dor_id: 4133318

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/657/660

100.1.#.a: Berdichevsky, D.; Richardson, J. G.; Thomspson, B. J.; Reames, D. V.; Macdowall, R.; Plunkett, S. P.; Michels, D. J.; Kaiser, M. L.; Lepping, R. P.; Ogilvie, K. W.; Stone, R. G.

524.#.#.a: Berdichevsky, D., et al. (2000). Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact. Geofísica Internacional; Vol. 39 Núm. 1: Enero 1, 2000; 5-11. Recuperado de https://repositorio.unam.mx/contenidos/4133318

245.1.0.a: Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact

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

561.1.#.a: Instituto de Geofísica, UNAM

264.#.0.c: 2000

264.#.1.c: 2000-01-01

653.#.#.a: Viento solar; Tormentas geomagnéticas; actividad solar; Solar wind; geomagnetic storms; solar activity

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/657

001.#.#.#: 063.oai:revistagi.geofisica.unam.mx:article/657

041.#.7.h: spa

520.3.#.a: We present examples of solar ejecta, including possible interplanetary magnetic clouds, which generated fast forward interplanetary shocks as they moved rapidly through the interplanetary medium. These events occurred before and during the ISTP era. The example from 1982, close to solar maximum, was observed by the SOLWIND, ISEE, HELIOS, and IMP spacecraft which provide wide coverage of the Sun and inner heliosphere. The second event occurred on May 1998. A detailed description of its solar origin is provided by observations from instruments on the SOHO spacecraft, while observations of the shock-generated radio emissions and energetic particles and near-earth solar wind magnetic fields and plasmas are provided by the Wind spacecraft. We revisit potential tools for space weather forecasting, namely: the power of monitoring the Sun with sensors located within a wide range of heliospheric longitudes and distances, the high resolution in time and light-intensity of the extreme ultraviolet imager and solar coronograph, the remote sensing of drifting radio emissions and the local observation of MeV energetic ions.doi: https://doi.org/10.22201/igeof.00167169p.2000.39.1.289

773.1.#.t: Geofísica Internacional; Vol. 39 Núm. 1: Enero 1, 2000; 5-11

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: 5-11

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

doi: https://doi.org/10.22201/igeof.00167169p.2000.39.1.289

handle: 00aaee9a95643d96

harvesting_date: 2023-06-20 16:00:00.0

856.#.0.q: application/pdf

file_creation_date: 2000-07-07 10:33:13.0

file_modification_date: 2022-07-13 16:41:02.0

file_creator: D. Berdichevsky

file_name: 05acc82050abd2ccc6da8a52490e4bfbab014020441ce6b7a8d0816845b903d5.pdf

file_pages_number: 7

file_format_version: application/pdf; version=1.6

file_size: 160159

245.1.0.b: Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact

last_modified: 2023-06-20 16:00:00

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

license_type: by-nc-sa

No entro en nada

No entro en nada 2

Artículo

Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact

Berdichevsky, D.; Richardson, J. G.; Thomspson, B. J.; Reames, D. V.; Macdowall, R.; Plunkett, S. P.; Michels, D. J.; Kaiser, M. L.; Lepping, R. P.; Ogilvie, K. W.; Stone, R. G.

Instituto de Geofísica, UNAM, publicado en Geofísica Internacional, y cosechado de Revistas UNAM

Licencia de uso

Procedencia del contenido

Entidad o dependencia
Instituto de Geofísica, UNAM
Revista
Repositorio
Contacto
Revistas UNAM. Dirección General de Publicaciones y Fomento Editorial, UNAM en revistas@unam.mx

Cita

Berdichevsky, D., et al. (2000). Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact. Geofísica Internacional; Vol. 39 Núm. 1: Enero 1, 2000; 5-11. Recuperado de https://repositorio.unam.mx/contenidos/4133318

Descripción del recurso

Autor(es)
Berdichevsky, D.; Richardson, J. G.; Thomspson, B. J.; Reames, D. V.; Macdowall, R.; Plunkett, S. P.; Michels, D. J.; Kaiser, M. L.; Lepping, R. P.; Ogilvie, K. W.; Stone, R. G.
Tipo
Artículo de Investigación
Área del conocimiento
Físico Matemáticas y Ciencias de la Tierra
Título
Examples of fast solar wind transients, their sources and the forecast of possible geomagnetic impact
Fecha
2000-01-01
Resumen
We present examples of solar ejecta, including possible interplanetary magnetic clouds, which generated fast forward interplanetary shocks as they moved rapidly through the interplanetary medium. These events occurred before and during the ISTP era. The example from 1982, close to solar maximum, was observed by the SOLWIND, ISEE, HELIOS, and IMP spacecraft which provide wide coverage of the Sun and inner heliosphere. The second event occurred on May 1998. A detailed description of its solar origin is provided by observations from instruments on the SOHO spacecraft, while observations of the shock-generated radio emissions and energetic particles and near-earth solar wind magnetic fields and plasmas are provided by the Wind spacecraft. We revisit potential tools for space weather forecasting, namely: the power of monitoring the Sun with sensors located within a wide range of heliospheric longitudes and distances, the high resolution in time and light-intensity of the extreme ultraviolet imager and solar coronograph, the remote sensing of drifting radio emissions and the local observation of MeV energetic ions.doi: https://doi.org/10.22201/igeof.00167169p.2000.39.1.289
Tema
Viento solar; Tormentas geomagnéticas; actividad solar; Solar wind; geomagnetic storms; solar activity
Idioma
spa
ISSN
ISSN-L: 2954-436X; ISSN impreso: 0016-7169

Enlaces