Vaata kolmapäev, 5 mai 2010 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 2010 May 05 2201 UTCValminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-iga
Ühine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 125 Välja antud 2200Z kuni 05 May 2010IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 04-2100Z kuni 05-2100Z Solar activity increased to moderate levels. Region
1069 (N41W40) produced an M1/Sf flare at 05/1719Z and a C8 flare at
05/1152Z, as well as occasional lesser B- and C-class flares. Region
1069 gradually increased in area and maintained a beta-gamma
magnetic configuration. Region 1066 (S26W22) produced a B4 flare at
05/1618Z associated with an EIT-wave/dimming event. New Region 1070
(N21W08), a small simple B-type spot group, was assigned late in the
period.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be low
during days 1 - 3 (06 - 08 May) with a chance for isolated M-class
flares from Region 1069.
IIA. Summaarne geofüüsikaline aktiivsus 04-2100Z kuni 05-2100Z
Geomagnetic field activity was at quiet to (briefly) unsettled
levels. ACE solar wind measurements indicated Earth remained within
a subsiding coronal hole high-speed stream. Velocities gradually
decreased from 620 to 538 km/sec during the summary period. The
greater than 2 MeV electron flux at geosynchronous orbit reached
high levels during the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
Geomagnetic field activity is
expected to be at mostly quiet levels during days 1 - 2 (06 - 07
May) as the coronal hole high-speed stream continues to subside.
Field activity is expected to increase to unsettled levels on day 3
(08 May) in response to the B4 wave/dimming event mentioned above.
III. Sündmuste tõenäosus 06 Maykuni 08 May
| Klass M | 30% | 30% | 30% |
| Klass X | 01% | 01% | 01% |
| Prooton | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 05 May 083 Prognoositud 06 May-08 May 084/084/084 90 päeva keskmine 05 May 082
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 04 May 007/010 Hinnanguline Afr/Ap 05 May 006/008 Prognoositud Afr/Ap 06 May-08 May 005/005-005/005-010/010
VI. Geomagnetilised aktiivsuse tõenäosused 06 May kuni 08 May
| A. Keskmistel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 10% | 05% | 15% |
| Väike torm | 01% | 01% | 01% |
| Suur-tõsine torm | 01% | 01% | 01% |
| B. Kõrgetel laiuskraadidel | |||
|---|---|---|---|
| Aktiivne | 15% | 10% | 20% |
| Väike torm | 05% | 01% | 01% |
| Suur-tõsine torm | 01% | 01% | 01% |
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