๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Time-evolution of cosmic-ray intensity modulation

โœ Scribed by J. Xanthakis; H. Mavromichalaki; B. Petropoulos


Publisher
Springer
Year
1989
Tongue
English
Weight
754 KB
Volume
122
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Time-lag of cosmic-ray intensity
โœ H. Mavromichalaki; B. Petropoulos ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 580 KB
Study and effect of magnetic clouds on t
โœ Badruddin; D. Venkatesan; B. Y. Zhu ๐Ÿ“‚ Article ๐Ÿ“… 1991 ๐Ÿ› Springer ๐ŸŒ English โš– 391 KB

Data of cosmic-ray intensity from the Calgary Super Neutron Monitor and interplanetary plasma and field data are divided into three groups corresponding to the magnetic clouds preceded by shocks, followed by interaction region and clouds without any such association, observed during the period 1967-

A study of the modulating effect of sola
โœ G. A. Bowe; C. J. Hatton ๐Ÿ“‚ Article ๐Ÿ“… 1982 ๐Ÿ› Springer ๐ŸŒ English โš– 417 KB

The cosmic ray 11-year variation for solar cycle 20 is attributed to the modulating effect of solar flare-induced shocks propagating through the interplanetary medium to the boundary of the heliosphere. The relative influence of these disturbances upon the cosmic ray intensity as a function of their

Time evolution of cosmic-ray intensity a
โœ H. Mavromichalaki; P. Preka-Papadema; B. Petropoulos; A. Vassilaki; I. Tsagouri ๐Ÿ“‚ Article ๐Ÿ“… 2003 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 404 KB

Analysis of the time series into trigonometric series allows the investigation of cosmic-ray (CR) intensity variations in a range of periodicities from a few days to 1 year. By this technique the amplitude and the phase of all observed uctuations can be given. For this purpose, daily CR intensity va