Vaata esmaspäev, 26 juuli 2004 arhiivi
Päikese aktiivsuse aruanne
Igale käesolevas aruandes mainitud päikesepurskele on kohaldatud Kosmose Ilmaennustuskeskuse (SWPC) skaalafaktor. SWPC skaleerimisteguri tõttu on päikesepursked esitatud 42% väiksemana kui samade teadusliku kvaliteediga andmete puhul. Meie arhiveeritud päikesepursete andmetest on skaleerimisstegur eemaldatud, et kajastada tegelikke füüsikalisi ühikuid.
Päikese ja geofüüsikalise aktiivsuse aruanne 2004 Jul 26 2200 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 208 Välja antud 2200Z kuni 26 Jul 2004IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 25-2100Z kuni 26-2100Z Solar activity was moderate. Region 652 (N08W47)
produced two M-class flares - an M1/Sf at 26/0552Z, and an M1/2n at
26/1730Z. This region continues in a slow decay phase, but still
exceeds 1000 millionths of white light area coverage in a moderately
complex beta-gamma-delta configuration. Growth was observed in
newly numbered Region 654 (N07E38), but no activity of note has
occurred. The remainder of the disk and limb was quiet.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be
moderate. Region 652 will likely produce further M-class activity
and still maintains potential for a major flare.
IIA. Summaarne geofüüsikaline aktiivsus 25-2100Z kuni 26-2100Z
The geomagnetic field ranged from quiet to severe storm levels. The
severe geomagnetic storm that occurred yesterday, continued into the
early hours of this period. Major to severe geomagnetic storm
periods were observed through 26/0300Z. Solar wind speed remained
elevated from 500 to over 700 km/s, but IMF Bz was generally around
zero from 0300Z through the end of the period. Consequently, the
geomagnetic field was mostly quiet to unsettled. The greater than 10
MeV proton event that began yesterday at 25/1855Z, is still in
progress. The peak so far was 271 pfu at 26/1905Z. The greater than
2 MeV electrons at geosynchronous orbit reached high levels today.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to range from quiet to major storm levels. A full halo CME
was observed on LASCO imagery following yesterday's long duration M1
flare at 25/1514Z. This CME will likely impact the geomagnetic field
early on 27 July. Expect minor to major storm periods at all
latitudes and severe storm levels at high latitudes. The storm is
expected to end by 28 July. Mostly unsettled to active conditions
are expected on 28 July. A return to quiet to unsettled levels is
expected on 29 July with isolated high latitude active periods
possible. The greater than 10 MeV proton event in progress now will
likely end on 28 July.
III. Sündmuste tõenäosus 27 Julkuni 29 Jul
| Klass M | 65% | 65% | 50% |
| Klass X | 15% | 10% | 10% |
| Prooton | 99% | 25% | 10% |
| PCAF | red | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 26 Jul 128 Prognoositud 27 Jul-29 Jul 125/120/115 90 päeva keskmine 26 Jul 105
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 25 Jul 064/122 Hinnanguline Afr/Ap 26 Jul 020/040 Prognoositud Afr/Ap 27 Jul-29 Jul 060/055-025/030-015/020
VI. Geomagnetilised aktiivsuse tõenäosused 27 Jul kuni 29 Jul
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 40% | 20% |
| Väike torm | 40% | 20% | 10% |
| Suur-tõsine torm | 40% | 10% | 05% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 20% | 50% | 30% |
| Väike torm | 30% | 25% | 15% |
| Suur-tõsine torm | 50% | 15% | 05% |
Kõik ajad UTC-s
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