Abstract
We discuss present knowledge about interstellar dust grains in the heliosphere in order to give goals for future investigations. As far as the identification of the interstellar flux from brightness observations is concerned we calculate the influence of interstellar dust entering the solar system on the Zodiacal light and Zodiacal emission brightness. In case of the Zodiacal light produced by the scattering of solar radiation, the brightness from interstellar dust within the solar system is not detectable within the limits of present observations. In the case of the thermal emission a distinction of the brightness from the interstellar dust component may be possible. This would be especially interesting for an analysis of the overall spatial distribution of the interstellar flux in the solar system. As far as the identification of the interstellar flux from impact experiments is concerned, parameters like the impact direction are essential. Since the interstellar dust flux is modified in the outer solar system already, it is helpful to probe its variation with increasing distance from the Sun in interstellar upstream direction.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Backman, D.E. and Paresce, F.: 1993, ‘The VEGA Phenomenon’, in Protostars and Planets III, Eds.E.h. Levy, J.I. Lunine and M. S. Matthews (Tuscon: Univ. Arizona Press), p 1253.
Baguhl, M., Grün, E., Hamilton, D.P. et al.: 1995, ‘The Flux of Interstellar Dust observed by Ulysses and Galileo’, Space Sci. Rev. 72, 471–476.
Eggert, et al. this issue
Fahr, H.J.: 1971, ‘The Interplanetary Hydrogen Cone and its Solar Cycle Variations’, Astronom Astrophys. 14, 263–274.
Frisch, P.C.: 1995,’Characteristics of Nearby Interstellar Matter’, Space Sci. Rev. 72, 499–592.
Geiss, J., Gloeckler, G., Mall, U., von Steiger R., Galvin, A.B. and Ogilvie, K.W.: 1994, ‘Interstellar Oxygen, Nitrogen and Neon in the Heliosphere’, Astron. Astrophys. 282, 924–933.
Giese, R.H.: 1979, ‘Zodiacal Light and Local Interstellar Dust: Predictions for an Out-of-Ecliptic Spacecraft’, Astron. Astrophys. 77, 223–226.
Grün, E. Gustafson,B., Mann, I. et al.: 1994, ‘Interstellar Dust in the Heliosphere’ Astron. Astrophys. 286,915–924.
Lallement, R.: 1990, in S. Grzedzielski an E. Page (eds.), ‘Scattering of Solar UV on Local Neutral Gases’, COSPAR Colloquia Series, No 1, Physics of the Outer Heliosphere, Pergamon Press, London, pp. 49–60.
Mann, I.: 1995, ‘Spatial Distribution and Orbital Properties of Interplanetary Dust at High Latitudes’, Space Sci Rev. 72, 477–482.
Mann, I. and Grün, E.: 1995, ‘Dust beyond the Asteroid Belt’, Planet. Space Sci. 43, 827–832.
Morfill, G. and Grün, E.: 1979 ‘The Motion of Changed Dust Particles in Interplanetary Space’, Planet. Space Sci. 27,1269–1282.
Witte, M. Rosenbauer, H., Banaskiewicz, M. and Fahr, H.: 1993, ‘Ulysses Neutral Gas Experiment: Determination of the Velocity and the Temperature of the Interstellar Neutral Helium’, Adv. Space Res. 13(6), 121–130.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1996 Kluwer Academic Publishers
About this paper
Cite this paper
Mann, I. (1996). Interstellar Grains in the Solar System: Requirements for an Analysis. In: Von Steiger, R., Lallement, R., Lee, M.A. (eds) The Heliosphere in the Local Interstellar Medium. Space Science Series of ISSI, vol 1. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1782-8_27
Download citation
DOI: https://doi.org/10.1007/978-94-009-1782-8_27
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7296-0
Online ISBN: 978-94-009-1782-8
eBook Packages: Springer Book Archive