Viewing archive of Monday, 7 December 2015

Daily bulletin on solar and geomagnetic activity from the SIDC

Issued: 2015 Dec 07 1230 UTC

SIDC Forecast

Valid from 1230 UTC, 07 Dec 2015 until 09 Dec 2015
Solar flares

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

Geomagnetism

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

Solar protons

Quiet

10cm fluxAp
07 Dec 2015103019
08 Dec 2015104018
09 Dec 2015105013

Bulletin

Solar activity remains to be low, with only two low C-class flares reported in the past 24 hours. The C1.1 flare observed at the East solar limb this morning (peaking at 04:19 UT) was associated with the coronal EUV wave and rather narrow CME. We do not expect significant change in the level of the solar activity. Low C-class flares are possible in the coming hours. No Earth directed CMEs were observed in the last 24 hours. The Earth is currently inside of the fast flow associated with the strongly extended northern polar coronal hole. During last 36 hours the solar wind speed is slowly increasing, with the current value of about 640 km/s. The interplanetary magnetic field magnitude is slightly elevated and it amounts about 14 nT. We expect further increase of the solar wind speed which, together with the possibly negative values of the Bz component of the interplanetary magnetic field, might induce active to minor storm geomagnetic conditions in the coming hours.

Today's estimated international sunspot number (ISN): 056, based on 14 stations.

Solar indices for 06 Dec 2015

Wolf number Catania///
10cm solar flux102
AK Chambon La Forêt037
AK Wingst023
Estimated Ap027
Estimated international sunspot number049 - Based on 22 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

<< Go to daily overview page

Active geomagnetic conditions

Observed Kp: 4
Threshold reached: 22:46 UTC

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

Reykjavik

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

Tórshavn
Oulu, Rovaniemi, Kuopio, Sodankylä
Trondheim
Arkhangelsk
Kiruna, Luleå, Sundsvall, Umeå
The direction of the interplanetary magnetic field is slightly South (-6.38nT).

Latest news

Support SpaceWeatherLive.com!

A lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!

Donate SpaceWeatherLive Pro
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

23:00 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 22:47 UTC

alert


20:45 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 50GW at 21:37 UTC


01:45 UTC - Geomagnetic activity

Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC

alert


Wednesday, 9 April 2025
08:12 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 76GW at 08:57 UTC


02:00 UTC - Geomagnetic activity

Minor G1 geomagnetic storm (Kp5) Threshold Reached: 01:45 UTC

alert


Get instant alerts!

Space weather facts

Last X-flare2025/03/28X1.1
Last M-flare2025/04/08M1.5
Last geomagnetic storm2025/04/06Kp5 (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
March 2025134.2 -20.4
April 2025144.7 +10.5
Last 30 days138.8 +1.3

This day in history*

Solar flares
12001X3.14
22002X1.17
32023M2.83
42002M2.34
52000M1.23
DstG
11990-281G4
21982-137G3
31957-124G3
41959-122G4
51960-81G3
*since 1994

Social networks