๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Observations of sunspot umbral velocity oscillations

โœ Scribed by Arvind Bhatnagar; W. C. Livingston; J. W. Harvey


Publisher
Springer
Year
1972
Tongue
English
Weight
383 KB
Volume
27
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis


Sunspot umbral molecular lines have been used to look for the oscillatory velocities in the umbra. Power spectrum analysis showed conspicuous power for periods in the range between 448 and 310 s. The maximum peak-to-peak amplitude of the umbral oscillatory velocity component is observed to be in the order of 0.5 km s 1.


๐Ÿ“œ SIMILAR VOLUMES


Sunspot umbral oscillations in Mgiik
โœ Joseph B. Gurman ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 853 KB

Time series observations of the profile of the Mgn k line 22795.52 have been obtained in five sunspots with the Ultraviolet Spectrometer and Polarimeter (UVSP) on the Solar Maximum Mission. The three sunspots with umbrae larger than the 3" x 3" pixel size show significant oscillations in integrated

The spectrum of umbral oscillations of t
โœ V. I. Zhukov; V. I. Efremov; B. T. Nuraliev ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 232 KB

Proper periods are calculated for oscillations of an isothermal gaseous layer with a homogeneous vertical magnetic field, limited by two rigid horizontal boundaries. The obtained results are in good agreement with the observed umbral oscillations in a sunspot.

Observations of the horizontal velocity
โœ N. R. Sheeley ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 676 KB

During the summer and fall of 1971, Doppler spectroheliograms were obtained for several sunspots located near the solar limb. These observations confirm a previous result based on the study of only a few sunspots that in the plage-free photosphere surrounding sunspots the spatiallyaveraged, horizont