๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Dynamics of Quiescent Prominences

โœ Scribed by Vladimir Ruzdjak, Einar Tandberg-Hanssen

Book ID
127430294
Publisher
Springer
Year
1990
Tongue
English
Weight
2 MB
Series
LNP0363
Edition
1
Category
Library
ISBN-13
9783540529736

No coin nor oath required. For personal study only.

โœฆ Synopsis

For some time to come, this book should be the main source for research in prominences. It surveys the results of the past years, including the "Hvar Reference Atmosphere", which was developed by a panel as a model for quiescent prominences. The reader will find papers on the formation of and physical conditions in prominences, on magnetic fields, on mass motion and energy flow, and on the prominence-corona interface.

๐Ÿ“œ SIMILAR VOLUMES

Origin of quiescent prominences
Origin of quiescent prominences
โœ S. B. Pikel'ner ๐Ÿ“‚ Article ๐Ÿ“… 1971 ๐Ÿ› Springer ๐ŸŒ English โš– 370 KB

For stable equilibrium, prominences must be supported with magnetic lines of force leaning

Dynamical fine structure of a quiescent
Dynamical fine structure of a quiescent prominence
โœ P. Mein; N. Mein ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 931 KB

A quiescent prominence has been observed with the MSDP spectrograph at the Pic du Midi Observatory. He profiles are obtained simultaneously in a 2D field, allowing a statistical analysis. The standard deviations of Doppler shifts and line widths are investigated as functions of the line intensity. T

Velocity fields in quiescent prominences
Velocity fields in quiescent prominences
โœ Eberhart Jensen ๐Ÿ“‚ Article ๐Ÿ“… 1982 ๐Ÿ› Springer ๐ŸŒ English โš– 532 KB

Three quiescent prominences were observed in the Ca ~I K-line and a fourth one also in the H-line at Oslo Solar Observatory, Harestua, and reduced by Rustad (1974) and by Engvold et al. (1980). These data are used to study the distribution of the line-of-sight velocity component, N(uo). It is pointe