Viewing archive of onsdag, 26 oktober 2011
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 2011 Oct 26 2205 UTCSkapad av NOAA © SWPC och bearbetad av SpaceWeatherLive.com
USAF/NOAA rapport för sol- och geofysisk aktivitet
SDF Nummer 299 publicerat klockan 2200Z på 26 Oct 2011IA. Analys av solfläcksgrupper och solaktivitet från 25-2100Z till 26-2100Z Solar activity was at low levels due to a single C1
x-ray event at 26/1001Z from Region 1324 (N12W38). Associated with
this event was a partial-halo CME, first observed in LASCO C2
imagery lifting off the NW limb at 26/1000Z. GOES-15 SXI imagery
first observed material movement from Region 1324 in a W-NW
direction at about 26/0800Z. Limited imagery prevented a thorough
analysis of the CMEs potential geoeffectiveness. The region
exhibited significant decay in area and spot count and was
classified as a beta magnetic configuration. Regions 1325 (N17W12)
and 1327 (S20W67) also indicated decay in both area coverage and
spot count. The remaining regions were unchanged.
IB. Prognos för solaktivitet
Solar activity is expected to be low
with a slight chance for M-class activity all three days (27 - 29
October).
IIA. Sammanfattning av geofysisk aktivitet 25-2100Z till 26-2100Z
The geomagnetic field was quiet at all latitudes. Solar wind speeds
decayed through the period from near 550 km/s to about 400 km/s
while the Bz component of the interplanetary magnetic field did not
vary much beyond +/- 4 nT.
IIB. Prognos för geofysisk aktivitet
The geomagnetic field is
expected to be quiet on day one (27 October). Quiet to unsettled
conditions are expected on days two and three (28 - 29 October) as a
recurrent coronal hole high speed stream rotates into a geoeffective
position.
III. Chans för solutbrott från 27 Oct till 29 Oct
| M-klass | 10% | 10% | 10% |
| X-klass | 01% | 01% | 01% |
| Proton | 01% | 01% | 01% |
| PCAF | Green | ||
IV. Penticton 10.7 cm Flux
Observerad 26 Oct 132 Prognoserat 27 Oct-29 Oct 130/130/130 90 Day Mean 26 Oct 124
V. Geomagnetiskt A-index
Observerad Afr/Ap 25 Oct 027/033 Förväntat Afr/Ap 26 Oct 003/005 Prognoserat Afr/Ap 27 Oct-29 Oct 005/005-007/007-007/008
VI. Chanser för geomagnetisk aktivitet från 27 Oct till 29 Oct
| A. Medelhöga breddgrader | |||
|---|---|---|---|
| Aktivt | 05% | 10% | 10% |
| Små stormförhållanden | 01% | 01% | 01% |
| Svåra stormförhållanden | 01% | 01% | 01% |
| B. Höga breddgrader | |||
|---|---|---|---|
| Aktivt | 10% | 15% | 20% |
| Små stormförhållanden | 05% | 10% | 10% |
| Svåra stormförhållanden | 01% | 01% | 01% |
Senaste nytt
måndag, 22 april 2024
Lot's of sunspots! Big chance for major flare activity?
lördag, 23 mars 2024
X1.1 solar flare with earth-directed CME
onsdag, 20 mars 2024
Sunspot region 3615, G1 watch
Senaste inläggen
Unproven theories 344AR3654 25Unspecified geomagnetic activity 954Changelog/Featurelog 154What are these long and thin eruptions? 9
Fler foruminläggStöd SpaceWeatherLive.com!
För att vara tillgängliga vid stora norrskensutbrott måsta vi ha kraftiga servrar som kan hantera alla besökare. Donera och stöd vårt projekt, så att vi kan finnas online även under stora stormar!
Rymdvädersfakta
| Senaste X-utbrottet | 2024/03/28 | X1.1 |
| Senaste M-utbrottet | 2024/04/27 | M3.0 |
| Senaste geomagnetiska stormen | 2024/04/26 | Kp5+ (G1) |
| Fläckfria dagar | |
|---|---|
| Senaste dag utan solfläckar | 2022/06/08 |
| Månadsvis faktiskt antal solfläckar | |
|---|---|
| mars 2024 | 104.9 -19.8 |
| Last 30 days | 137.7 +30.3 |