Viewing archive of Wednesday, 16 March 2016

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2016 Mar 16 1231 UTC

SIDC Forecast

Valid from 1230 UTC, 16 Mar 2016 until 18 Mar 2016
Solar flares

C-class flares expected, (probability >=50%)

Geomagnetism

Active conditions expected (A>=20 or K=4)

Solar protons

Warning condition (activity levels expected to increase, but no numeric forecast given)

10cm fluxAp
16 Mar 2016095025
17 Mar 2016095011
18 Mar 2016095005

Bulletin

Two C-class flares were observed during the last 24 hours, with a C2.2 flare as the strongest one. The C2.2 flare peaked at 6:46 UT this morning and originated from NOAA active region 2522, which is located at the West limb. The flare was associated with a CME with first measurement at 7:00 UT in LASCO/C2. A first analysis indicates there is no Earth directed component, but further analysis will be needed to confirm this. There was also a radio type II burst observed (at Humain) and an enhancement in the proton flux at >10MeV was noted. The threshold for a proton event has not been exceeded at this moment, but further increases of the proton flux are possible. Flaring at the C-level is expected to continue.

The solar wind is still under influence of the coronal hole high speed stream, with solar wind speeds between 450 and 600 km/s. The magnetic field magnitude is nearly 10 nT with a fluctuating north-south component. Geomagnetic conditions reached minor storm levels (K=5) for several time slots before and after UT midnight, both at the local (Dourbes) and global (estimated NOAA Kp) level. Quiet to unsettled conditions, with a few isolated slots of active levels are expected.

Today's estimated international sunspot number (ISN): 063, based on 14 stations.

Solar indices for 15 Mar 2016

Wolf number Catania///
10cm solar flux094
AK Chambon La Forêt039
AK Wingst029
Estimated Ap028
Estimated international sunspot number053 - Based on 25 stations

Noticeable events summary

DayBeginMaxEndLocStrengthOP10cmCatania/NOAARadio burst types
None

Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive

All times in UTC

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Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Gillam, MB, Yellowknife, NT
The solar wind speed is currently moderately high (599.9 km/sec.)

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