Vaata neljapäev, 28 oktoober 1999 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 1999 Oct 28 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 301 Välja antud 2200Z kuni 28 OCT 1999IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 27-2100Z kuni 28-2100Z SOLAR ACTIVITY WAS LOW. THE DEPARTURE OF REGION 8737
NEAR SW13 AND THE SIMPLIFICATION OF REGION 8739 (S11W37) CAUSED
FLARE COUNTS TO FALL OVER THE PAST 24 HOURS. VERY LITTLE ACTIVITY
OCCURRED, THE MOST NOTABLE EVENT BEING A C1/SF FROM 8739 AT 0457Z.
NEWLY ASSIGNED REGION 8747 (N10E59) HAS BRIGHT PLAGE AND DID PRODUCE
A FEW SUBFLARES DURING THE INTERVAL.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE LOW
TO MODERATE. ALTHOUGH SEEMINGLY MORE BENIGN, REGION 8739 MAY STILL
GENERATE AN ISOLATED M-CLASS EVENT.
IIA. Summaarne geofüüsikaline aktiivsus 27-2100Z kuni 28-2100Z
THE GEOMAGNETIC FIELD VARIED FROM QUIET TO MINOR STORM LEVELS DURING
THE DAY. ABOUT 1200Z, SOLAR WIND PLASMA AND MAGNETIC FIELD
EXPERIENCED A CHANGE AT THE ACE SPACECRAFT, RESULTING IN THE
DISTURBED LEVELS SEEN DURING THE LATTER HALF OF THE PERIOD. THESE
DATA SUGGEST A GLANCING BLOW BY A TRANSIENT AS THE CAUSE OF THE
ELEVATED ACTIVITY. THE GREATER THAN 2 MEV ELECTRON FLUX AT
GEOSYNCHRONOUS ORBIT REACHED HIGH LEVELS FROM 1330-1630Z,
APPROXIMATELY.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE AT UNSETTLED TO ACTIVE LEVELS FOR THE NEXT FEW DAYS.
EPISODIC MINOR STORM CONDITIONS ARE DISTINCTLY POSSIBLE DURING LOCAL
NIGHTTIME HOURS. A HIGH SPEED STREAM IS EXPECTED TO PROLONG THE
UNSETTLED CONDITIONS THROUGH OCTOBER 31.
III. Sündmuste tõenäosus 29 OCTkuni 31 OCT
| Klass M | 30% | 30% | 30% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 28 OCT 184 Prognoositud 29 OCT-31 OCT 175/165/160 90 päeva keskmine 28 OCT 157
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 27 OCT 010/017 ESTIMATED AFR/AP 28 OCT 015/015 PREDICTED AFR/AP 29 OCT-31 OCT 020/020-015/020-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 29 OCT kuni 31 OCT
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 40% | 30% | 30% |
| Väike torm | 25% | 20% | 20% |
| Suur-tõsine torm | 05% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 50% | 40% | 40% |
| Väike torm | 30% | 25% | 25% |
| Suur-tõsine torm | 05% | 05% | 05% |
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