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Statistical characterization of strong and mid solar flares and sun EUV rate monitoring with GNSS

Author
Monte, E.; Hernandez, M.; Garcia-Rigo, A.; Beniguel, Y.; Orús, R.; Prieto-Cerdeira, R.; Schlueter, S.
Type of activity
Journal article
Journal
Geophysical research abstracts
Date of publication
2015-03-16
Volume
17
First page
1
Last page
1
Repository
http://hdl.handle.net/2117/26834 Open in new window
URL
http://meetingorganizer.copernicus.org/EGU2015/EGU2015-12036.pdf Open in new window
Abstract
The global network of permanent Global Navigation Satellite Systems (GNSS) receivers has become an useful and affordable way of monitoring the Solar EUV flux rate, especially -for the time being- in the context of Major and Mid geoeffective intensity Solar Flares (M. Hernandez-Pajares et al., SpaceWeather, doi:10.1029/2012SW000826, 2012). In fact the maturity of this technique (GNSS Solar FLAre Indicator, GSFLAI) has allowed to incorporate it in operational real-time (RT) conditions, thanks to t...
Citation
Monte, E. [et al.]. Statistical characterization of strong and mid solar flares and sun EUV rate monitoring with GNSS. "Geophysical research abstracts", 16 Març 2015, vol. 17, p. 1.
Keywords
EUV rate monitoring, GNSS, Strong and Mid Solar Flares
Group of research
IDEAI-UPC - Intelligent Data Science and Artificial Intelligence Research Center
IonSAT - Ionospheric determination and navigation based on Satellite And Terrestrial systems
TALP - Centre for Language and Speech Technologies and Applications
VEU - Speech Processing Group

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