Vaata teisipäev, 1 aprill 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 Apr 01 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga

Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne

SDF number 091 Välja antud 2200Z kuni 01 APR 1997

IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 31-2100Z kuni 01-2100Z

SOLAR ACTIVITY WAS MODERATE. REGION 8026 (S25E07), A 13 SPOT 'CAO' GROUP, GENERATED A SINGLE M1/1B FLARE AT 01/1348, WHICH WAS PRECEEDED BY THREE C-CLASS EVENTS. THE REGION HAD BEEN SURGING PRIOR TO, BUT HAD STOPPED BEFORE THE ONSET OF THE M1 EVENT. AN ASSOCIATED HIGH SPEED DARK SURGE ACCOMPANIED THE M1 FLARE. ALL FOUR FLARES OCCURRED NEAR THE SMALL OPPOSITE POLARITY FIELD EAST OF THE SOUTHERNMOST PENUMBRA, WHICH SUPPORTS THE MT. WILSON SOLAR OBSERVATORY'S MAGNETIC CLASSIFICATION OF THIS REGION AS A BETA-GAMMA-DELTA. NUMEROUS RADIO BURSTS AT VARIOUS FREQUENCIES WERE OBSERVED BEORE AND AFTER THE FLARE ACTIVITY. IN ADDITION, TWO FILAMENTS DISSAPPEARED OVERNIGHT FROM REGION 8026, WITH THE LARGER OF THE TWO (7 DEGREES) HAVING BECOME HIGHLY ACTIVE PRIOR TO DISAPPEARING.
IB. Päikese aktiivsuse ennustus
SOLAR ACTIVITY IS EXPECTED TO BE VERY LOW TO LOW, WITH A CONTINUED CHANCE FOR ISOLATED M-CLASS EVENTS FOR THE NEXT THREE DAYS.
IIA. Summaarne geofüüsikaline aktiivsus 31-2100Z kuni 01-2100Z
THE GEOMAGNETIC FIELD WAS MOSTLY UNSETTLED FOR THE FIRST HALF OF THE REPORTING PERIOD, WITH A SINGLE PERIOD OF ACTIVE CONDITIONS RECORDED AT FREDRICKSBURG DURING THE INTERVAL 01/0300-0600Z, AND THEN QUIET FOR THE SECOND HALF OF THE DAY. THE GREATER THAN 2 MEV ELECTRONS WERE IN THE MODERATE TO HIGH RANGE.
IIB. Geofüüsikalise aktiivsuse ennustus
THE GEOMAGNETIC FIELD IS EXPECTED TO BE QUIET TO UNSETTLED FOR THE NEXT THREE DAYS, WITH A CHANCE FOR ISOLATED PERIODS OF ACTIVE CONDITIONS.
III. Sündmuste tõenäosus 02 APRkuni 04 APR
Klass M20%15%10%
Klass X01%01%01%
Prooton01%01%01%
PCAFGREEN
IV. Pikklaine 10.7 cm kiirgus
  Vaadeldud       01 APR 076
  Prognoositud   02 APR-04 APR  076/077/078
  90 päeva keskmine        01 APR 074
V. Geomagneetiline A-indeks
OBSERVED AFR/AP 31 MAR  007/005
ESTIMATED AFR/AP 01 APR  012/010
PREDICTED AFR/AP 02 APR-04 APR  010/010-010/010-010/006
VI. Geomagnetilised aktiivsuse tõenäosused 02 APR kuni 04 APR
A. Keskmistel laiuskraadidel
Aktiivne20%20%20%
Väike torm10%10%10%
Suur-tõsine torm05%05%05%
B. Kõrgetel laiuskraadidel
Aktiivne25%25%25%
Väike torm15%15%15%
Suur-tõsine torm05%05%05%

<< Mine igapäevase ülevaate lehele

Viimane uudis

Toeta 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!

54%
Toetage SpaceWeatherLive meie kaupadega
Vaadake meie kaupa

Fakte kosmose ilmast

Viimane X-loide05/05/2024X1.2
Viimane M-loide05/05/2024M1.0
Viimane geomagnetiline torm02/05/2024Kp7- (G3)
Plekivabasid päevi
Viimane päikese plekivaba päev08/06/2022
Kuu keskmine päikeseplekkide arv
aprill 2024136.5 +31.6
Viimased 30 päeva153.8 +59.7

See päev ajaloos*

Päikesepursked ehk loited
12015X3.93
22024X1.2
32024X1.2
42024M8.3
52024M7.3
ApG
1193765G3
2198944G3
3199842G3
4195929G2
5193927G2
*alates 1994

Sotsiaalvõrgustikud