Near-Earth heliospheric magnetic field intensity since 1750: 2. Cosmogenic radionuclide reconstructions

This is Part 2 of a study of the near-Earth heliospheric magnetic field strength, B, since 1750. Part 1 produced composite estimates of B from geomagnetic and sunspot data over the period 1750-2013. Sunspot-based reconstructions can be extended back to 1610, but the paleocosmic ray (PCR) record is t...

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Detalhes bibliográficos
Autor principal: Owens, M. J. (author)
Outros Autores: Cliver, E. (author), McCracken, K. G. (author), Beer, J. (author), Barnard, L. (author), Lockwood, M. (author), Rouillard, A. (author), Passos, Dário (author), Riley, P. (author), Usoskin, I. (author), Wang, Y-M. (author)
Formato: article
Idioma:eng
Publicado em: 2017
Texto completo:http://hdl.handle.net/10400.1/9400
País:Portugal
Oai:oai:sapientia.ualg.pt:10400.1/9400

Texto Completo

http://hdl.handle.net/10400.1/9400

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