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Authordc.contributor.authorStorini, M. 
Authordc.contributor.authorKudela, K. es_CL
Authordc.contributor.authorCordaro Cárdenas, Enrique es_CL
Authordc.contributor.authorMassetti, S. es_CL
Admission datedc.date.accessioned2007-05-18T14:47:09Z
Available datedc.date.available2007-05-18T14:47:09Z
Publication datedc.date.issued2005
Cita de ítemdc.identifier.citationINFLUENCE OF THE SUN'S RADIATION AND PARTICLES ON THE EARTH'S ATMOSPHERE AND CLIMATE ADVANCES IN SPACE RESEARCHen
Identifierdc.identifier.issn0273-1177
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/124597
Abstractdc.description.abstractThe list of Ground-Level Enhancements (GLEs) occurring during the on-going solar cycle (no. 23) is used to show that they are absent during a time interval of the maximum phase in which a relative reduction in the sunspot area extent occurs. This period refers to October 2000 to March 2001 and it is associated with the concept of the Gnevyshev Gap, introduced 10 years ago by the Rome cosmic ray group. Also, effects of the Gnevyshev Gap in the solar cycle modulation of the atmospheric attenuation coefficient for Rome neutron monitor during the past solar cycle (no. 22) are illustrated. Moreover, it is suggested that GLE data files should be prepared by using the appropriate attenuation coefficient for each level of solar activity.en
Lenguagedc.language.isoenen
Publisherdc.publisherPERGAMON-ELSEVIER SCIENCE LTDen
Keywordsdc.subjectSOLAR PROTON EVENTSen
Títulodc.titleGround-level enhancements during solar cycle 23: results from SVIRCO, LOMNICKY STIT and LARC neutron monitorsen
Document typedc.typeArtículo de revista


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