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2.3.5 Magellan Collections of Large Cosmic Dust Particles

Published online by Cambridge University Press:  12 April 2016

D. S. Hallgren ,
C. L. Hemenway  and
R. Wlochowicz
D. S. Hallgren
Affiliation:
Dudley Observatory, Albany, N. Y.USA
C. L. Hemenway
Affiliation:
Dudley Observatory, Albany, N. Y.USA
R. Wlochowicz
Affiliation:
Herzberg Institute of Astrophysics, National Research Council of Canada, Ottawa, Ontario/Canada

Abstract

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A new balloon collection technique, Magellan, for obtaining large cosmic dust particles > 50µ is described. The technique utilized a 40 m2 aperture funnel suspended 300 m below a balloon at an altitude of 25 km. First results indicate that the collected particles are diverse both chemically and physically.

Type
2 In Situ Measurements of Interplanetary Dust
Information
International Astronomical Union Colloquium , Volume 31: Interplanetary Dust and Zodiacal Light , 1976 , pp. 284 - 288
Copyright
Copyright © Springer-Verlag 1976

References

1. Hemenway, C. L. et al “New High Altitude Balloon Top Cosmic Dust Collection Technique”, Space Research XI, p. 393–395, Berlin, Akademie Verlag, 1971.Google Scholar
2. Wlochowicz, R. et al “Magellan – A Balloon-Borne Collection Technique for Large Cosmic Dust Particles”, submitted to Canadian J. of Physics, 1975.Google Scholar
3. Hemenway, C. L. et al “Near Earth Cosmic Dust Results from S-149”, AIAA/AGU, Conf. on Scientific Results from Skylab, 1974.CrossRefGoogle Scholar
4. Opik, E. J., “Physics of Meteor Flight in the Atmosphere”, Interscience, 1958.Google Scholar
5. Blanchard, M. B., et al “Artificial Meteor Studies: Olivine”, J. Geophysical Res., V. 79, No. 26, 1974.CrossRefGoogle Scholar