Saturday 19th of August 2017
Wolverhampton Amateur Radio Society
Founded in 1922 | Call sign G8TA

Wolverhampton ARS Logo

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

RSGB Affiliated

RSGB Logo

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]

Social Networking

Google+

YouTube

Solar Data

Space Weather Feed[+]

CH HSS sparks isolated periods of G1 geomagnetic storming
Our planet is under the influence of a coronal hole high speed stream (CH HSS) which is causing isolated periods of G1 - Minor geomagnetic storming over the past 2 days, August 17 and 18, 2017. Meanwhile, solar activity is very low. There is only one numbered active...... Read more

Major solar flare erupts near the eastern limb, no Earth-directed CMEs
A pair of solar flares erupted near the eastern limb of the Sun at about 00:55 and 03:25 UTC on July 23, 2017 and were observed in STEREO-A EUVI 195 imagery. The source is Active Region 2665 which produced a long-duration M2.4 solar flare and Earth-directed CME on...... Read more

Positive polarity CH HSS sparks G1 geomagnetic storm
A positive polarity coronal hole high speed stream (CH HSS) is affecting our planet and will continue to do so over the next three days. Over the past 24 hours, by 12:30 UTC on July 22, solar wind parameters as measured by DSCOVR spacecraft reflected the influence...... Read more

CME hits Earth, sparks G2 - Moderate geomagnetic storm
A coronal mass ejection (CME) produced by the July 14th M2.4 long-duration solar flare hit Earth's magnetic field at 06:01 UTC on July 16, 2017. G2 - Moderate geomagnetic storming started 9 hours later. The S1 Minor solar radiation storm that started at 09:00...... Read more

Long-duration M2.4 solar flare erupts, Earth-directed CME
Active Region 2665 produced a long-duration solar flare measuring M2.4 at its peak time on July 14, 2017. Today's event lasted for more than 2 hours; it started at 01:07, peaked at 02:09 and ended at 03:24 UTC. The eruption produced a coronal mass ejection (CME)...... Read more

CH HSS sparks geomagnetic storms reaching G1 levels
Our planet is under the influence of a positive polarity CH HSS which is causing geomagnetic storms reaching G1 - Minor levels. During the past 24 hours, solar wind parameters reflected the onset of a co-rotating interactive region (CIR) followed by the influence of...... Read more

Impulsive M1.3 solar flare erupts from big Region 2665
Big sunspot region 2665 (beta) erupted with an impulsive solar flare measuring M1.3 at its peak time on July 9, 2017. The event started at 03:09, peaked at 03:18 and ended at 03:37 UTC. The last time our star unleashed an M-class solar flare was on July 4, 2017....... Read more

Impulsive M1.3 solar flare erupts near the west limb
Solar activity was at moderate levels on July 3, 2017, with 14 B-class and one impulsive M1.3 solar flare observed at 16:15 UTC. The M-class event started at 15:37 and ended at 16:18 UTC. The last time our star unleashed an M-class solar flare was on April 3, 2017....... Read more

Partial-halo CME impact sparks G1 geomagnetic storm
A partial-halo coronal mass ejection (CME) produced on June 28, 2017 hit Earth's magnetic field at 17:12 UTC on July 1, almost 24 hours earlier than expected. The impact was weak but managed to spark a G1 - Minor geomagnetic storm 17 hours later. G1 Watch...... Read more

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