Viewing archive of Tuesday, 26 November 2013

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2013 Nov 26 1256 UTC

SIDC Forecast

Valid from 1230 UTC, 26 Nov 2013 until 28 Nov 2013
Solar flares

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

Geomagnetism

Quiet (A<20 and K<4)

Solar protons

Quiet

10cm fluxAp
26 Nov 2013119006
27 Nov 2013125007
28 Nov 2013125008

Bulletin

The active region which was the most active the past days turned over de west limb and is now out of view. A new active region is ready to rotate over the east limb in the southern hemisphere. It produced C-flare this morning and yesterday. More C-flares are likely. The solar wind speed is slow: around 300 km/s. The total interplanetary magnetic field (IMF) is even below 4nT. Consequently, there are no geomagnetic disturbances. The Kp and local K Dourbes are below 3. There is no indication yet that this situation will change, except for a small northern coronal hole that passed already the central meridian. The fast speed of this coronal hole might arrive late today or tomorrow.

Today's estimated international sunspot number (ISN): 025, based on 08 stations.

Solar indices for 25 Nov 2013

Wolf number Catania065
10cm solar flux119
AK Chambon La Forêt002
AK Wingst000
Estimated Ap001
Estimated international sunspot number030 - Based on 12 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

Vorkuta
The solar wind speed is currently moderately high (524.1 km/sec.)
The maximum X-ray flux of the past two hours is:
M1.08

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