Het archief bekijken van zondag 17 oktober 2010
Activiteitenrapport
Bij elke genoemde zonnevlam in dit rapport werd een schaalfactor toegepast door het Space Weather Prediction Center (SWPC). Vanwege de SWPC-schaalfactor worden zonnevlammen 42% kleiner gerapporteerd dan voor de wetenschappelijke data. De schaalfactor werd verwijderd uit onze gearchiveerde zonnevlamdata om de werkelijke fysieke eenheden weer te geven.
Rapport van de zonne- en geofysische activiteit van 2010 Oct 17 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.beUSAF/NOAA rapport van de zonneactiviteit en geofysische activiteit
SDF Nummer 290 gepubliceerd omstreeks 2200Z op 17 Oct 2010
IA. Analyse van de actieve zonneregio's en zonneactiviteit van 16-2100Z tot 17-2100Z
Solar activity was at low levels due to a few C-class
events from Region 1112 (S20W44), the largest a C1.7 x-ray event
observed at 17/0859Z. The region continued to evolve over the past
24 hours, increasing in both area and extent, while maintaining
Beta-Gamma magnetic characteristics. New Region 1116 (N22W14) was
numbered as a simple bi-polar spot group.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be at
very low to low levels all three days of the forecast period (18 -
20 October), with a chance for M-class events from evolving Region
1112.
IIA. Samenvatting geofysische activiteit 16-2100Z tot 17-2100Z
The geomagnetic field ranged from quiet to minor storm levels during
the period. Activity was at quiet to unsettled levels until about
17/0700Z when the field became disturbed. Geomagnetic activity
increased to active to minor storm levels through 17/0900Z,
returning to mostly quiet levels through the remainder of the
period. At about 17/0400Z, signatures at the ACE satellite indicated
gradual increases in temperature, density and wind velocity. The Bz
component of the interplanetary magnetic field (IMF) turned
southward, and remained south for about 7 hours, reaching a maximum
deflection of -7nT at 17/0737Z. The Bt component of the IMF reached
a maximum of 10nT at 17/0520Z. This short-lived disturbance is
thought to have been a result of a glancing blow from the
slow-moving CME observed on 10 October.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is
expected to be at quiet to active levels all three days of the
forecast period (18 - 20 October). Isolated minor storm periods are
possible on 19 October. A coronal hole high speed stream (CH HSS) is
expected to rotate into a geoeffective position late on 18 October,
followed by a second geoeffective CH HSS likely to arrive early on
20 October. These features, coupled with possible effects from the
CME observed on 14 October, expected to arrive on 19 October, are
the reasons for the forecasted increase in geomagnetic activity.
III. Kans zonnevlammen van 18 Oct tot 20 Oct
Klasse M | 25% | 25% | 25% |
Klasse X | 01% | 01% | 01% |
Proton | 01% | 01% | 01% |
PCAF | Green
|
IV. Penticton 10.7 cm Flux
Geobserveerd 17 Oct 084
Voorspeld 18 Oct-20 Oct 086/086/086
90 dagen gemiddelde 17 Oct 081
V. Geomagnetische A index
Geobserveerd Afr/Ap 16 Oct 003/006
Geraamd Afr/Ap 17 Oct 009/013
Voorspeld Afr/Ap 18 Oct-20 Oct 008/010-012/012-008/010
VI. Kansen op geomagnetische activiteit van 18 Oct tot 20 Oct
A. Gemiddelde breedtegraad |
Actief | 20% | 30% | 20% |
Kleine storm | 05% | 15% | 05% |
Zware-ernstige stormcondities | 01% | 01% | 01% |
B. Hoge breedtegraad |
Actief | 25% | 35% | 25% |
Kleine storm | 15% | 20% | 15% |
Zware-ernstige stormcondities | 01% | 01% | 01% |
Alle tijden in UTC
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