Issued: 2019 Jun 26 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
26 Jun 2019 | 068 | 008 |
27 Jun 2019 | 067 | 011 |
28 Jun 2019 | 067 | 006 |
Solar flaring activity continues to be very low without flares reported. One of the two numbered active regions NOAA AR 2742 rotated behind the west solar limb. Presently only one active region is observed on the visible side of the Sun, Catania sunspot group 19 (NOAA AR 2743). This sunspot group has only alpha configuration of its photospheric magnetic field and is therefore not expected to be source of flaring activity in the coming hours. During last few days only very narrow and slow CMEs were reported and there were no Earth directed CMEs. The solar protons remained at the background level.
The solar wind speed is presently about 400 km/s and slowly increasing. The interplanetary magnetic field magnitude remains to be low, with the value of about 3 nT. The in situ observations do not show clear signatures of the fast solar wind, but observed increase of the solar wind speed could be possibly associated with the expected arrival of the fast solar wind. The geomagnetic conditions are quiet and we expect quiet to possibly unsettled geomagnetic conditions.
Today's estimated international sunspot number (ISN): 011, based on 18 stations.
Wolf number Catania | 011 |
10cm solar flux | 068 |
AK Chambon La Forêt | 009 |
AK Wingst | 004 |
Estimated Ap | 005 |
Estimated international sunspot number | 012 - Based on 26 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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