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2.1.2 Preliminary Results of the Micrometeoroid Experiment on Board Helios A

Published online by Cambridge University Press:  12 April 2016

E. Grün
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg, F.R.G.
J. Kissel
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg, F.R.G.
H. Fechtig
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg, F.R.G.
P. Gammelin
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg, F.R.G.
H.-J. Hoffmann
Affiliation:
Physikalisches Institut, Rheinische Friedrich-Wilhelms-UniversitätBonn/F.R.G.

Abstract

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For the first time in situ measurements of interplanetary dust have been performed between 0.3 AU and 1 AU from the sun by the micrometeoroid experiment on board Helios A. The measured particle masses are between 10−15 g and 10−8 g and their measured speeds are between 2 km/sec and 20 km/sec. Particle impacts are identified by the time-of-flight spectra of the ions released upon impact. 15 large particles (m ≥ 10−12 g) were detected from Dec. 15, 1974 to Sept. 5, 1975. They show a strong increase of the impact rate (appr. a factor of 10) between 1 AU and 0.3 AU. The directions from which they impacted the sensor are concentrated between the solar direction and the apex direction of the Helios spacecraft.

Type
2 In Situ Measurements of Interplanetary Dust
Copyright
Copyright © Springer-Verlag 1976

References

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