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dc.contributor.authorBlanco Ávalos, Juan José es_ES
dc.contributor.authorGarcía Tejedor, Juan Ignacio es_ES
dc.contributor.authorGarcía Población, Óscar es_ES
dc.contributor.authorCatalán Picchottito, Edwin Joé es_ES
dc.contributor.authorMedina Doctor, José es_ES
dc.contributor.authorGómez Herrero, Raúl es_ES
dc.date.accessioned2017-09-05T08:58:11Z
dc.date.available2017-09-05T08:58:11Z
dc.date.issued2013-07-01
dc.identifier.bibliographicCitationProceedings of the 33rd International Cosmic Rays Conference The Astroparticle Physics Conference, 2013en
dc.identifier.isbn978-85-89064-29-3
dc.identifier.urihttp://hdl.handle.net/10017/30317
dc.description.abstractThe Castilla-La Mancha (CaLMa) neutron monitor is continuously operating since 26 October 2011. It is located at Guadalajara (40°38"N, 3°9"W) at 708 m above sea level and 55 km away from Madrid. It iscovering a gap in the Neutron Monitor Data Base (NMDB), thanks to its geographical location, its height above sea level and its vertical cutoff rigidity (6.95 GV). CaLMa is providing counts of galactic cosmic rays (GCRs) with a temporal resolution of 1 min, being the mean count rate 5 c/s/counter. This high cadence allows the monitoring of solar activity by mean the observed variation in count rate. Both in the sort term and in the long term activity, i.e., flare or coronal mass ejections and solar modulation, can therefore be studied with CaLMa"s measurements. During this last year, CaLMa has measured variations in the GCR count rate related to interplanetary coronal mass ejections, fast solar wind streams, shocks and stream interaction regions. In this work we analyze the solar wind condition associated to variations in CaLMa"s count rate and we compare them with other neutron monitors.en
dc.description.sponsorshipJunta de Comunidades de Castilla-La Manchaes_ES
dc.description.sponsorshipMinisterio de Ciencia y Tecnologíaes_ES
dc.format.mimetypeapplication/pdfen
dc.language.isoengen
dc.rightsAttribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.subjectNeutron monitoren
dc.subjectCosmic raysen
dc.subjectSolar energetic particlesen
dc.subjectSolar activityen
dc.titleFollowing solar activity with CaLMaen
dc.typeinfo:eu-repo/semantics/bookParten
dc.subject.ecienciaFísicaes_ES
dc.subject.ecienciaPhysicsen
dc.contributor.affiliationUniversidad de Alcalá. Departamento de Automáticaes_ES
dc.contributor.affiliationUniversidad de Alcalá. Departamento de Física y Matemáticases_ES
dc.date.updated2017-07-27T11:37:24Z
dc.type.versioninfo:eu-repo/semantics/publishedVersionen
dc.relation.projectIDinfo:eu-repo/grantAgreement/JCCM//PPII1001506529/ESes_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/MICIN//AYA2011-29727-C02-01/ES/SOLAR ORBITER ENERGETIC PARTICLE DETECTOR SYSTEM MANAGEMENTen
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.identifier.uxxiCO/0000013209
dc.identifier.publicationtitleProceedings of the 33rd International Cosmic Rays Conference The Astroparticle Physics Conferenceen


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