Time- and space-variable structures of interstellar gas passing over the heliosphere - Consequences for the interplanetary UV resonance glow

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Heliosphere, Interplanetary Gas, Interstellar Gas, Luminescence, Ultraviolet Radiation, Lyman Alpha Radiation, Solar Wind, Spatial Distribution, Voyager Project

Scientific paper

There are good reasons to believe that the solar system, propagating through the ambient interstellar medium with a peculiar velocity of about 23 km/s, may be swept over by an inhomogeneous gaseous medium resulting in time-variable inflow parameters at its border. This situation is theoretically studied here for the first time in terms of the resulting time-dependent heliospheric density distributions and associated resonance glow structures. Quantitative theoretical results are presented for a large number of LISM fluctuation periods and amplitudes by which time- and space-variable LISM conditions are described. It is especially evident that fluctuation periods between 20 to 100 yrs may give noticeable imprints on the upwind/downwind glow structures. Finally we show that the effects of time-dependent LISM boundary conditions may at least be partly responsible for presently unexplained inconsistencies in synoptic interpretations of distant upwind and downwind glow data.

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