Software Telescope
An anonymous reader writes "The BBC News is running the story 'Pyramid power' probes universe which is about LOFAR's software telescope for radio astronomy. The heart of the system is a IBM Blue Gene which processes data from an array of simple pyramidal radio antennae. The array of antennae are also multitasking in the fields of geophysics and agriculture."
When Lofar Meets Stella
350 KM Diameter Radio Telescope Array
I was talking to a professor in astronomy here and he mentioned about some of the conflicts between US and Europe regarding the plan. That is one of the reasons why US is also working on Square Kilometer Array. LOFAR imaging telescope are designed for the 10-240 MHz frequency range where as SKA will cover 0.15-20GHz or higher. Hopefully the two efforts will complement each other.
The bandwidth of the connection between each Remote Stations and the Central Processing Systems will be ~10 Gbit/s, of which ~ 2.5 Gbit/s will be occupied by the sustained datarate resulting from the sensors.
LOFAR produces very large data streams, especially for the astronomy application (e.g. 6 TB of raw visibility data for an 8 beam, 4 hour synthesis observation, after integration for 1 sec and over 10kHz).
They mention that final post-processing can be done at a central processing station (I am guessing the Blue Gene one) or locally by the users. Only bottlenecks seems to be the bandwidth.
LOFAR post-processing can take place either at the Central Processor or locally with the users (in particular at Science Centers). If the available Internet capacity is sufficient, intermediate dataproducts can be transported to the user, and local processing can be done. Otherwise processing resources at the Central Processor are available for further data reduction (within the limits of the Central Processor processing budget).
Of course, you would know this if you had RTFA before you posted...
The antennas are pyramid shaped because each of those pyramids actually contains two dipole antennas, to capture the EM field in two perpendicular polarisations. (I am involved in the project so trust me on this one ;-))