๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Fine structure of wave motions in the solar photosphere: Observations and theory

โœ Scribed by R. I. Kostyk; N. G. Shchukina; E. V. Khomenko


Book ID
110216290
Publisher
Springer
Year
2006
Tongue
English
Weight
694 KB
Volume
50
Category
Article
ISSN
1063-7729

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Wave behavior in the solar photosphere:
โœ Ciro Marmolino; Robin T. Stebbins ๐Ÿ“‚ Article ๐Ÿ“… 1989 ๐Ÿ› Springer ๐ŸŒ English โš– 790 KB

We report detailed comparisons between theoretical and empirical eigenfunctions of velocity and intensity for the 5-min modes in the photosphere. The comparison process is accomplished by obtaining synthetic profiles of the FeI 25434 ~ line in the presence of waveforms given by dynamical calculation

Absolute wavelengths of Fraunhofer lines
โœ D. L. Lambert; E. A. Mallia ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 345 KB

Absolute wavelengths for Fraunhofer lines are compared with laboratory measurements for several atomic and molecular spectra. The wavelength differences are shown to be consistent with the proposal that the deeper layers of the photosphere are in convective motion: ve -~ 3 km/sec for log To> --1.0.

Observations of solar chromospheric fine
โœ William A. Sloan ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 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.

Cyclotron wave instability in the corona
โœ V. V. Zheleznyakov; E. Ya. Zlotnik ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 928 KB

The longitudinal waves (Bernstein modes and plasma waves near the hybrid frequency) in a mixture of equilibrium coronal plasma and a small group of energetic electrons are investigated. The energetic electrons have a nonequilibrium momentum distribution inherent in trapped particles. The frequency d