Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-02T18:52:15.809Z Has data issue: false hasContentIssue false
  • English
  • Français

Solar: Fine Structure of the Flare of 1968 June 9

Published online by Cambridge University Press:  25 April 2016

R. G. Giovanelli
R. G. Giovanelli*
Affiliation:
Division of Physics, CSIRO, Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

A class 2 flare began on 1968 June 9 in the active region near 17°N 40°E, at about 00h15m U.T., maximum 00h37m, terminating about 02h30m. The event was recorded at Culgoora with the 5-inch flare-patrol and 12-inch chromo-spheric telescopes at solar diameters and frame intervals of 16 mm/10 s and 17 cm/3 s respectively. Both telescopes used Halle filters, pass bands about 0.5Å centred on Hα, and Duplopan 35 mm film. The seeing was mediocre, with occasional fairly good frames.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 184 - 185
Copyright
Copyright © Astronomical Society of Australia 1969

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Bruzek, A., Zeits. f. Astrophys., 54, 225 (1962).Google Scholar
2 Bruzek, A., AAS-NASA Symposium on Solar Flares, p. 301 (1963).Google Scholar
3 Bruzek, A., Astrophys. J., 140, 746 (1964).Google Scholar
4 Leighton, R. B., Astrophys. J., 130, 366 (1959).Google Scholar