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Hα oscillations in sunspot umbrae

✍ Scribed by Gary L. Phillis


Publisher
Springer
Year
1975
Tongue
English
Weight
689 KB
Volume
41
Category
Article
ISSN
0038-0938

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✦ Synopsis


Direct measurement of intensity and photographic subtractions of simultaneous Doppler filtergrams at Hc~zk0.3 ,~ in a time-lapse sequence of McMath 11482 has shown velocity oscillations in sunspot umbrae. These oscillations exhibit the following characteristics: (a) A characteristic oscillation frequency for each umbra, with the periods ranging from 145:k10s to 180zkl0s. (b) A duration of at least 8 cycles. (c) A Doppler shift of 10 km s z. (d) An oscillating element size of 3" or less. (e) A visibility to a radius vector of about 0.9.


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