Vaata kolmapäev, 5 märts 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 Mar 05 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 064 Välja antud 2200Z kuni 05 MAR 1997IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 04-2100Z kuni 05-2100Z SOLAR ACTIVITY REMAINED VERY LOW. HOWEVER, SEVERAL
SMALL B-CLASS X-RAY BURSTS OCCURRED. IT IS LIKELY THESE BURSTS WERE
FROM A REGION ABOUT TO ROTATE ONTO THE DISK NEAR N04. ACTIVE SURGING
AND BRIGHT KNOTS OF H-ALPHA EMISSION WERE OBSERVED OVER THIS AREA.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY SHOULD REMAIN AT VERY
LOW LEVELS. THERE IS A POSSIBILITY OF C-CLASS EVENTS FROM THE REGION
BEYOND THE NORTHEAST LIMB. A BETTER ASSESSMENT OF FLARE POTENTIAL
CAN BE MADE ONCE THE SUNSPOT GROUP APPEARS.
IIA. Summaarne geofüüsikaline aktiivsus 04-2100Z kuni 05-2100Z
THE GEOMAGNETIC FIELD WAS QUIET UNTIL NEAR 05/1630Z. AFTER THAT TIME,
GENERALLY UNSETTLED TO ACTIVE CONDITIONS WERE OBSERVED WITH ISOLATED
MINOR STORMING OBSERVED AT A FEW HIGH LATITUDE SITES. RECENT SOLAR
WIND DATA SHOW INCREASING DENSITY AND VELOCITY. THE SOURCE OF THIS
DISTURBANCE IS UNKNOWN. ENERGETIC ELECTRON FLUXES WERE HIGH FOR MOST
OF THE PERIOD BUT DROPPED TO MODERATE LEVELS AFTER 05/1930Z.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS
FORECAST TO BE PREDOMINANTLY QUIET TO UNSETTLED FOR THE NEXT THREE
DAYS. ISOLATED ACTIVE CONDITIONS ARE POSSIBLE DURING 06 MAR.
III. Sündmuste tõenäosus 06 MARkuni 08 MAR
| Klass M | 01% | 01% | 01% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | GREEN | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 05 MAR 075 Prognoositud 06 MAR-08 MAR 077/079/080 90 päeva keskmine 05 MAR 075
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 04 MAR 004/004 ESTIMATED AFR/AP 05 MAR 007/008 PREDICTED AFR/AP 06 MAR-08 MAR 010/010-005/005-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 06 MAR kuni 08 MAR
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 10% | 15% |
| Väike torm | 15% | 05% | 05% |
| Suur-tõsine torm | 05% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 10% | 20% |
| Väike torm | 10% | 10% | 05% |
| Suur-tõsine torm | 05% | 01% | 01% |
<< Mine igapäevase ülevaate lehele
Viimane uudis
esmaspäev, 22 aprill 2024
Lot's of sunspots! Big chance for major flare activity?
laupäev, 23 märts 2024
X1.1 solar flare with earth-directed CME
kolmapäev, 20 märts 2024
Sunspot region 3615, G1 watch
Viimane foorumi postitus
Veel teemasidToeta SpaceWeatherLive.com-i!
Paljud inimesed külastavad SpaceWeatherLive lehte selleks, et jälgida, mis toimub Päikesel või, kas on oodata virmalisi. Suurema liiklusega on serveri koormus ning maksumus kõrgem. Kui sulle meeldib see, mida me sinu heaks teeme, siis saad sa sellele ka ise natukene kaasa aidata, annetades selle lehe käigus hoidmise ja arendamise heaks. Ette tänades SpeaceWeatherLive meeskond!
Fakte kosmose ilmast
| Viimane X-loide | 03/05/2024 | X1.6 |
| Viimane M-loide | 03/05/2024 | M4.4 |
| Viimane geomagnetiline torm | 02/05/2024 | Kp7- (G3) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| aprill 2024 | 136.5 +31.6 |
| Viimased 30 päeva | 149.4 +51.8 |