Issued: 2016 May 30 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
30 May 2016 | 080 | 015 |
31 May 2016 | 075 | 014 |
01 Jun 2016 | 075 | 010 |
A new active region (AR) NOAA 2550 has developed rapidly during the past few hours. Solar flaring activity was restricted to a C1.4 flare (peaking at 7:37 UT, originating from NOAA AR 2550) and several B-class flares. The C1.4 flare was associated with a type II burst, observed at Humain. No Earth directed coronal mass ejections (CMEs) were observed.
The probability for a C-class flare is increasing, with mainly NOAA AR 2550 as source candidate. The Earth is currently under the influence of a coronal hole (CH) high speed stream (HSS). Solar wind speed increased from 450 km/s, reaching a maximum of 600 km/s and is currently around 500 km/s. Bz ranged from -5 and +5 nT, with a maximum magnitude of the interplanetary magnetic field (IMF) of 8 nT. The IMF was directed towards the Sun. Quiet (K=0-2) to unsettled (K=3) conditions were registered at the local level (Dourbes). Some episodes with active conditions are expected over the next 24 hours.
Today's estimated international sunspot number (ISN): 047, based on 10 stations.
Wolf number Catania | /// |
10cm solar flux | 083 |
AK Chambon La Forêt | 018 |
AK Wingst | 007 |
Estimated Ap | 008 |
Estimated international sunspot number | 030 - Based on 20 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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