Visualització de l'arxiu de dimecres, 18 d’abril 2001

Informe d'activitat solar

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.
Informe d'activitat Geofísica-Solar 2001 Apr 18 2200 UTC
Preparat pel SWPC NOAA © i processat per SpaceWeatherLive.com

Informe conjunt segons USAF / NOAA d’activitat Solar i Geofísica

SDF número 108 emès a 2200Z el Apr 18 2001

IA. Anàlisi de les regions actives solars i de l'activitat de 2100Z-17 a 2100Z-18

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. Previsió d'activitat solar
Solar activity is expected to be predominantly low with a chance for an isolated M flare from Region 9433.
IIA. Resum d'activitat geofísica del 2100Z-17 al 2100Z-18
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. Previsió d'activitat geofísica
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. Probabilitats d’esdeveniments de les Apr del 19 a les Apr del 21
Classe M40%40%40%
Classe X05%05%05%
Protó99%10%01%
PCAFin progress
IV. Penticton Flux de 10,7 cm
  Observat       18 Apr 132
  Predit   19 Apr-21 Apr  135/145/155
  Mitjana de 90 dies        18 Apr 165
V. Índexs geomagnètics A
  Observat Afr/Ap 17 Apr  004/007
  Estimat     Afr/Ap 18 Apr  028/050
  Predit    Afr/Ap 19 Apr-21 Apr  012/015-010/015-005/010
VI. Probabilitats d’activitat geomagnètica del 19 Apr al 21 Apr
A. Latituds mitjanes
Actiu30%25%10%
Tempesta menor05%05%01%
Tempesta major-severa01%01%01%
B. Latituds altes
Actiu50%50%30%
Tempesta menor15%15%05%
Tempesta major-severa05%05%01%

All times in UTC

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