angeles, CA 90089, USA
2Moscow State University, Department of Aeromechanics and Gas Dynamics, School of Mechanics and Mathematics, Moscow, 119899, Russia
3Space Research Institute (IKI), Russian Academy of Sciences
4Institute for Problems in Mechanics, Russian Academy of Sciences

Abstract. The Pioneer 10 (P10) Ly α 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 stationary VLISM heliospheric model was found that best fitted both the P10 1984 data and the 1986 data. The failure to find a single best fit model is most probably due to the fact that the heliospheric model used here did not incorporate time-dependence and interstellar magnetic field effects.

Citation: Judge, D. L., Izmodenov, V. V., Gruntman, M., and Gangopadhyay, P.: Interpretation of Pioneer 10 heliospheric Ly α glow data obtained beyond 30 AU, Astrophys. Space Sci. Trans., 1, 29-34, doi:10.5194/astra-1-29-2005, 2005.
 
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