Shah, G. A. ; Krishna Swamy, K. S. (1988) Nature of dust grains in comets Monthly Notices of the Royal Astronomical Society, 233 . pp. 573-579. ISSN 0035-8711
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Official URL: http://onlinelibrary.wiley.com/journal/10.1111/%28...
Abstract
The observed reddening in the wavelength range 0.26-2.25 microns for comae of several comets can be represented quite well with model grains having real and imaginary parts of refractive index, m = m-prime - im-double prime, given by m-prime of about 1.38 and m-double prime of about 0.039, respectively. It is also possible to explain the observations of linear polarization and geometric albedo of comet comae.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to John Wiley and Sons. |
| ID Code: | 87415 |
| Deposited On: | 19 Mar 2012 06:48 |
| Last Modified: | 19 Mar 2012 06:48 |
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