Het archief bekijken van woensdag 18 april 2001

Activiteitenrapport

Rapport van de zonne- en geofysische activiteit van 2001 Apr 18 2200 UTC
Opgemaakt door de NOAA © SWPC en verwerkt door Poollicht.be

USAF/NOAA rapport van de zonneactiviteit en geofysische activiteit

SDF Nummer 108 gepubliceerd omstreeks 2200Z op 18 Apr 2001

IA. Analyse van de actieve zonneregio's en zonneactiviteit van 17-2100Z tot 18-2100Z

Solar activity was moderate. The largest flare of the period was an optically uncorrelated M1 at 17/2157 UTC. EIT imagery suggests the source of this flare to be returning Region 9393, which has been newly numbered as Region 9433 (N15E74). Old Region 9415 (L=360) produced a C2 flare, CME, Type II sweep, and 570 sfu tenflare at 18/0215 UTC. The region was almost 25 degrees beyond the West limb at the time, which likely masked the full strength of the x-ray flare. New Region 9432 (N09E21) was also numbered today.
IB. Voorspelling zonneactiviteit
Solar activity is expected to be predominantly low with a chance for an isolated M flare from Region 9433.
IIA. Samenvatting geofysische activiteit 17-2100Z tot 18-2100Z
The geomagnetic field has been quiet to minor storm, with severe storm conditions at high latitudes. An interplanetary shock passed the ACE spacecraft at 18/0005 UTC; subsequently the Boulder magnetometer registered a 50 nT sudden impulse at 18/0048 UTC. This shock was likely associated with the X14/2B on 15 April. Greater than 10 MeV and greater than 100 MeV proton events began at 18/0315 UTC and 18/0255 UTC respectively, most likely associated with the activity from old Region 9415 discussed in Part IA. The greater than 10 MeV protons reached a peak of 321 pfu at 18/1045 UTC, while the greater than 100 MeV protons reached 12 pfu at 18/0600 UTC. The Thule neutron monitor measured a ground level event between 18/0242 UTC and 18/0914 UTC; a polar cap absorption (PCA) event began at 18/0425 UTC and remains in progress. Values for the greater than 2 MeV electrons at geosynchronous orbit were not reported due to sensor contamination by the proton event.
IIB. Voorspelling geofysische activiteit
The geomagnetic field is expected to be quiet to active on day one of the forecast period, dropping to quiet to unsettled on days two and three. The proton events and PCA are expected to end on day one.
III. Kans zonnevlammen van 19 Apr tot 21 Apr
Klasse M40%40%40%
Klasse X05%05%05%
Proton99%10%01%
PCAFin progress
IV. Penticton 10.7 cm Flux
  Geobserveerd       18 Apr 132
  Voorspeld   19 Apr-21 Apr  135/145/155
  90 Day Mean        18 Apr 165
V. Geomagnetische A index
  Geobserveerd Afr/Ap 17 Apr  004/007
  Verwacht     Afr/Ap 18 Apr  028/050
  Voorspeld    Afr/Ap 19 Apr-21 Apr  012/015-010/015-005/010
VI. Kansen geomagnetische activiteit van 19 Apr tot 21 Apr
A. Gemiddelde breedtegraad
Actief30%25%10%
Kleine stormcondities05%05%01%
Zware-ernstige stormcondities01%01%01%
B. Hoge breedtegraad
Actief50%50%30%
Kleine stormcondities15%15%05%
Zware-ernstige stormcondities05%05%01%

<< Keer terug naar de overview pagina

Laatste nieuws

Steun Poollicht.be!

Om ook bereikbaar te blijven bij grote poollichtkansen hebben we een zware server nodig die alle bezoekers aankan. Doneer en steun dit project zodat we online blijven en je geen enkele poollichtkans mist!

59%
Steun SpaceWeatherLive met onze merchandise
Check nu onze merchandise

Ruimteweer feitjes

Laatste X-klasse uitbarsting10/05/2022X1.5
Laatste M-klasse uitbarsting25/05/2022M1.3
Laatste geomagnetische storm30/04/2022Kp5 (G1)
Zonnevlekkenloze dagen
Laatste zonnevlekkenloze dag11/12/2021

Deze dag in de geschiedenis*

Zonnevlammen
12003M1.9
21999M1.2
32003M1.0
42005C8.6
52003C7.4
ApG
1202112G1
2200316
3201318
4200015
5200713
*sinds 1994

Sociale netwerken