Abstract
WE compare here the prediction of the coronal features made by Schatten1 with the photographic observation made by us in Yurgamish, Siberia.
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
Schatten, K. H., Nature, 220, 1211 (1968).
Laffineur, M., Bloch, M., and Bretz, M., CR Acad. Sci. Paris, No. 15, 2180 (1961).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
LAFFINEUR, M., BURNICHON, ML. & KOUTCHMY, S. Weighted Observation of the Corona during the Total Solar Eclipse of September 22, 1968. Nature 222, 461–462 (1969). https://doi.org/10.1038/222461a0
Received:
Issue date:
DOI: https://doi.org/10.1038/222461a0
This article is cited by
-
Solar eclipses as an astrophysical laboratory
Nature (2009)
-
Photometric Study of the Solar Corona
Nature (1970)
-
Prediction of the Coronal Structure for the Solar Eclipse of March 7, 1970
Nature (1970)
-
Magnetic fields and the solar corona
Solar Physics (1970)
