Viewing archive of fredag, 28 mars 2003
Solaktivitetsrapport
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 för sol- och geofysisk aktivitet 2003 Mar 28 2200 UTCSkapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com
USAF/NOAA rapport för sol- och geofysisk aktivitet
SDF Nummer 087 publicerat klockan 2200Z på 28 Mar 2003IA. Analys av solfläcksgrupper och solaktivitet från 27-2100Z till 28-2100Z Solar activity was low due to a single C1 flare at
27/2325Z, likely associated with activity from near the southwest
limb. Region 319 (N12W18) has stabilized following a period of
rapid growth in the previous 24 hours. Despite its moderate size,
this region maintains a fairly simple magnetic configuration and has
been stable. Region 321 (N04E21) exhibited slight decay and was
relatively quiet this period. New Region 326 (S12E74) was numbered
today.
IB. Prognos för solaktivitet
Solar activity is expected to continue
at low levels. Regions 319 and 321 have good potential for C-class
flares and a small chance for an M-class event.
IIA. Sammanfattning av geofysisk aktivitet 27-2100Z till 28-2100Z
The geomagnetic field was mostly quiet to active with isolated minor
storm periods during local nighttime hours. The most active
conditions early in the period were due to a waning high speed
coronal hole stream. A weak transient passed the ACE spacecraft
between 28/1400 - 1500Z. Predominantly southward Bz in the IMF
resulted in active levels late in the period. The greater than 2 MeV
electron fluxes at geosynchronous orbit reached high levels.
IIB. Prognos för geofysisk aktivitet
The geomagnetic field is
expected to be quiet to active. Isolated minor storm periods at
higher latitudes are possible through day one and again on day three
as another weak coronal hole moves into a geoeffective position.
III. Chans för solutbrott från 29 Mar till 31 Mar
| M-klass | 30% | 30% | 30% |
| X-klass | 05% | 05% | 05% |
| Proton | 01% | 01% | 01% |
| PCAF | green | ||
IV. Penticton 10.7 cm Flux
Observerad 28 Mar 147 Prognoserat 29 Mar-31 Mar 150/155/150 90 Day Mean 28 Mar 133
V. Geomagnetiskt A-index
Observerad Afr/Ap 27 Mar 016/027 Förväntat Afr/Ap 28 Mar 018/020 Prognoserat Afr/Ap 29 Mar-31 Mar 012/012-010/012-015/015
VI. Chanser för geomagnetisk aktivitet från 29 Mar till 31 Mar
| A. Medelhöga breddgrader | |||
|---|---|---|---|
| Aktivt | 40% | 25% | 30% |
| Små stormförhållanden | 20% | 10% | 15% |
| Svåra stormförhållanden | 05% | 01% | 01% |
| B. Höga breddgrader | |||
|---|---|---|---|
| Aktivt | 50% | 35% | 40% |
| Små stormförhållanden | 25% | 15% | 20% |
| Svåra stormförhållanden | 10% | 05% | 05% |
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