Field dependent cosmic ray streaming at high rigidities
Journal Article
·
· J. Geophys. Res.; (United States)
Data from underground ..mu.. meson telescopes at depths of 25, 40, and 80 mwe covering the period 1965--1973 have been analyzed as a function of interplanetary magnetic field direction. Cosmic ray streaming both in and perpendicular to the ecliptic plane, with directions dependent on the sense of the interplanetary magnetic field, is observed throughout the period at all depths. The field dependent streaming in the ecliptic plane exhibits some variability in amplitude and phase but contains a component in the direction perpendicular to the interplanetary magnetic field direction which is consistent with B x delN streaming due to a perpendicular cosmic ray density gradient pointing southward (higher density below the ecliptic plane than above it). In the case of the field dependent streaming perpendicular to the ecliptic plane the direction of the streaming has remained remarkably consistent over the 9-year period. One possible source of this streaming is B x delN streaming due to a radial heliocentric cosmic ray density gradient; this possibility is discussed along with other possible sources. There does not appear to be an obvious variation in the amplitude of the field dependent streaming either in or perpendicular to the ecliptic plane with increasing rigidity; both effects are still apparent at rigidities well above the 52-GV threshold rigidity of the Socorro 80-mwe telescope. The amplitudes of both anisotropies appear larger at solar maximum than at solar minimum. (AIP)
- Research Organization:
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131
- OSTI ID:
- 7270201
- Journal Information:
- J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 81:13; ISSN JGREA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Cosmic ray density gradients related to north-south asymmetry in activity on the sun
Three-dimensional structure of relativistic galactic cosmic ray anisotropies associated with solar rotation
Long-term variations of the cosmic ray north-south anisotropy and the radial cosmic ray gradient at high rigidity
Journal Article
·
Fri Feb 28 23:00:00 EST 1986
· J. Geophys. Res.; (United States)
·
OSTI ID:5875546
Three-dimensional structure of relativistic galactic cosmic ray anisotropies associated with solar rotation
Journal Article
·
Fri Mar 14 23:00:00 EST 1980
· Astrophys. J.; (United States)
·
OSTI ID:5364296
Long-term variations of the cosmic ray north-south anisotropy and the radial cosmic ray gradient at high rigidity
Journal Article
·
Wed Jun 01 00:00:00 EDT 1988
· J. Geophys. Res.; (United States)
·
OSTI ID:6907888
Related Subjects
640101* -- Astrophysics & Cosmology-- Cosmic Radiation
640104 -- Astrophysics & Cosmology-- Solar Phenomena
640107 -- Astrophysics & Cosmology-- Planetary Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AMPLITUDES
ANISOTROPY
BEAM DYNAMICS
CHARGED PARTICLE DETECTION
COSMIC RADIATION
INTERPLANETARY MAGNETIC FIELDS
IONIZING RADIATIONS
MAGNETIC FIELDS
MUON DETECTION
OSCILLATIONS
PHASE OSCILLATIONS
RADIATION DETECTION
RADIATIONS
SOLAR RADIATION
640104 -- Astrophysics & Cosmology-- Solar Phenomena
640107 -- Astrophysics & Cosmology-- Planetary Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AMPLITUDES
ANISOTROPY
BEAM DYNAMICS
CHARGED PARTICLE DETECTION
COSMIC RADIATION
INTERPLANETARY MAGNETIC FIELDS
IONIZING RADIATIONS
MAGNETIC FIELDS
MUON DETECTION
OSCILLATIONS
PHASE OSCILLATIONS
RADIATION DETECTION
RADIATIONS
SOLAR RADIATION