Other
Scientific paper
Jun 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002stin...0259662f&link_type=abstract
Technical Report, Rept-II-4010
Other
Solar Flux, Irradiance, Extreme Ultraviolet Radiation, Radiation Measurement, Time Series Analysis, Solar Protons, Soho Mission, Data Correlation, Solar Radiation
Scientific paper
The Extreme Ultraviolet (EUV) irradiance central and first order channel time series (COC and FOC) from the Solar EUV Monitor aboard the Solar and Heliospheric observatory (SOHO) issued in early 2002 covering the time period 1/1/96-31/1201 were analyzed in terms of other solar measurements and indices. A significant solar proton effect in the first order irradiance was found and characterized. When this effect is removed, the two irradiance time series are almost perfectly correlated. Earlier studies have shown good correlation between the FOC and the Hall core-to-wing ratio and likewise, it was the strongest component of the COC. Analysis of the FOC showed dependence on the F10.7 radio flux. Analysis of the CDC signals showed additional dependences on F10.7 and the GOES x-ray fluxes. The SEM FOC was also well correlated with thein 30.4 nm channel of the SOHO EUV Imaging Telescope (EIT). The irradiance derived from all four EIT channels (30.4 nm, 17.1 nm, 28.4 nm, and 19.5 nm) showed better correlation with MgII than F10.7.
No associations
LandOfFree
Studies of Solar EUV Irradiance from SOHO does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Studies of Solar EUV Irradiance from SOHO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Studies of Solar EUV Irradiance from SOHO will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1201561