Emesso: 2013 Feb 17 1157 UTC
Eruptive (C-class flares expected, probability >= 50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
17 Feb 2013 | 108 | 006 |
18 Feb 2013 | 112 | 007 |
19 Feb 2013 | 116 | 011 |
Solar activity was low during the past 24 hours, with only a C1.0 flare on Feb. 17 (0036 UT peak time) from a new region, NOAA AR 1675, which emerged on Feb. 16. This is the main source for additional C flares in the next 48 hours, together, albeit with a lower probability, with NOAA AR 1671 and 1673. Geomagnetic activity was unsettled to active at planetary levels and reached even minor storm conditions at local level (K=5 at Dourbes from 15 to 18UT). This corresponds to a small shock observed by the ACE spacecraft around 1200 UT, linked to a moderate fast solar wind stream, associated with a coronal hole becoming geoeffective. Bz excursions down to -10 nT were observed on that day around 1400UT. We expect quiet conditions to prevail for the next 48 hours, and then reach unsettled to possibly active conditions for isolated periods, by the end of Feb. 19, or the the first half of Feb. 20, due to the arrival of the CME of Feb. 15.
Today's estimated international sunspot number (ISN): 061, based on 05 stations.
Wolf number Catania | /// |
10cm solar flux | 103 |
AK Chambon La Forêt | 019 |
AK Wingst | 010 |
Estimated Ap | 011 |
Estimated international sunspot number | 021 - Based on 07 stations |
Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
---|---|---|---|---|---|---|---|---|---|---|
Nessuna |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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