dor_id: 4141280

506.#.#.a: Público

590.#.#.d: Los artículos enviados a la revista "Geofísica Internacional", se juzgan por medio de un proceso de revisión por pares

510.0.#.a: Consejo Nacional de Ciencia y Tecnología (CONACyT); Scientific Electronic Library Online (SciELO); SCOPUS, Dialnet, Directory of Open Access Journals (DOAJ); Geobase

561.#.#.u: https://www.geofisica.unam.mx/

650.#.4.x: Físico Matemáticas y Ciencias de la Tierra

336.#.#.b: article

336.#.#.3: Artículo de Investigación

336.#.#.a: Artículo

351.#.#.6: http://revistagi.geofisica.unam.mx/index.php/RGI

351.#.#.b: Geofísica Internacional

351.#.#.a: Artículos

harvesting_group: RevistasUNAM

270.1.#.p: Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

590.#.#.c: Open Journal Systems (OJS)

270.#.#.d: MX

270.1.#.d: México

590.#.#.b: Concentrador

883.#.#.u: https://revistas.unam.mx/catalogo/

883.#.#.a: Revistas UNAM

590.#.#.a: Coordinación de Difusión Cultural

883.#.#.1: https://www.publicaciones.unam.mx/

883.#.#.q: Dirección General de Publicaciones y Fomento Editorial

850.#.#.a: Universidad Nacional Autónoma de México

856.4.0.u: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/1686/1839

100.1.#.a: Ahluwalia, H. S.; Escobar V., I.

524.#.#.a: Ahluwalia, H. S., et al. (1963). The cosmic ray intensity variations and the electromagnetic states of the interplanetary space. Geofísica Internacional; Vol. 3 Núm. 2: Abril 1, 1963; 21-41. Recuperado de https://repositorio.unam.mx/contenidos/4141280

245.1.0.a: The cosmic ray intensity variations and the electromagnetic states of the interplanetary space

502.#.#.c: Universidad Nacional Autónoma de México

561.1.#.a: Instituto de Geofísica, UNAM

264.#.0.c: 1963

264.#.1.c: 1963-04-01

653.#.#.a: Radiación cósmica; Rayos cósmicos; Espacio interplanetario; Viento solar; Cosmic radiation; Cosmic rays; Interplanetary space; Solar wind

506.1.#.a: La titularidad de los derechos patrimoniales de esta obra pertenece a las instituciones editoras. Su uso se rige por una licencia Creative Commons BY-NC-SA 4.0 Internacional, https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es, para un uso diferente consultar al responsable jurídico del repositorio por medio del correo electrónico revistagi@igeofisica.unam.mx

884.#.#.k: http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/1686

001.#.#.#: 063.oai:revistagi.geofisica.unam.mx:article/1686

041.#.7.h: spa

520.3.#.a: Changes in the electromagnetic states of the interplanetary space produce temporal fluctuations in cosmic ray intensity as observed on the Earth. The changes in the interplanetary electromagnetic states are, on the other hand, brought about by solar wind. The study of cosmic ray intensity variations, therefore, provides an easy way to obtain information with respect to the parameters that characterize the solar wind at any given time. Evidence available from the study of quiet day solar diurnal variation of cosmic rays indicates that solar diurnal variation of cosmic rays indicates that solar wind velocity is usually above 100 Km/sec and that the wind velocity undergoes a 22·year cyclic change. Also it is demonstrated that the shift to earlier hours of the time of maximum of disturbed day solar diurnal variation observed during early stages of the cosmic ray storms enables one to choose between Parker"s "blast wave" model and the "magnetic tongue" model advocated by Gold and others for the configuration of interplanetary magnetic field obtainable on geomagnetically disturbed days. Observations fit the blast wave model better. A qualitative model, in which solar wind plays a major role, is presented to explain the gross features of the secular variation of isotropic intensity of cosmic rays in terms of currently most accepted ideas. The model requires that the interplanetary magnetic field should extend over a distance amounting to several tens of astronomic units from the Sun.

773.1.#.t: Geofísica Internacional; Vol. 3 Núm. 2: Abril 1, 1963; 21-41

773.1.#.o: http://revistagi.geofisica.unam.mx/index.php/RGI

022.#.#.a: ISSN-L: 2954-436X; ISSN impreso: 0016-7169

310.#.#.a: Trimestral

300.#.#.a: Páginas: 21-41

264.#.1.b: Instituto de Geofísica, UNAM

doi: https://doi.org/10.22201/igeof.2954436xe.1963.3.2.1686

handle: 008bea80379c8a2c

harvesting_date: 2023-06-20 17:00:00.0

856.#.0.q: application/pdf

file_creation_date: 2023-01-31 15:41:31.0

file_modification_date: 2023-04-25 20:13:04.0

file_creator: H. S. Ahluwalia

file_name: 7a0e9926fb363e3ba30fc11afa821a79fe9f804f6cf9ce0f7b3799404436cee6.pdf

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245.1.0.b: Variaciones en intensidad de la radiación cósmica y los estados electromagnéticos del espacio interplanetario

last_modified: 2023-06-20 17:00:00

license_url: https://creativecommons.org/licenses/by-nc-sa/4.0/legalcode.es

license_type: by-nc-sa

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