Het archief bekijken van donderdag 8 september 2005
Activiteitenrapport
Rapport van de zonne- en geofysische activiteit van 2005 Sep 08 2204 UTCOpgemaakt door de NOAA © SWPC en verwerkt door Poollicht.be
USAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 251 gepubliceerd omstreeks 2200Z op 08 Sep 2005IA. Analyse van de actieve zonneregio's en zonneactiviteit van 07-2100Z tot 08-2100Z Solar activity remains at high levels. An X5/2b flare
was in progress from Region 808 (S09E67) at the time of this
writing. Moderate centimetric radio bursts are also in progress,
including a 990 sfu Tenflare. Very active Region 808 is rotating
into view as a large and complex sunspot cluster. Limb proximity is
still hindering the analysis, but this compact spot group will
likely exceed 1000 millionths of white light area. Numerous C-class
flares and two M2 flares preceded the X5 event. New Region 809
(N10E60) was numbered today.
IB. Voorspelling zonneactiviteit
Solar activity is expected to remain
at high levels. Region 808 is a large and complex sunspot group
capable of producing M and X-class flares.
IIA. Samenvatting geofysische activiteit 07-2100Z tot 08-2100Z
The geomagnetic field was quiet to unsettled. A sudden disturbance of
41 nT (magnetic crochet) was observed in the geomagnetic field
following today's X5 flare. A greater than 10 and greater than 100
MeV proton event occurred following yesterday's X17 flare on the
southeast limb. The greater than 10 MeV proton event began at
08/0215Z and remains in progress. The peak flux so far was 87 pfu at
08/1950Z. The greater than 100 MeV proton event began at 08/0405Z
and also remains in progress. The peak flux was 7 pfu at 08/1925Z.
A greater than 100 MeV proton event from a source on the east
limb is extremely rare. The greater than 2 MeV electron flux at
geosynchronous orbit was at high levels again today.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to range from quiet to minor storm levels. The CME
associated with yesterday's X17 flare was very large and very fast.
Although the magnetic cloud associated with this CME is not expected
to impact Earth, a shock passage is expected, which will likely
produce active to minor storm periods on 09 Sep. Isolated active
periods are expected on 10 and 11 Sep. The greater than 10 MeV
proton event currently in progress is expected to continue through
10 Sep. A further enhancement in the greater than 10 MeV protons
will likely follow the anticipated shock passage on 09 Sep. Today's
X5 flare may enhance the existing proton event. The greater than 100
MeV proton event will persist through 09 Sep.
III. Kans zonnevlammen van 09 Sep tot 11 Sep
| Klasse M | 80% | 80% | 80% |
| Klasse X | 50% | 50% | 50% |
| Proton | 99% | 90% | 75% |
| PCAF | in progress | ||
IV. Penticton 10.7 cm Flux
Geobserveerd 08 Sep 094 Voorspeld 09 Sep-11 Sep 100/110/110 90 Day Mean 08 Sep 091
V. Geomagnetische A index
Geobserveerd Afr/Ap 07 Sep 018/015 Verwacht Afr/Ap 08 Sep 008/012 Voorspeld Afr/Ap 09 Sep-11 Sep 020/025-015/020-008/010
VI. Kansen geomagnetische activiteit van 09 Sep tot 11 Sep
| A. Gemiddelde breedtegraad | |||
|---|---|---|---|
| Actief | 40% | 30% | 25% |
| Kleine stormcondities | 20% | 15% | 10% |
| Zware-ernstige stormcondities | 10% | 05% | 01% |
| B. Hoge breedtegraad | |||
|---|---|---|---|
| Actief | 50% | 40% | 30% |
| Kleine stormcondities | 30% | 20% | 15% |
| Zware-ernstige stormcondities | 15% | 10% | 05% |
Laatste nieuws
zondag 15 januari 2023
Busy Sun! M-class flares and coronal mass ejections!
maandag 9 januari 2023
X1.9 solar flare
vrijdag 6 januari 2023
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