Cosmic ray unidirectional latitude gradient: Evidence for north-south asymmetric solar modulation
Journal Article
·
· Journal of Geophysical Research; (United States)
- Univ. of Delaware, Newark, NJ (USA)
The cosmic ray diurnal anisotropy is determined separately in toward and away sectors of the interplanetary magnetic field through analysis of neutron monitor records spanning the period 1953-1988. The authors suggest that the dominant cause of differences (between sectors) of the anisotropy is a unidirectional latitude gradient, which is indicative of a north-south asymmetry in the solar modulation of cosmic rays. The magnitude of the latitude gradient deduced from the observations is typically of the order of 0.7%/AU, and its direction varies in a manner not obviously related to either the 11-year sunspot cycle or the 22-year solar magnetic cycle. Further support for the reality of a unidirectional gradient is provided by an analysis of the cosmic ray density segregated according to sector polarity. The density is found to differ significantly in the two sector types, and the amount of difference is correlated with the concurrently measured unidirectional latitude gradient in the expected manner. They examine two hypotheses to account for a north-south asymmetry of solar modulation: (1) that the asymmetric modulation results from a north-south asymmetry in the winding angle of the interplanetary magnetic field spiral and (2) that the asymmetric modulation is related to a corresponding north-south asymmetry of solar activity as indicated by sunspot number. Both hypotheses are consistent with the data, suggesting that multiple factors may give rise to north-south asymmetric solar modulation.
- OSTI ID:
- 5226291
- Journal Information:
- Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 96:A7; ISSN 0148-0227; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Geomagnetic activity and north-south asymmetry of cosmic rays circa 1 GV. Final report, 1 March 1977-30 September 1984
Latitudinal cosmic ray gradients: Their relation to solar activity asymmetry
THE LATITUDE DISTRIBUTION OF SMALL-SCALE MAGNETIC ELEMENTS IN SOLAR CYCLE 23
Technical Report
·
Fri Sep 26 00:00:00 EDT 1986
·
OSTI ID:6846100
Latitudinal cosmic ray gradients: Their relation to solar activity asymmetry
Journal Article
·
Thu Jan 31 23:00:00 EST 1991
· Journal of Geophysical Research; (United States)
·
OSTI ID:5194880
THE LATITUDE DISTRIBUTION OF SMALL-SCALE MAGNETIC ELEMENTS IN SOLAR CYCLE 23
Journal Article
·
Thu Jan 19 23:00:00 EST 2012
· Astrophysical Journal
·
OSTI ID:22012001
Related Subjects
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANISOTROPY
ASYMMETRY
COSMIC RADIATION
COSMIC RAY FLUX
DAILY VARIATIONS
INTERPLANETARY MAGNETIC FIELDS
IONIZING RADIATIONS
MAGNETIC FIELDS
MEASURING INSTRUMENTS
MODULATION
MONITORS
NEUTRON MONITORS
RADIATION FLUX
RADIATION MONITORS
RADIATIONS
SOLAR ACTIVITY
VARIATIONS
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANISOTROPY
ASYMMETRY
COSMIC RADIATION
COSMIC RAY FLUX
DAILY VARIATIONS
INTERPLANETARY MAGNETIC FIELDS
IONIZING RADIATIONS
MAGNETIC FIELDS
MEASURING INSTRUMENTS
MODULATION
MONITORS
NEUTRON MONITORS
RADIATION FLUX
RADIATION MONITORS
RADIATIONS
SOLAR ACTIVITY
VARIATIONS