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A High-Velocity Component of Atomic Hydrogen in Comet Bennett (1970 II)

Published online by Cambridge University Press:  22 February 2018

Extract

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The Lyman alpha emission from Comet Bennett (1970II) was measured near perihelion (March 1970) by the University of Colorado ultraviolet photometer experiment on OGO-5 The spectrometer field of view of about 3° crossed the cometary hydrogen coma four times. The hydrogen coma was observed to extend more than 30 x 106 km in the antisolar direction.

A model for the hydrogen density was developed which took the actual cometary motion and the gradients of the forces of gravitation and radiation pressure into account Exact trajectories of atoms in the orbital plane representing the column densities perpendicular to the plane were calculated. The variation of the hydrogen lifetime along the trajectory as well as the solar Lα profile were considered.

Type
Part I
Copyright
Copyright © NASA 1976

References

Bertaux, J. L., Blamont, J. E., Festou, M. 1973, Astron and Astrophys. 25, 415.Google Scholar
Haser, L. 1966, Les Congres et Collogues de l'Universite de Liege 37, 233.Google Scholar
Keller, H. U. 1971, Mitt Astron Ges 30, 143.Google Scholar
Keller, H. U. 1973a, Astron. and Astrophys 23, 269.Google Scholar
Keller, H. U. 1973b, Astron. and Astrophys 27, 51.Google Scholar
Keller, H. U., Thomas, G. E. 1975, Astron and Astrophys 39, 7.Google Scholar