๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Coupling of the coronal he abundance to the solar wind

โœ Scribed by V. H. Hansteen; E. Leer; T. E. Holzer


Publisher
Springer Netherlands
Year
1994
Tongue
English
Weight
411 KB
Volume
70
Category
Article
ISSN
0038-6308

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


The abundance of3He in the solar wind -
โœ P. Bochsler; J. Geiss; A. Maeder ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer ๐ŸŒ English โš– 724 KB

3He is an intermediate product in the proton-proton chain, and standard models of the Sun predict a large bulge of enhanced 3He abundance near Mr/M o = 0.6 in the contemporary Sun. The relatively low abundance of 3He at the solar surface, which is derived from solar wind observations, poses severe c

The coronal source of the slow solar win
โœ Henrik Lundstedt ๐Ÿ“‚ Article ๐Ÿ“… 1989 ๐Ÿ› Springer ๐ŸŒ English โš– 369 KB

Periods of very low solar wind velocity at 1 AU, during the interval from 1977 to 1983, are identified and mapped back to the coronal source surface at 2.5 R o. In total 25 such low-velocity events were found. Inferred source locations were characterized with respect to their position relative to th

Variations of ฮฑ-particle abundance in th
โœ G. Moreno; F. Palmiotto ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 148 KB

The existence of a long-term variation, related to the solar activity, of the average a-particle abundance in the solar wind has been suggested by Robbins et al. (1970) and recently confirmed by Bollea et al. (1972) andOgilvie (1972). Hirshberg et al. (1972b), comparing the distribution of the a-par