Vaata esmaspäev, 3 aprill 2000 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 2000 Apr 03 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 094 Välja antud 2200Z kuni 03 APR 2000IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 02-2100Z kuni 03-2100Z SOLAR ACTIVITY REMAINED LOW. SEVERAL SMALL C-CLASS
SUBFLARES OCCURRED. MOST DISK REGIONS EXHIBITED DECAY WITH THE
EXCEPTION OF 8933 (N18W57) THAT GREW AT A MODERATE PACE. PLAGE WAS
BRIGHT IN THIS REGION FOR MOST OF THE PERIOD. OLD REGION 8906 WHICH
PRODUCED 8 M-CLASS EVENTS LAST ROTATION BEGAN TO APPEAR AT THE
SOUTHEAST LIMB. NO SPOTS WERE VISIBLE BUT A LARGE DIFFUSE PLAGE
FIELD BECAME EVIDENT.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY SHOULD BE LOW TO
MODERATE. REGION 8933 SHOULD BEGIN TO PRODUCE FREQUENT SMALL C-CLASS
EVENTS. SHOULD GROWTH CONTINUE HERE, A FILAMENT JUST TO THE EAST OF
THIS REGION MAY ERUPT WITH A LONG DURATION C-CLASS EVENT AND MASS
EJECTION. OTHER REGIONS ON THE DISK ARE CAPABLE OF ONLY ISOLATED
M-CLASS EVENTS. IT IS DIFFICULT TO ASSESS THE FLARE POTENTIAL OF
RETURNING REGION 8906 AT THIS TIME. THE LACK OF DISCERNIBLE FLARES
FROM THIS AREA ARGUES FOR A REDUCED POTENTIAL FROM LAST ROTATION.
IIA. Summaarne geofüüsikaline aktiivsus 02-2100Z kuni 03-2100Z
THE GEOMAGNETIC FIELD WAS QUIET TO UNSETTLED. SOLAR WIND VELOCITIES
DECREASED TO LOW LEVELS DURING THE PERIOD. ENERGETIC ELECTRON FLUXES
AT GEOSYNCHRONOUS BECAME ELEVATED BUT DID NOT REACH HIGH LEVELS.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD SHOULD
REMAIN PREDOMINANTLY QUIET TO UNSETTLED FOR THE NEXT THREE DAYS.
ISOLATED ACTIVE PERIODS MAY OCCUR.
III. Sündmuste tõenäosus 04 APRkuni 06 APR
| Klass M | 50% | 50% | 50% |
| Klass X | 05% | 05% | 05% |
| Prooton | 05% | 05% | 05% |
| PCAF | GREEN | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 03 APR 215 Prognoositud 04 APR-06 APR 218/215/210 90 päeva keskmine 03 APR 184
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 02 APR 014/016 ESTIMATED AFR/AP 03 APR 010/012 PREDICTED AFR/AP 04 APR-06 APR 008/012-010/015-008/012
VI. Geomagnetilised aktiivsuse tõenäosused 04 APR kuni 06 APR
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 25% | 10% |
| Väike torm | 05% | 10% | 05% |
| Suur-tõsine torm | 01% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 25% | 30% | 15% |
| Väike torm | 10% | 15% | 05% |
| Suur-tõsine torm | 01% | 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
What are these long and thin eruptions? 1AR 3637, 3638, 3643 89Unproven theories 341Space Weather Memes 338Filaments and prominences 55
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 | 28/03/2024 | X1.1 |
| Viimane M-loide | 25/04/2024 | M1.0 |
| Viimane geomagnetiline torm | 19/04/2024 | Kp7 (G3) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| märts 2024 | 104.9 -19.8 |
| Viimased 30 päeva | 133.9 +26.6 |