Välja antud: 2013 Jun 22 1210 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
22 Jun 2013 | 140 | 019 |
23 Jun 2013 | 145 | 005 |
24 Jun 2013 | 145 | 003 |
The background X-ray radiation is near the top of the B-level. NOAA AR 1777 has a probability of more than 50% to flare in the C-level. M-flares are still possible. Solar wind speed is around 600 km/s. The density and the magnetic field decreased. This behaviour of the solar wind parameters is a typical coronal hole signature: a co-rotating interaction region with relatively high density and compressed magnetic field is followed by the actual fast solar wind emanating from the coronal hole itself. This is a typical lower density plasma. Geomagnetic conditions returned to quiet/unsettled conditions.
Today's estimated international sunspot number (ISN): 083, based on 09 stations.
Wolf number Catania | /// |
10cm solar flux | 133 |
AK Chambon La Forêt | 027 |
AK Wingst | 020 |
Estimated Ap | 022 |
Estimated international sunspot number | 095 - Based on 17 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
Kõik ajad UTC-s
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