Issued: 2014 Jun 01 1229 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 01 Jun 2014 | 109 | 003 |
| 02 Jun 2014 | 113 | 006 |
| 03 Jun 2014 | 116 | 003 |
There are currently 5 sunspot regions visible. Three C-class flares were recorded over the last 24 hours. Near the time of its disappearance from the solar surface, active region NOAA 2076 produced a C1-flare peaking at 15:56UT. The strongest event of the period was a C2-flare in NOAA 2079 peaking at 01:37UT. The associated CME was directed away from Earth. NOAA 2077 produced a C1-flare peaking at 11:53UT. Further C-class flaring is expected, in particular from sunspot regions NOAA 2077 and NOAA 2079. Solar wind speed declined from about 350 to 300 km/s, Bz being mostly positive with maximum excursions to +8 nT. The geomagnetic field was quiet. A small coronal hole that passed the central meridian on 29 May can influence the geomagnetic field as of 2 June. Geomagnetic conditions are expected to remain quiet, though locally a brief active episode is possible.
Today's estimated international sunspot number (ISN): 045, based on 17 stations.
| Wolf number Catania | /// |
| 10cm solar flux | /// |
| AK Chambon La Forêt | 007 |
| AK Wingst | 004 |
| Estimated Ap | 003 |
| Estimated international sunspot number | /// - Based on /// 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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