Issued: 2015 Oct 19 1230 UTC
M-class flares expected (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 19 Oct 2015 | 120 | 007 |
| 20 Oct 2015 | 120 | 006 |
| 21 Oct 2015 | 120 | 011 |
Solar activity was low with only four low level C-class flares (C1.7 being the maximum) from NOAA active regions 2434 and 2436 and 2437. NOAA AR 2437, which had produced a few M-class flares on October 17, has rounded the East limb only producing flares at the C-level during the past period. Catania sunspot region 52 is a new region near S09E12. No Earth- directed CMEs were observed. Flaring activity at the C-level is expected.
The solar wind speed decreased from about 480 km/s to 400 km/s. The magnetic field magnitude currently is about 5 nT with a mainly negative Bz component. Mostly quiet to unsettled geomagnetic conditions were observed, which are expected to continue. There is a chance for a few episodes of active to minor storming conditions due to the moderate speed stream from an equatorial coronal hole, expected to arrive on October 21.
Today's estimated international sunspot number (ISN): 087, based on 09 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 120 |
| AK Chambon La Forêt | 023 |
| AK Wingst | 017 |
| Estimated Ap | 020 |
| Estimated international sunspot number | 071 - Based on 17 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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