Vaata kolmapäev, 10 september 1997 arhiivi
Päikese aktiivsuse aruanne
Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Päikese ja geofüüsikalise aktiivsuse aruanne 1997 Sep 10 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 253 Välja antud 2200Z kuni 10 SEP 1997IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 09-2100Z kuni 10-2100Z SOLAR ACTIVITY WAS LOW. A SINGLE C1 FLARE WAS OBSERVED
DURING THE PAST 24 HOURS, MOSTLY LIKELY ORIGINATING FROM REGION 8084
(N22W01). REGION 8084, A STABLE 22-SPOT 'DSI' BETA GROUP, ALSO
GENERATED FOUR SUBFLARES DURING THE PERIOD. REGION 8083 (S28W35), A
19-SPOT 'DKO' BETA GROUP, PRODUCED A COUPLE OF SUBFLARES WHILE
GROWING IN SIZE BY 30% TO 710 MILLIONTHS. REGION 8085 (S26E27), THE
MOST COMPLEX AND POTENTIALLY SIGNIFICANT REGION ON THE VISIBLE DISK
AS A 24-SPOT 'FKI' BETA-GAMMA GROUP, HAS STOPPED GROWING AT 610
MILLIONTHS AND IS CURRENTLY QUIET.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE LOW
TO MODERATE. THE PROBABILITY OF C-CLASS ACTIVITY FROM ANY OF REGIONS
8083, 8084, AND 8085 REMAINS HIGH. IN ADDITION, REGION 8085 HAS THE
POTENTIAL TO GENERATE LOW TO MID-LEVEL M-CLASS ACTIVITY.
IIA. Summaarne geofüüsikaline aktiivsus 09-2100Z kuni 10-2100Z
THE GEOMAGNETIC FIELD HAS BEEN MOSTLY UNSETTLED AT ALL LATITUDES FOR
THE PAST 24 HOURS. THE GREATER THAN 2 MEV ELECTRON FLUX ALTERNATED
BETWEEN NORMAL AND HIGH.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE MOSTLY UNSETTLED FOR THE NEXT 2 DAYS, WITH THE
POTENTIAL FOR ACTIVE CONDITIONS AND ISOLATED PERIODS OF MINOR
STORMING ON DAY 3 IN RESPONSE TO YESTERDAY'S HALO MASS EJECTION THAT
ACCOMPANIED THE M1 FLARE FROM REGION 8083.
III. Sündmuste tõenäosus 11 SEPkuni 13 SEP
| Klass M | 40% | 40% | 40% |
| Klass X | 05% | 05% | 05% |
| Prooton | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 10 SEP 115 Prognoositud 11 SEP-13 SEP 115/115/115 90 päeva keskmine 10 SEP 077
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 09 SEP 019/019 ESTIMATED AFR/AP 10 SEP 017/015 PREDICTED AFR/AP 11 SEP-13 SEP 015/012-015/008-015/008
VI. Geomagnetilised aktiivsuse tõenäosused 11 SEP kuni 13 SEP
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 20% | 30% |
| Väike torm | 10% | 10% | 15% |
| Suur-tõsine torm | 01% | 01% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 20% | 30% |
| Väike torm | 10% | 15% | 20% |
| Suur-tõsine torm | 01% | 01% | 05% |
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