๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Structure of the interplanetary magnetic clouds and their solar origins

โœ Scribed by K. Marubashi


Publisher
Elsevier Science
Year
1986
Tongue
English
Weight
345 KB
Volume
6
Category
Article
ISSN
0273-1177

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


On the three-dimensional structure of th
โœ Osamu Kaburaki; Yuzuru Yoshii ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 487 KB

The three-dimensional structure of the solar magnetic field in the interplanetary space is inferred from a theoretical point of view. We use the magnetic field produced by a magnetic dipole rotating obliquely in vacuum. The correction for the presence of a plasma surrounding the Sun is taken into ac

Observation of sectored structure in the
โœ R. A. Howard; M. J. Koomen ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 433 KB

Daily images of the white light corona between 3 and 10 R| have been recorded by a coronagraph aboard the OSO-7 unmanned satellite since October 3, 1971. Images for the years 1972 and 1973 have been examined for persistent coronal forms. For most of 1972 there passed over the Sun's east limb a regul

Recurrency and the origin of the vertica
โœ M. I. Pudovkin; D. I. Ponyavin; A. D. Chertkov ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Springer ๐ŸŒ English โš– 354 KB

The autocorrelation functions of the solar wind velocity and of the IMF components as well as of the geomagnetic activity indices are studied for two periods: August-December, 1965 and January-May, 1974. The vertical component of the IMF is shown to exhibit a rather definite recurrency relatively in