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Solar activity and ionospheric response as seen from combined SolACES and SDO-EVE solar EUV spectra

Ionospheric response to solar EUV variability during late 2012 through mid 2013 is shown by the EUV-TEC proxy based on combined SolACES and SDO/EVE solar spectra. The results are compared with global TEC analyses. We found that EUV-TEC describes TEC variability better than the conventional F107 index, especially during periods of strong solar flare activity.

Identiferoai:union.ndltd.org:DRESDEN/oai:qucosa:de:qucosa:16435
Date10 October 2017
CreatorsJacobi, Christoph, Nikutowski, B., Hein, J., Unglaub, C., Erhardt, Ch., Brunner, R., Schmidtke, G.
ContributorsUniversität Leipzig, Universität Leipzig
Source SetsHochschulschriftenserver (HSSS) der SLUB Dresden
LanguageEnglish, German
Detected LanguageEnglish
Typeinfo:eu-repo/semantics/publishedVersion, doc-type:article, info:eu-repo/semantics/article, doc-type:Text
Rightsinfo:eu-repo/semantics/openAccess
Relationurn:nbn:de:bsz:15-qucosa-212081, qucosa:15003

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