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Queuing an Observation Schedule
Working in the scheduling directory is strongly discouraged. It will very likely lead to frustration and spam for any other users on the ilofar account. It is advised to prepare schedules on your local machine or in the temp folder. Once you have used the pre...
Interrupting Scheduled Observations
The interruptObs.sh script operates in one of two modes: focused and global. In focused mode, it will take an input schedule, determine the relevant launched instances for that schedule, and specifically shut down all related screens, tmuxes and processes. In ...
Processing Pulsar Data
CDMT (Stokes I) Method The GPUs in ucc4 are typically used to reduce the majority of the pulsar data produced by the station into mode 5, 8x channelised, 16x downsampled Sigproc Stokes I filterbanks. This is achieved through using a python3 script, cdmtProc.p...
Processing Solar Data (Basic)
UPM Method Solar data is typically processed using udpPacketManager, to produce a Stokes IV output, downsampled by a factor of 256 to 1.3ms, using a set of automated scripts. The process_data.sh script can be set to process any subdirectories with data on a ...
Processing Other Data (EMPTY)
UPM Method
Bash Aliases
LGC $ # Access the LCU while in local mode $ lcu $ # Access the Recording node (ucc1) $ ucc1 $ # Access the scheduling directory $ sched $ # Test a schedule file $ testsched my_input_file.txt UCC1 $ # Access recording drive 1 (old) $ cdr ...