Vaata esmaspäev, 7 mai 2012 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 2012 May 07 2200 UTC
Valminud NOAA © SWPC ja töödeldud SpaceWeatherLive.com-igaÜhine USAF / NOAA päikese- ja geofüüsikaalase aktiivsuse aruanne
SDF number 128 Välja antud 2200Z kuni 07 May 2012
IA. Päikese aktiivsete piirkondade ja päikeseaktiivsuse analüüs alates 06-2100Z kuni 07-2100Z
Solar activity has been at moderate levels for the past
24 hours. Even though Region 1476 (N10E48) is the largest, 810
Millionths, and most magnetically complex, Fkc/beta-gamma; todays
only M-class event came from the sunspot cluster Region 1470
(S15W57) and Region 1471 (S19W50). This sunspot complex produced an
M1/1n x-ray event at 07/1431Z. Multiple discrete radio frequency
bursts were associated with this event, as well as a 240 sfu
Tenflare and a Type IV radio sweep. These characteristics, as well
as COR2 imagery from the STEREO A spacecraft suggest an Earth
directed CME. Initial analysis suggests only a weak disturbance of
the Earths magnetic field. Earlier in the day around 07/0400Z,
another CME was observed in STEREO A imagery but after analysis, it
was determined to not have an Earth-directed component. Region 1476
continues to grow in size and magnetic complexity as it rotates
further onto the solar disk.
IB. Päikese aktiivsuse ennustus
Solar activity is expected to be at
low to moderate levels for the next three days (08 - 10 May).
IIA. Summaarne geofüüsikaline aktiivsus 06-2100Z kuni 07-2100Z
The geomagnetic field has been at quiet levels for the past 24 hours.
IIB. Geofüüsikalise aktiivsuse ennustus
The geomagnetic field is
expected to be at quiet to unsettled levels on day one (08 May) as a
solar sector boundary crossing is expected, as well as possible
effects from a weak CME, observed leaving the solar disk on 05 May.
Quiet to unsettled with a chance for active levels are expected on
day two (09 May), as a coronal hole high-speed stream (CH HSS) moves
into a geoeffective position. Quiet to active levels with a chance
for minor storm levels are expected on day three (10 May) as effect
from the CH HSS continue with the possible arrival of todays CME.
III. Sündmuste tõenäosus 08 Maykuni 10 May
Klass M | 75% | 75% | 75% |
Klass X | 10% | 10% | 10% |
Prooton | 01% | 01% | 01% |
PCAF | green
|
IV. Pikklaine 10.7 cm kiirgus
Vaadeldud 07 May 122
Prognoositud 08 May-10 May 120/120/120
90 päeva keskmine 07 May 112
V. Geomagneetiline A-indeks
Vaadeldud Afr/Ap 06 May 005/004
Hinnanguline Afr/Ap 07 May 004/004
Prognoositud Afr/Ap 08 May-10 May 007/007-009/012-015/015
VI. Geomagnetilised aktiivsuse tõenäosused 08 May kuni 10 May
A. Keskmistel laiuskraadidel |
Aktiivne | 10% | 35% | 40% |
Väike torm | 01% | 10% | 20% |
Suur-tõsine torm | 01% | 01% | 05% |
B. Kõrgetel laiuskraadidel |
Aktiivne | 15% | 45% | 40% |
Väike torm | 01% | 20% | 25% |
Suur-tõsine torm | 01% | 05% | 10% |
Kõik ajad UTC-s
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