Vaata kolmapäev, 30 august 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 Aug 30 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 243 Välja antud 2200Z kuni 30 AUG 2000IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 29-2100Z kuni 30-2100Z SOLAR ACTIVITY WAS LOW. TODAY'S MOST SIGNIFICANT X-RAY
EVENT WAS A LONG DURATION C4 EVENT FROM 29/2235Z TO 30/0028Z. THERE
WAS AN ASSOCIATED CME DIRECTED AWAY FROM THE SOUTHEAST LIMB WHICH
WAS OBSERVED TO ENTER THE C2 FIELD OF VIEW AT 29/2354Z AND THE C3
FIELD OF VIEW AT 30/0042Z. DISK ACTIVITY WAS APPARENT IN EIT IMAGES
BETWEEN REGIONS 9148 (S19E18) AND 9143 (S18W06). ADDITIONAL
LOW-LEVEL C-CLASS EVENTS WERE OBSERVED THROUGHOUT THE DAY. REGION
9149 (N11E44) IS CURRENTLY THE LARGEST GROUP ON THE DISK WITH AN
AREA OF 330 MILLIONTHS. THE GROUP APPEARS TO BE STABLE AT THIS TIME.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE
MOSTLY LOW, BUT THERE IS A SLIGHT-TO-FAIR CHANCE FOR AN ISOLATED
M-CLASS EVENT DURING THE NEXT THREE DAYS.
IIA. GEOPHYSICAL ACTIVITY SUMMARY 29/2100Z TO 30/2100Z:
THE GEOMAGNETIC FIELD RANGED FROM QUIET TO ACTIVE LEVELS DURING THE
PAST 24 HOURS. REAL-TIME SOLAR WIND OBSERVATIONS FROM ACE INDICATE
THE CONTINUATION OF A HIGH-SPEED, POSITIVE-POLARITY, CORONAL HOLE
STREAM. THE FLOW SEEMS TO BE WEAKENING SLOWLY AS EVIDENCED BY A
GRADUAL DECLINE IN THE VELOCITY. THE GREATER THAN 2 MEV ELECTRON
FLUX AT GEOSYNCHRONOUS ORBIT WAS HIGH (GREATER THAN 1000 PFU) DURING
THE PAST 24 HOURS.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS
EXPECTED TO BE PREDOMINANTLY UNSETTLED DURING THE NEXT THREE DAYS.
III. Sündmuste tõenäosus 31 AUGkuni 02 SEP
| Klass M | 30% | 30% | 30% |
| Klass X | 05% | 05% | 05% |
| Prooton | 05% | 05% | 05% |
| PCAF | GREEN | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 30 AUG 165 Prognoositud 31 AUG-02 SEP 168/168/165 90 päeva keskmine 30 AUG 182
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 29 AUG 021/031 ESTIMATED AFR/AP 30 AUG 018/018 PREDICTED AFR/AP 31 AUG-02 SEP 012/012-012/010-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 31 AUG kuni 02 SEP
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 30% | 30% | 25% |
| Väike torm | 10% | 10% | 05% |
| Suur-tõsine torm | 05% | 05% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 30% | 30% | 25% |
| Väike torm | 15% | 15% | 10% |
| Suur-tõsine torm | 10% | 10% | 05% |
<< 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
Filaments and prominences 67Unspecified geomagnetic activity 959Latest SC25 Predictions 105ionosphere D detection 11AR3654 44
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 | 01/05/2024 | M1.9 |
| Viimane geomagnetiline torm | 26/04/2024 | Kp5+ (G1) |
| Plekivabasid päevi | |
|---|---|
| Viimane päikese plekivaba päev | 08/06/2022 |
| Kuu keskmine päikeseplekkide arv | |
|---|---|
| märts 2024 | 104.9 -19.8 |
| Viimased 30 päeva | 148.1 +49.1 |