Sidereal cosmic ray variation and its relation with the interplanetary magnetic field polarity

Contenido principal del artículo

Javier A. Otaola

Resumen

Datos de la componente mesónica de la intensidad de la radiación cósmica, registrada a diferentes profundidades, han sido comparados con las predicciones del modelo propuesto por Swinson. Las observaciones en la superficie y a profundidades moderadas muestran un efecto dependiente de la polaridad del campo del tipo propuesto por Swinson. Las observaciones a profundidades mayores de 40 metros de agua equivalente no muestran dicho efecto. Se da una explicación en términos de la función de respuesta del detector. La pequeña variación sideral observada a 60 metros de agua equivalente se explica en base al movimiento del sistema solar relativo a estrellas cercanas.

Publication Facts

Metric
This article
Other articles
Peer reviewers 
2,4 promedio

Reviewer profiles  N/D

Author statements

Author statements
This article
Other articles
Data availability 
N/A
16%
External funding 
N/D
32% con financiadores
Competing interests 
N/D
11%
Metric
Para esta revista
Other journals
Articles accepted 
Artículos aceptados: 2%
33% aceptado
Days to publication 
17661
145

Indexado: {$indexList}

Editor & editorial board
profiles
Academic society 
Geofísica Internacional

Detalles del artículo

Cómo citar
Otaola, J. A. (1974). Sidereal cosmic ray variation and its relation with the interplanetary magnetic field polarity. Geofísica Internacional, 14(4), 317–328. https://doi.org/10.22201/igeof.00167169p.1974.14.4.966
Sección
Artículo

Citas

AHLUWALIA, H. S., 1971. Median primary energy of response of a cosmic ray telescope underground, J. Geophys. Res., 76 : 5358-5360. DOI: https://doi.org/10.1029/JA076i022p05358

AHLUWALIA, H. S. and J. H. ERIKSEN, 1971. Coupling functions applicable to the underground meson telescopes, J. Geophys. Res., 76 : 6613-6627. DOI: https://doi.org/10.1029/JA076i028p06613

DUTT, 1. C., 1965. Variations of underground cosmic ray intensity with time, Ph. D. Thesis, University of London.

ELLIOT, H., T. THAMBYAHPILLAI and D. S. PEACOCK, 1970. Search for a sidereal anisotropy at 60 m. w. e. depth, Acta Phys. Hung., 29 (2) : 491-500.

ELLIOT, H., T. THAMBYAHPILLAI and J. A. OTAOLA, 1972. Comment on a paper by D. B. Swinson, "Solar Modulation Origin of Sidereal Cosmic Ray Anisotropies", J. Geophys. Res., 77 : 1342-1344. DOI: https://doi.org/10.1029/JA077i007p01342

HUMBLE, J. E., A. G. FENTON, R. D. SPELLER, J. A. OTAOLA, T. THAMBYAHPILLAI, J. C. DUTI, T. MATHEWS, T. MIYAZAKI and D. S. PEACOCK, 1973. Underground cosmic ray observations and interplanetary magnetic field directions. Proc. Internal. Cosmic Ray Conf., Denver. Vol. 2, 976-981.

LENTS, G. A., R. B. MCKIBBEN, J. J. O'GALLAGHER, M. PERKINS, J. A. SIMPSON and A. J. TUZZOLINO, Proc. 13 Int. Cosmic Rays Conf., Denver Colorado, 1973.

MIYAZAKI, T., 1973. Private communication.

NAGASHIMA, K., H. UENO, S. MORI and S. SAGISAKI, 1968. A two-way sidereal anistropy, Can, J. Phys., 46 : 5611. DOI: https://doi.org/10.1139/p68-307

OTAOLA, J. A., 1973. Terrestrial effects of the interplanetary magnetic field sector structure, Ph. D. Thesis, Unviersity of London.

PEACOCK, D. S., 1967. Solar and sidereal daily variations of the cosmic ray intensity observed underground. Ph. D. Thesis, University of London.

PEACOCK, D. S., 1970. Underground response functions and the upper limiting rigidity to solar modulation, Acta Phys. Hung., 29 (2) : 189-194.

SPELLER, R., T. THAMBYAHPILLAI and H. ELLIOT, 1972. Cosmic ray isotropy and the origin problem, Nature, 235 : 25-29. DOI: https://doi.org/10.1038/235025a0

SVALGAARD, L., 1972. Interplanetary magnetic -sector structure 1926-1971, J. Geophys. Res., 77 : 4027-4034. DOI: https://doi.org/10.1029/JA077i022p04027

SWINSON, D. B., 1969. "Sidereal" cosmic-ray diurnal variations, J. Geophys. Res., 74 : 5591-5598. DOI: https://doi.org/10.1029/JA074i024p05591

SWINSON, D. B., 1971. Solar modulation origin of "sidereal" cosmic ray anisotropies, J. Geophys. Res., 76 : 4217-4223. DOI: https://doi.org/10.1029/JA076i019p04217

THOMSON, D. M., 1973. The heliocentric radial gradient in cosmic ray density and the 'Swinson' sidereal time variation, Planet. Space Sci., 21 : 133-143. DOI: https://doi.org/10.1016/0032-0633(73)90025-1

WILCOX, J. M. and D. S. COLBURN, 1969. Interplanetary sector structure in the rising portion of the sunspot cycle, J. Geophys. Res., 74 : 2383-2392. DOI: https://doi.org/10.1029/JA074i009p02388

WILCOX, J. M. and D. S: COLBURN, 1 ~70. Interplanetary sector structure near the maximum of the sunspot cycle, J. Geophys. Res., 75 : 6366-6370. DOI: https://doi.org/10.1029/JA075i031p06366

WILCOX, J. M. and D. S. COLBURN, 1972. Interplanetary sector structure at solar maximum, J. Geophys. Res., 77 : 751-756. DOI: https://doi.org/10.1029/JA077i004p00751