Affichage des archives de samedi, 18 octobre 2003
Rapport d'activité solaire
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.
Rapport d'activité solaire et géophysique 2003 Oct 18 2200 UTCFait par le NOAA © SWPC et adapté par SpaceWeatherLive.com
Rapport de l'USAF/NOAA sur l'activité solaire et géophysique
SDF numéro 291 publié à 2200Z le 18 Oct 2003IA. Analyse des régions solaires actives et activité du 17-2100Z au 18-2100Z Solar activity was low. A noticeable increase in flare
activity and background levels was observed during the past 24
hours. Most of this increase was due to newly numbered Region 484
(N05E68) which appears to be a compact D-type group with 240
millionths of area. The region produced numerous C-class flares: the
largest was a C4.9 at 1653 UTC. A partial halo CME was observed off
the southeast limb, beginning at 1554 UTC. The plane of sky velocity
was estimated to be about 700 km/s. Region 483 (S08E55) was assigned
today but so far is a small stable sunspot group. The other active
regions on the disk showed occasional brightenings but were mostly
quiet and stable.
IB. Prévisions d'activité solaire
Solar activity is expected to be low
for the next three days with Region 484 as the dominant source of
activity. There is a slight chance for an isolated M-class event
during the next three days.
IIA. Résumé de l'activité géophysique du 17-2100Z au 18-2100Z
The geomagnetic field ranged from unsettled to minor storm levels as
the high speed solar wind stream continues. The solar wind speed did
not show any trend today and the average velocity was around 540
km/s. The interplanetary magnetic field Z-component fluctuated
between -7 nT and + 5 nT but was weakly negative on average. The
greater than 2 MeV electron fluxes were at high levels during the
past 24 hours.
IIB. Prévision de l'activité géophysique
The geomagnetic field is
expected to be unsettled to active for the next 24 hours. There
should be a gradual decline in activity sometime tomorrow and
conditions should be mostly unsettled for the second day. An
increase to mostly active with some minor storm periods is expected
on the third day as a new coronal hole rotates into favorable
position at that time. Today's CME is not expected to directly
impact Earth but might result in a glancing blow that could provide
a boost to activity on the third day.
III. Probabilité d'éruption solaire du 19 Oct au 21 Oct
| Classe M | 20% | 20% | 20% |
| Classe X | 01% | 01% | 01% |
| Proton | 01% | 01% | 01% |
| PCAF | green | ||
IV. Flux Penticton 10.7 cm
Observé 18 Oct 109 Prévisionnel 19 Oct-21 Oct 115/115/120 Moyenne des 90 derniers jours 18 Oct 116
V. Indice géomagnetique A
Observé Afr/Ap 17 Oct 020/031 Estimé Afr/Ap 18 Oct 017/025 Prévisionnel Afr/Ap 19 Oct-21 Oct 012/020-012/015-020/030
VI. Probabilités d'activité géomagnétique du 19 Oct au 21 Oct
| A. Latitudes moyennes | |||
|---|---|---|---|
| Actif | 30% | 30% | 30% |
| Tempête mineure | 25% | 25% | 40% |
| Tempête majeure/sévère | 05% | 05% | 15% |
| B. Hautes latitudes | |||
|---|---|---|---|
| Actif | 30% | 30% | 25% |
| Tempête mineure | 25% | 25% | 30% |
| Tempête majeure/sévère | 05% | 05% | 35% |
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