Abstract
THERE has been for three weeks past a very remarkable renewal of the afterglow. There is a quite deep secondary red glow after the stars are fully out. I should say that no such afterglow has been seen since 1886, or three years after the Krakatsão eruption. There is also a great extension of the white hazy atmospheric corona around the sun, very marked also around the moon. I am unable, however, to make out any of the pink colour on the outer edge of the haze, which was so charcteristic of “Bishop's Ring,” and distinguishable at Honolulu for two years. Apparently there has recently been a great reinforcement added to the material in the upper atmosphere, which produces the afterglows.
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
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
BISHOP, S. The Afterglow. Nature 47, 102–103 (1892). https://doi.org/10.1038/047102d0
Issue Date:
DOI: https://doi.org/10.1038/047102d0
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.