Galactic cosmic-ray anisotropy and its heliospheric modulation, inferred from the sidereal semidiurnal variations observed in the rigidity range 300–600 GV with multidirectional muon telescope at Sakashita underground station
- 31 December 1991
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 39 (12) , 1637-1655
- https://doi.org/10.1016/0032-0633(91)90025-6
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- Cosmic-ray sidereal daily variation of galactic origin to be observed with existing underground muon telescopesPlanetary and Space Science, 1990
- The polar heliospheric magnetic fieldGeophysical Research Letters, 1989
- A theory of cosmic ray anisotropies of solar originPlanetary and Space Science, 1986
- Measurement of the cosmic-ray sidereal anisotropy near 1500 GVThe Astrophysical Journal, 1981
- Sector structure of the interplanetary magnetic field and anisotropy of 50–1000 GV cosmic raysAstrophysics and Space Science, 1980
- Ultraviolet observations of cool stars. VII - Local interstellar hydrogen and deuterium Lyman-alphaThe Astrophysical Journal, 1978
- An interpretation of Mariner 10 helium (584 A) and hydrogen (1216 A) interplanetary emission observationsThe Astrophysical Journal, 1978
- The directional dependence of the primary cosmic rays of energies 1011 – 1012 eVNature, 1976
- Studies of solar magnetic fieldsSolar Physics, 1974
- Evidence for a Two-Way Sidereal Anisotropy in the Charged Primary Cosmic RadiationNature, 1966