ASYMMETRY IN THE RECOVERY FROM A VERY DEEP FORBUSH-TYPE DECREASE IN COSMIC- RAY INTENSITY
Journal Article
·
· Canadian Journal of Physics (Canada)
The intensity-time curves for cosmic rays recorded at some 30 stations distributed all over the world are examined for structure in the recovery period from the third in a series of three closely spaced Forbush type decreases which occurred in the middle of July 1959. It is shown that the structure of mtensity peaks is regular and that these occur at each station at the same effective local time. It is fourd that this is consistent with the hynethesis that recovery from a very deep Forbush type decrease is first apparent in directions making 15 and 165 deg with the sun-earth line, respectively. The analyses suggest further that during recovery from this deep Forbush decrease, temporary openings appeared in the intensity depressing mechanism which allowed intensity increases in limited directions. (auth)
- Research Organization:
- National Research Council, Ottawa
- Sponsoring Organization:
- USDOE
- NSA Number:
- NSA-15-011896
- OSTI ID:
- 4081471
- Report Number(s):
- NRC-6133; 0008-4204
- Journal Information:
- Canadian Journal of Physics (Canada), Journal Name: Canadian Journal of Physics (Canada) Vol. Vol: 39; ISSN CJPHA
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
Similar Records
ASYMMETRIES IN THE FORBUSH DECREASES OF THE COSMIC RADIATION. 2. SUPERIMPOSED INTENSITY VARIATIONS DURING A FORBUSH DECREASE
THE COSMIC RAY ALPHA-PARTICLE FLUX DURING SHARP FORBUSH INTENSITY DECREASES
The Onset Times of Forbush-Type Cosmic Ray Intensity Decreases
Journal Article
·
Thu Mar 14 23:00:00 EST 1963
· Journal of Geophysical Research (U.S.)
·
OSTI ID:4743901
THE COSMIC RAY ALPHA-PARTICLE FLUX DURING SHARP FORBUSH INTENSITY DECREASES
Journal Article
·
Wed Nov 30 23:00:00 EST 1960
· J. Geophys. Research
·
OSTI ID:4083947
The Onset Times of Forbush-Type Cosmic Ray Intensity Decreases
Journal Article
·
Tue Sep 01 00:00:00 EDT 1959
· Canadian Journal of Physics
·
OSTI ID:4197715