Abstract
DETERMINATION of vertical distributions of ozone from lunar eclipse observations1 suggests the practicability of similar ground-based, optical methods, provided ‘screens’ more amenable to experimental control than the Moon can be used. Alternatives are noctilucent clouds, atmospheric layers, balloons, and artificial Earth satellites. Noctilucent clouds are rather rare and beyond experimental control; ionospheric layers give very limited information2, as do other atmospheric layers such as sodium3. Following a suggestion by Dr. V. D. Hopper of this Department, a method analogous to the lunar eclipse method has therefore been developed in Melbourne, for initial application to ground-based filter photometric observations of balloons at twilight.
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 Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Paetzold, H. K., J. Atmos. Terr. Phys., 2, 183 (1952).
Penndorf, R., J. Met., 5, 152 (1948).
Dufay, J., C.R. Acad. Sci., Paris, 225, 690 (1947).
Laby, J., Lim, Y. K., and Hopper, V. D., Nuo Cim. (X), 5, 249 (1957).
Dufay, J., Ann. Astrophys., 5, 93 (1942).
Khvostikov, I. A., Uspekhi Fiz. Nauk, 49, 229 (1956).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
PITTOCK, A. A Twilight Method of determining the Vertical Distribution of Ozone. Nature 190, 426–427 (1961). https://doi.org/10.1038/190426a0
Issue Date:
DOI: https://doi.org/10.1038/190426a0
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.