𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Implications of observations of the solar wind and corona for solar wind models

✍ Scribed by W. I. Axford; J. F. McKenzie


Publisher
Springer Netherlands
Year
1996
Tongue
English
Weight
187 KB
Volume
243
Category
Article
ISSN
0004-640X

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


The green corona, the solar wind and geo
✍ J. SΓ½kora πŸ“‚ Article πŸ“… 1992 πŸ› Springer 🌐 English βš– 783 KB

The long-term distribution of the Green Corona Low Brightness Regions (GCLBR\*) on the solar surface is investigated. The frequency curves of the GCLBR follow the solar cycle, but are displaced considerably relative to the curve of the sunspot number cycle. The observed displacement increases with t

Observation of solar wind heavy ions
✍ M. B. Cattaneo; V. Formisano; G. Moreno; F. Palmiotto; F. Palutan; P. Saraceno πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 197 KB

Plasma experiment on board of the ESRO satellite HEOS-1 observed heavy ions with energy per unit charge 2.5 and 4 times higher than protons. Observations refer to the driving piston of the interplanetary shock occurred on 31 March 1970. \* Laboratorio per le Radiazioni Extraterrestri del C. N. R., B

A plasmoid model for the solar wind
✍ Teruo Tamano πŸ“‚ Article πŸ“… 1991 πŸ› Springer 🌐 English βš– 714 KB

A model describing magnetized plasmoids as a possible origin of the solar wind is discussed. The magnetized plasmoids are assumed to be created and accelerated to a very high speed through reconnection processes from small-scale magnetic loops. Afterward, the plasmoids are considered to be nearly in