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

Description

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.

Links & Downloads

1. urn:nbn:de:bsz:15-qucosa2-164352
2. https://ul.qucosa.de/id/qucosa%3A16435
3. https://ul.qucosa.de/api/qucosa%3A16435/attachment/ATT-0/

Tags

EUV-Variabilität, Ionosphäre

info:eu-repo/classification/ddc/551

ddc:551

Additional Fields

Identifer	oai:union.ndltd.org:DRESDEN/oai:qucosa:de:qucosa:16435
Date	10 October 2017
Creators	Jacobi, Christoph, Nikutowski, B., Hein, J., Unglaub, C., Erhardt, Ch., Brunner, R., Schmidtke, G.
Contributors	Universität Leipzig, Universität Leipzig
Source Sets	Hochschulschriftenserver (HSSS) der SLUB Dresden
Language	English, German
Detected Language	English
Type	info:eu-repo/semantics/publishedVersion, doc-type:article, info:eu-repo/semantics/article, doc-type:Text
Rights	info:eu-repo/semantics/openAccess
Relation	urn:nbn:de:bsz:15-qucosa-212081, qucosa:15003