Abstract
CONSIDERABLE efforts have been made by many workers1 to obtain meteor spectra. From the earlier observations it has been established that all meteor spectra from each shower are remarkably similar to each other, having the same general features within the limitations of photographic resolution and emulsion sensitivity2.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on SpringerLink
- Instant access to the full article PDF.
USD 39.95
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Halliday, Ian, J. Roy. Astro. Soc. Canada, 52, 169 (1958).
Millman, P. M., paper presented at the Eighty-first Meeting of the Amer. Astro. Soc., Ottawa, June 19–23, 1949.
Millman, P. M., Sky and Tel., 15, 375 (1956).
Millman, P. M., J. Roy. Astro. Soc. Canada, 54, 189 (1960).
Whipple, F. L., Astrophys. J., 111, 375 (1950).
Millman, P. M., Nature, 172, 853 (1953).
Moore, C. E., Contr. Princeton Univ. Obs., No. 20 (1945).
Millman, P. M., Ann. Astro. Obs. Harvard Coll., 82, No. 6 (1932).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
RAO, M., LOKANADHAM, B. A Typical Leonid Meteor Spectrum. Nature 197, 169–170 (1963). https://doi.org/10.1038/197169a0
Issue date:
DOI: https://doi.org/10.1038/197169a0
This article is cited by
-
Wake Spectrum of a Leonid Meteor
Nature (1963)
-
Spectra of Meteor Wakes
Nature (1963)
-
Spectra of Meteor Wakes
Nature (1963)


