A type U burst was detected by CALLISTO at Rosse Solar Terrestial Observatory (RSTO) on the 11th of November 2010.
The plot shows the Height of the emitting plasma using the 4xNewkirk model.
The emitting region is Shown in the upper panel. The burst were generated by the NOAA 11126 active region.
Callisto measures radio emission from solar flares and coronal mass ejections in the range 45-870 MHz. We have been testing the system in Trinity College Dublin, before its move to a radio-quiet site in Birr Castle. There it will be used to study the effects of solar radio bursts on wireless communications, GPS and electrical power distribution. See www.rosseobservatory.ie for details and real time data.
Monday 21 February 2011
Motor Driver Maintenance
The motor driver that is used to track the Sun during the day, pointing CALLISTO antenna to the Sun, experienced some problems in the mechanics.
| The motor driver during the maintenaince |
The motor was successful bring back to Trinity College Dublin workshop were was repaired. Many thanks to Dave, TCD workshop Manager.
| Joe, Peter and Dave in the Mechanical workshop. |
On February the 18th 2011 the Motor Driver was seated back in Operation.
| Removing the motor driver from the mount. |
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