[HN Gopher] Cosmic: SETI Institute Is Unlocking the Mysteries of...
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Cosmic: SETI Institute Is Unlocking the Mysteries of the Universe
Author : ulrischa
Score : 39 points
Date : 2024-01-14 16:06 UTC (6 hours ago)
(HTM) web link (www.seti.org)
(TXT) w3m dump (www.seti.org)
| menthe wrote:
| More technical article about the new deployment:
| https://science.nrao.edu/facilities/vla/observing/cosmic-set...
|
| So glad to see SETI alive. Next step, building a proof-of-work
| token to bring back SETI@Home and leverage thousands more GPUs
| :']
| agucova wrote:
| From the article: The COSMIC system is a
| cluster of FPGA, CPU, and GPU hardware, which at all times
| receives a copy of digitized data streams from each of the
| VLA's antennas. The data received by COSMIC necessarily
| reflects antenna-pointing, LO-tuning and digitization settings
| commanded by VLA observers, but otherwise operates completely
| independently. In particular, COSMIC is unaffected by any of
| the interferometric phasing, channelization, or correlation
| processes of the VLA's facility instrument: WIDAR.
| COSMIC comprises three main components: A fiber
| optic splitter, which duplicates digitized data streams from
| the VLA antennas and delivers these to COSMIC digital
| instrumentation. A small FPGA Cluster, which receives
| VLA antenna digitized data streams, channelizes these to 1 MHz
| frequency resolution, and transmits these data streams over
| multiple industry-standard 100 Gb/s Ethernet links. A
| CPU/GPU Cluster which receives 1 MHz resolution data over
| Ethernet and performs a variety of digital signal processing
| operations, ultimately outputting SETI signals of interest
| (often referred to as "hits") into a database for further
| analysis.
|
| And the CPU/GPU cluster in particular is extremely interesting:
| The COSMIC CPU/GPU pipeline implements a beamformer, high-
| resolution channelizer, doppler-drift search, and calibration
| correlator. The configuration parameters of these algorithms
| may be varied in order to best leverage the array's behaviour
| as dictated by the Primary Observer. The COSMIC
| CPU/GPU processing pipeline is still under development, but
| will have the following capabilities: Buffering
| of ~ 5 minutes voltage data for all antennas in the VLA;
| Beamforming of up to 32 coherent tied-array beams;
| Incoherent beamforming; Configurable frequency
| resolution between 1 MHz and 1 Hz; Inter-antenna
| correlation (used for gain calibration observations) with
| millisecond time resolution; and Doppler drift
| searching for narrow band signals (in antenna or beam data)
| with linear drift rates between -50 Hz/s and +50 Hz/s.
| In normal operation, the COSMIC system will search for
| candidate signals with non-zero linear drift rates, and will
| permanently archive small data snippets (< 100 kHz bandwidth
| and < 5 minutes duration) around these events.
|
| This is really cool!
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(page generated 2024-01-14 23:00 UTC)