Center-limb observations of line-center intensity fluctuations in the Na D and Na 5688 doublets and the Mg 4571 line are described. For small scale structures the rms distributions for the photospheric lines show maxima of 20% at a heliocentric angle of 40 ~ (Mg 4571) and 9% at 20 ~ (Na 5688). The r
โฆ LIBER โฆ
Fine Structure of the solar atmosphere from near-limb observations in three wavelengths
โ Scribed by A. A. Georgakilas; H. Dara; Th. Zachariadis; C. E. Alissandrakis; S. Koutchmy
- Book ID
- 110217235
- Publisher
- Springer
- Year
- 1997
- Tongue
- English
- Weight
- 369 KB
- Volume
- 172
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Center limb observations of inhomogeneit
โ
C. J. Cannon; P. R. Wilson
๐
Article
๐
1971
๐
Springer
๐
English
โ 899 KB
The height structure of solar active reg
โ
J. M. Mosher
๐
Article
๐
1979
๐
Springer
๐
English
โ 585 KB
Observation in the wing of the Hฮฑ line a
โ
S. Koutchmy; C. Macris
๐
Article
๐
1971
๐
Springer
๐
English
โ 553 KB
Fine structure of wave motions in the so
โ
R. I. Kostyk; N. G. Shchukina; E. V. Khomenko
๐
Article
๐
2006
๐
Springer
๐
English
โ 694 KB
Fine structure of convective motions in
โ
R. I. Kostyk; N. G. Shchukina
๐
Article
๐
2004
๐
Springer
๐
English
โ 298 KB
Observations of solar chromospheric fine
โ
William A. Sloan
๐
Article
๐
1968
๐
Springer
๐
English
โ 806 KB
A Cassegrain telescope with a resolution of 2 sec of arc was successfully flown in an Aerobee-150 rocket from White Sands Missile Range on October 20, 1965. A pinhole, 33/t in diameter, was placed at the focus of the telescope, followed by a photo-ionization detector with a lithium-fluoride window.