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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

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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
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