Tuesday 27th of June 2017
Wolverhampton Amateur Radio Society
Founded in 1922 | Call sign G8TA

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Regional Winner

COTY Regional winner

Wolverhampton Amateur Radio Society winner of the RSGB West Midlands Regional club of the year 2012 and 2013.
2012 was a fantastic year for Wolverhampton ARS, a year of rejuvenation as well as our 90th Birthday. We have seen a steady growth in our membership and with a full program of events we have become more active than in recent years and went on to win the Regional award for 2013.
The West Midlands Trophy is sponsored by web hosting solutions at www.intermip.net

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The Radio Society of Great Britain (RSGB) is the UK's national membership organisation for amateur radio enthusiasts. For more information on the RSGB [click here]

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Solar Data

Space Weather Feed[+]

Recurrent CH HSS sparks G1 geomagnetic storming
Earth is under the influence of a recurrent, negative polarity coronal hole high speed stream (CH HSS) today which is causing G1 - Minor geomagnetic storming. Solar wind speed increased to 548 km/s at 08:08 UTC while total field reached a maximum of 16 nT at 07:16...... Read more

CME impact sparks G3 - Strong geomagnetic storm
A coronal mass ejection (CME) produced during the early UTC hours of May 23, 2017 hit Earth's magnetic field at 15:36 UTC on May 27, more than 24 hours after it was expected. Although the solar wind speed is relatively slow, the embedded magnetic field had a...... Read more

CME headed toward Earth, impact expected around 12:00 UTC on May 26
An eruption near the center of Earth-facing side of the Sun produced a partial HALO CME (coronal mass ejection) during the early UTC hours of May 23, 2017. The CME is weak, but it has an Earth-directed component. Arrival at Earth is expected around 12:00 UTC on May...... Read more

G2 - Moderate geomagnetic storms expected
Geomagnetic storms reaching G2 - Moderate levels are expected over the next 48 hours due to the influence of a geoeffective coronal hole in combination with an Earth-directed component of coronal mass ejection (CME) produced on May 13. The first effects are expected...... Read more

G2 - Moderate geomagnetic storm, aurora seen as far south as Colorado
A potent coronal hole has become geoeffective and possibly in a combination with an April 18 CME is causing geomagnetic storms reaching G2 levels. This is the second of two geoeffective coronal holes to affect Earth this week. The effects are expected to persist...... Read more

G2 - Moderate geomagnetic storm level reached
A G2 - Moderate geomagnetic storm conditions were reached at 04:33 UTC on April 20, 2017. This activity is a result of continued coronal hole effects, the first of two expected to affect our planet this week. The geomagnetic field reached G1 - Minor levels during...... Read more

Geomagnetic storms reaching G1 level expected
Earth is under the influence of a recurrent, positive polarity coronal hole high speed stream (CH HSS). A G1 - Minor geomagnetic storm began at 05:59 UTC today. Solar wind parameters, as measured by the DSCOVR spacecraft, continued at mostly nominal levels over the...... Read more

Filament eruption, glancing blow possible on April 15
An approximate 14 degree solar filament eruption began at 20:25 UTC on April 9, 2017, from the northeast quadrant of the Sun. The event generated a coronal mass ejection (CME) and a glancing blow is possible on April 15. The CME was first observed in SOHO/LASCO C2...... Read more

G1 - Minor geomagnetic storm in progress
A G1 - Minor geomagnetic storm is in progress as of 08:14 UTC on April 4, 2017, due to Earth's proximity to the heliospheric current sheet (HCS) and weak influences of the southern polar, negative coronal hole high speed stream (CH HSS). Geomagnetic K-index of 5...... Read more

Moderately strong M5.8 solar flare erupts from Region 2644
A moderately strong solar flare measuring M5.8 (R2 - Moderate) erupted from Region 2644 at 14:29 UTC on April 3, 2017. The event started at 14:19 and ended at 14:34 UTC. This is the 7th and the strongest M-class solar flare since late April 1, 2017. It is also the...... Read more

Seven M-class solar flares erupt from Region 2644
Departing Active Region 2644 erupted with seven M-class solar flares since late April 1, 2017. The series started with M4.4 on April 1 and was followed by M5.3, M2.3, M2.1 and M5.7 on April 2, and M1.2 and M5.8 on April 3. Multiple coronal mass ejections were...... Read more

Geomagnetic storms begin as potent coronal hole becomes geoeffective
A recurrent, negative-polarity coronal hole is affecting our planet, causing geomagnetic storming. A G2 - Moderate geomagnetic storm watch is in effect for March 28 and 29. A high speed solar wind stream produced by a recurrent, negative-polarity (potent) coronal...... Read more

CH HSS sparks geomagnetic storming, G2 warning issued
Earth is under the influence of a positive polarity coronal hole high speed stream (CH HSS) which is causing geomagnetic storming. G1 - Minor geomagnetic storm threshold was first reached at 16:12 UTC on March 21, 2017. A G2 - Moderate geomagnetic storm warning was...... Read more

Earth under the influence of polar-connected CH HSS
A negative polarity, polar-connected coronal hole high speed stream (CH HSS) is affecting Earth for the second day in a row, sparking geomagnetic storms reaching G2 Moderate levels. Over the past 24 hours, the solar wind environment was elevated due to the passage...... Read more

Negative polarity CH HSS sparks G1 geomagnetic storm
Earth is under the influence of a recurrent, polar-connected coronal hole which has sparked G1 (Minor) geomagnetic storming today. Unsettled to active conditions, with G1 storming likely, are expected to continue through March 2. Geomagnetic K-index of 5 (G1 - Minor...... Read more

CH HSS sparks geomagnetic storm reaching G1 levels
Our planet is under the influence of a recurrent, positive polarity coronal hole high speed stream since around 20:48 UTC on February 23. This is causing G1 geomagnetic storming. Geomagnetic K-index of 5 (G1 - Minor geomagnetic storm) threshold was first reached at...... Read more

G1 geomagnetic storm in progress
A recurrent, negative polarity coronal hole high-speed stream (CH HSS) is affecting our planet causing isolated periods of G1 Minor geomagnetic storming and vivid auroras. High-speed solar wind speed hit Earth late January 31, 2017. Geomagnetic K-index of 5 (G1 -...... Read more