Issued: 2017 Jun 26 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
26 Jun 2017 | 074 | 010 |
27 Jun 2017 | 075 | 013 |
28 Jun 2017 | 075 | 008 |
Solar activity was at very low levels during the period. NOAA 2664 is currently the only sunspot region on the solar disk. It is slowly developing and produced a B1 flare on 26 June at 07:28UT. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10MeV proton flux was at nominal levels.
Quiet flaring conditions are expected, with a small chance on a C-class flare.
Earth was under the influence of a moderate speed coronal hole wind stream. Solar wind speed continued its gradual increase with current values around 560 km/s (DSCOVR). Bz fluctuated between -7 and +6 nT. The interplanetary magnetic field was mostly directed away from the Sun. A small positive equatorial coronal hole was at the central meridian on 25 June.
The geomagnetic field was at quiet to unsettled levels, and is expected to remain so, but with a chance on an active episode.
Today's estimated international sunspot number (ISN): 024, based on 20 stations.
Wolf number Catania | /// |
10cm solar flux | 074 |
AK Chambon La Forêt | 019 |
AK Wingst | 013 |
Estimated Ap | 013 |
Estimated international sunspot number | 019 - Based on 27 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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