Välja antud: 2019 Apr 20 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
20 Apr 2019 | 070 | 005 |
21 Apr 2019 | 070 | 003 |
22 Apr 2019 | 070 | 003 |
Solar activity was at very low levels. While rounding the west limb, NOAA 2738 produced 4 B-class flares, the strongest being a B8 flare peaking at 00:50UT. The lone sunspot group currently visible on the solar disk, NOAA 2739, was quiet and is decaying. No earth-directed coronal mass ejections were observed over the last 24 hours. The greater than 10 MeV proton flux was at nominal values. An equatorial negative polarity coronal hole (CH) is transiting the central meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed was fairly steady between 300 and 350 km/s (DSCOVR). Bz varied between -4 and +6 nT. The interplanetary magnetic field was mostly directed away from the Sun (positive sector) until about 07:00UT, when it switched back to towards the Sun (negative sector). Geomagnetic conditions were at quiet levels, with an isolated unsettled interval (14-17UT) recorded at Dourbes.
Quiet geomagnetic conditions are expected to continue, with a chance on an unsettled interval.
Today's estimated international sunspot number (ISN): 012, based on 26 stations.
Wolf number Catania | /// |
10cm solar flux | 073 |
AK Chambon La Forêt | 009 |
AK Wingst | /// |
Estimated Ap | 005 |
Estimated international sunspot number | 024 - Based on 28 stations |
Day | Begin | Max | Lõpp | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Puuduvad |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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