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New features in S2KRG v2.25 (http://SpaceWx.com website - S2KRG QUICK-LINK) are:

1) 2 new solar proxies:

a) The E162 proxy (reported in units of F10.7) is released with this version which enables a user to access the 162-day smoothed E10.7 for date ranges greater than 162 days. The MET v2.0 atmospheric density model uses the daily and 162-day (running boxcar) smoothed values.

b) The XE10 proxy (reported in units of F10.7) is released with this version and, for satellite operators, may provide slightly better modeling of atmospheric densities that affect satellite drag compared to F10.7 or E10.7. It is the integrated 1-40 nm energy flux whose energy is primarily absorbed by atomic oxygen above 200 km.

2) 185 new photoionization rates: Photoionization rates for 185 ions are calculated using cross sections interpolated over resonances for the ground states of atoms and all ions of the OP elements (Verner et al., 1996: H, He, Le, Be, B, C, N, O, F, Ne, Na, Mg, Al, Si, S, Ar, Ca, Fe). The cross sections are multiplied by photon flux to provide values. The photoionization rates are valid for the energy range from the ionization threshold to the first cross section jump due to inner shell photoionization.

3) The proxies in Earth-observed S2KRG v2.25 model are extended through 28-FEB-2005. This includes the updated composite Lyman-alpha released by T. Woods on December 1, 2004 containing values through November 28, 2004.

4) S2KRG v2.25 is only released for use on IDL 6.0 or higher and for the "observed" flux rather than "1-AU adjusted." An adjusted version will be released soon and, by request, an IDL 5.6 version will be released.

5) .The SOLAR2000 Professional Grade v2.25 is also available and provides forecasts of the same parameters as the Research Grade model for operational users. Please contact spacenvironment@spacenvironment.net for more information on S2KPG v2.2

12 Feb 05 - New predictions of solar flare qualities (http://SpaceWx.com website - FLARE QUICK-LINK) have a 1-minute resolution with a 2-minute cadence and a 6-minute latency. The X-ray flare evolution prediction is fully automated, uses the GOES 0.1-0.8 nm X-ray flux data, and provides a model of an expected flare profile based on the background level and the flare rise time. The past 72-hours of X-ray flux and prediction history are displayed along with text describing the dynamically-changing space weather-related impacts affecting communication, navigation, LEO, and GEO spacecraft systems.

 

 

 

 

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