Introduction to NICT’s evaluation of the space weather forecasts provided by Japan, US, Belgium, Australia and China. Mamoru Ishii, Shin’ichi Watari and.

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Presentation transcript:

Introduction to NICT’s evaluation of the space weather forecasts provided by Japan, US, Belgium, Australia and China. Mamoru Ishii, Shin’ichi Watari and Tsutomu Nagatsuma National Institute of Information and Communications Technology, Japan

UGEOA code Legend ISES/regional warning center has been using URSIgram Codes which were originally developed to facilitate the rapid exchange of information by telex. UGEOA code is one of URSIgram codes and means GEOALERT. NICT provide the hit rate of SW-forecast using UGEOA code from each RWC. GEOALERT TOK059 UGEOA IIIII YMMDD HHmm GSMII 1FIID 2FIID 3FIID PLAIN BT Key code UGEOA Flare forecast Last data line Text line Station indicator Groundbased solar data used for forecast Groundbased solar data used for forecast Year, Month and Day Site name and DOY Universal Time Proton forecast Magnetic forecast Break of text

Level of flare and gemagnetic forecast on the UGEOA code Flare forecast 0 = Quiet (<50% probability of C- class flares) 1 = Eruptive (C-class flares expected, probability >=50%) 2 = Active (M-class flares expected, probability >=50%) 3 = Major flares expected (X-class flares expected, probability >=50%) 4 = Proton flares expected (proton flares expected, probability >=50%) 8 = Warning condition (activity levels expected to increase, but no numeric forecast given) / = No forecast Geomagnetic forecast 0 = Quiet 1 = Active conditions expected (A>=20 or K=4) 2 = Minor storm expected (A>=30 or K=5) 3 = Major magstorm expected (A>=50 or K>=6) 4 = Severe magstorm expected (A>=100 or K>=7) 8 = Warning condition (activity levels expected to increase, but no numeric forecast given) / = No forecast

Space weather forecast by five RWC Tokyo Beijing Brussels Sydney Boulder

Results of evaluation in Solar flare forecast on March, 2015 Hit rate Threat Score Overestimate Underestimate

Hit Rate and Threat Score Forecast Major FlaresActiveEruptiveQuiet observed Major FlaresABCD ActiveEFGH EruptiveIJKL QuietMNOP T (Total) = A + B + … + P Overestimate Underestimate Hit Hit rate = (A+F+K+P)/T Threat Score = (A+F+K+P)/(T-P) Quiet condition is dominant especially in solar quiet period. In the case the subset of “P” tend to be large and the value of hit rate does not representative the actual meaning.

Result of evaluation in the geomagnetic disturbance on March 2015 Overestimate Underestimate

Comments on NICT forecasts in November, 2014 We check why our forecast failed every month. …When Active Region 2205 was located on the east limb of the solar disk (November 2nd to 3rd) The solar activity was mostly moderate when Active Region 2205 was located on the far side of the solar disk; however, a C9.4 flare occurred on the 2nd (UT) when the region was located on the east limb of the solar disk. (The magnetic field structure was unclear because the region was located on the east limb of the solar disk.) On the 3rd, a slightly high level of solar activity was forecast because further occurrence of C-class flares was expected on the basis of past records. However, M2.2 and M6.5 flares occurred in this region. Solar activity was not accurately forecast.

Hit rate of Flare forecast 9

Threat score of Flare forecast

Hit rate of Magnetic activities

Threat score of magnetic activities

Forecast evaluation on Web site