We report on studies of the k 1393 line of Si ix, lormed in the transition region at about 8(I 000 K, made using the Colorado experiment on OSO-8. Results indicate that the line width is somewhat greater in coronal holes compared to the quiet Sun, implying a dilterence in the broadening mechanism. T
Chromospheric oscillations observed in the line Ciiλ1336 with OSO-8
✍ Scribed by Eric G. Chipman
- Book ID
- 104644693
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 473 KB
- Volume
- 55
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
✦ Synopsis
Satellite observations of velocity and intensity oscillations were made of the upper chromospheric line C tt A 1336. The dominant period of oscillation is 300 s, with little evidence of the power peak in the range 150-200 s which has been observed in other chromospheric lines. Peak-to-peak amplitudes are 2 km s -a and 8% in velocity and intensity, respectively. Tentative evidence for 900-s periodicity is presented. Relative phase measurements show that maximum intensity for the 300-s oscillation leads maximum blueshift by approximately 145 s. Comparison of line and background (scattered light) intensity variation shows upward wave propagation, with time delays between the A 1800 continuum and C t~ A1336 variation of 27 s and 70 s for different cases.
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