NOTE: For queries from July 2016 and after, please use the newer Solar Flares Database on the NASA Heliophysics Portal (https://data.nas.nasa.gov/helio/) .
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TIME INTERVAL (Jan 01, 2002 - present date):
SELECT MAX TEMPEARATURE RANGE:
SELECT MAX EMISSION MEASURE RANGE:
SELECT FLARE GOES CLASS RANGE:
SELECT GOES FLARE DURATION:
SELECT GOES FLARE T-EM DELAY:
SELECT ENERGY RANGE:
SELECT DURATION RANGE:
SELECT PEAK RANGE:
SELECT OBSERVATIONAL QUALITY FLAGS:
SELECT AIA CHANNEL:
SELECT PEAK FLUX RANGE:
SELECT PEAK COUNTS NUMBER:
SELECT TOTAL COUNTS NUMBER:
SELECT MINIMUM NUMBER OF SOT FG IMAGES:
SELECT MINIMUM NUMBER OF SOT SP IMAGES:
SELECT MINIMUM NUMBER OF XRT IMAGES:
SELECT MINIMUM NUMBER OF EIS IMAGES:
SELECT TIME PRIOR THE FILAMENT ERUPTION:
SELECT EXTENSION OF THE FILAMENT COORDINATE BOX:
SELECT ARBITRARY INTEREST RATING:
SELECT FILAMENT TYPE:
SELECT FILAMENT ERUPTION TYPE:
SELECT FILAMENT SYMMETRY:
SELECT FILAMENT DIRECTION:
EXPAND OVSA EVENT TIME RANGE:
EXPAND EOVSA ONSET TIME RANGE (10 minutes by default):
SELECT THE SEARCH TIME INTERVAL RELATIVE TO THE FLARE START AND END TIMES (in minutes):
SELECT LIFTOFF TIME:
SELECT PRINCIPAL ANGLE:
SELECT ANGULAR WIDTH:
SELECT MEDIAN VELOCITY:
SELECT MIN VELOCITY:
SELECT MAX VELOCITY:
SELECT HALO TYPE:
The CME association is currently based on the CME onset time, and the flare Start time and End time.
EXPAND IRIS FOV BOX FOR:
SELECT SJI CHANNELS NEEDED TO BE OBSERVED:
SJI NUMBER OF IMAGES:
SELECT DESIRED RASTER MODES:
SELECT NUMBER OF SLIT POSITIONS IN ONE RASTER:
SELECT RASTER FOV (DISTANCE BETWEEN FIRST AND LAST SLIT POSITIONS):
SELECT RASTER CADENCE (TIME NEEDED TO COVER ALL SLIT POSITIONS):
SELECT RASTER LINES:
IRIS filters cannot be applied for the events with missing position and AR information; These events are ignored if the filter is switched on
SELECT SPE FLUX: