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Set de datos (Dataset).

ORCA Cruise, RV Sarmiento de Gamboa

Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027
Digital.CSIC. Repositorio Institucional del CSIC
  • Blanco, Juan José
  • CSIC - Unidad de Tecnología Marina (UTM)
ORCA Cruise (29SG20181116) carried out on the Research Vessel Sarmiento de Gamboa in 2018, Cosmic rays are high energy protons and atomic nuclei arriving to the Earth coming from the outer universe. Their study is very interesting because of the information they provide about their origin, the solar activity and the magnetosphere, among others. ORCA (Observatorio de Rayos Cosmicos Antartico) is a cosmic ray observatory aimed to study them with unprecedented accuracy in the Antarctic area. ORCA is composed by a neutron monitor (NEMO), a muon telescope (MITO) and a detector of the Trasgo familiy (TRISTAN). All the detectors with gather cosmic ray data on board of the Sarmiento de Gamboa oceanographic vessel along the journey between Spain and South America, before being installed in the Juan Carlos I Spanish Antarctic Base. Some of the main goals are to study the solar activity, the Earth magnetic field and the influence of the atmosphere in the cosmic ray data measured with ground detectors
 
DOI: http://hdl.handle.net/10261/236027
Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027

HANDLE: http://hdl.handle.net/10261/236027
Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027
 
Ver en: http://hdl.handle.net/10261/236027
Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027

Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027
Set de datos (Dataset). 2018

ORCA CRUISE, RV SARMIENTO DE GAMBOA

Digital.CSIC. Repositorio Institucional del CSIC
  • Blanco, Juan José
  • CSIC - Unidad de Tecnología Marina (UTM)
ORCA Cruise (29SG20181116) carried out on the Research Vessel Sarmiento de Gamboa in 2018, Cosmic rays are high energy protons and atomic nuclei arriving to the Earth coming from the outer universe. Their study is very interesting because of the information they provide about their origin, the solar activity and the magnetosphere, among others. ORCA (Observatorio de Rayos Cosmicos Antartico) is a cosmic ray observatory aimed to study them with unprecedented accuracy in the Antarctic area. ORCA is composed by a neutron monitor (NEMO), a muon telescope (MITO) and a detector of the Trasgo familiy (TRISTAN). All the detectors with gather cosmic ray data on board of the Sarmiento de Gamboa oceanographic vessel along the journey between Spain and South America, before being installed in the Juan Carlos I Spanish Antarctic Base. Some of the main goals are to study the solar activity, the Earth magnetic field and the influence of the atmosphere in the cosmic ray data measured with ground detectors




Digital.CSIC. Repositorio Institucional del CSIC
oai:digital.csic.es:10261/236027
Set de datos (Dataset). 2018

ORCA CRUISE, RV SARMIENTO DE GAMBOA

Digital.CSIC. Repositorio Institucional del CSIC
  • Blanco, Juan José
  • CSIC - Unidad de Tecnología Marina (UTM)
ORCA Cruise (29SG20181116) carried out on the Research Vessel Sarmiento de Gamboa in 2018, Cosmic rays are high energy protons and atomic nuclei arriving to the Earth coming from the outer universe. Their study is very interesting because of the information they provide about their origin, the solar activity and the magnetosphere, among others. ORCA (Observatorio de Rayos Cosmicos Antartico) is a cosmic ray observatory aimed to study them with unprecedented accuracy in the Antarctic area. ORCA is composed by a neutron monitor (NEMO), a muon telescope (MITO) and a detector of the Trasgo familiy (TRISTAN). All the detectors with gather cosmic ray data on board of the Sarmiento de Gamboa oceanographic vessel along the journey between Spain and South America, before being installed in the Juan Carlos I Spanish Antarctic Base. Some of the main goals are to study the solar activity, the Earth magnetic field and the influence of the atmosphere in the cosmic ray data measured with ground detectors




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