Issued: 2013 Oct 31 1249 UTC
Active (M-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 31 Oct 2013 | 130 | 015 |
| 01 Nov 2013 | 125 | 024 |
| 02 Nov 2013 | 120 | 003 |
There was only one C flare on the Sun during the past 24 hours, originating from Catania sunspot region 29 (NOAA active region 11884). The X-ray background level has been reduced to the B-level. For the next 48 hours, M flares are expected. No Earth directed CMEs were observed. The proton flux measured by GOES is currently decreasing. Solar wind speed reached a maximum of 400 km/s as observed by ACE. The magnitude of the interplanetary magnetic field (IMF) increased from 6 to 12 nT, mainly with a positive Bz component. Geomagnetic activity is quiet to unsettled (local K at Dourbes and NOAA Kp between 0 and 3). Unsettled to minor storm conditions (K= 3 to 5) are possible within the next 48 hours, due to weak effects of the CMEs that erupted on October 28.
Today's estimated international sunspot number (ISN): 089, based on 16 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 142 |
| AK Chambon La Forêt | 024 |
| AK Wingst | 015 |
| Estimated Ap | 016 |
| Estimated international sunspot number | 104 - Based on 25 stations |
| Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| None | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
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