Observing in "Fast" Mode: Difference between revisions
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===Hittite LO Command File=== | ===Hittite LO Command File=== | ||
The first requirement of the system is the local oscillator (LO) tuning itself, which is performed by a Hittite 40 GHz signal generator. An example control file is shown below: | The first requirement of the system is the local oscillator (LO) tuning itself, which is performed by a Hittite 40 GHz signal generator. An example control file (called an FSEQ file, a text file with extention .fsq) is shown below: | ||
:LIST:DWELL<br> | :LIST:DWELL<br> | ||
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:LIST:SEQUENCE 1, 2, 5, 6, 9, 13, 19, 20, 26, 37, 51<br> | :LIST:SEQUENCE 1, 2, 5, 6, 9, 13, 19, 20, 26, 37, 51<br> | ||
The first command LIST:DWELL gives a list of 52 durations, one for each of our possible tuning bands | The first command, LIST:DWELL, gives a list of 52 durations, one for each of our possible tuning bands. Most bands have a duration of 19.75 ms, slightly less than the target 20 ms in order to account for some overhead in tuning. Note that the 20th band has a duration of 0.8 s (I have highlighted it in bold). In the actual file, the LIST:DWELL command is on a single line, but here I have broken it into lines of 10 numbers each for clarity. The second command, LIST:SEQUENCE, specifies the bands to be used in the sequence, here a roughly logarithmically spaced set of bands over the whole range, but with band 20 (the dwell band) inserted. Note that the sum of durations for these 11 bands must add to 1 s (or slightly less due to the overhead). |
Revision as of 11:31, 13 May 2023
Fast Mode Observing Setup
Purpose
The normal operating mode of EOVSA is to tune across the entire 1-18 GHz band (50 tunings) each second, which means taking data in a given frequency band for 20 ms (actually 19 ms after 1 ms of settling time) per second. Some solar phenomena, especially coherent emission, varies on a much shorter timescale, making it of interest to have an observing mode that repeats a given frequency with higher time resolution. Luckily, the frequency-agile nature of EOVSA allows this.
Implementation
We have implemented a mode that we call "Fast Mode" where the system dwells on one or more bands for a larger fraction of a second and records data at a higher rate during that dwell time. This is subject to the system requirement of a 1-s repetition rate, but is otherwise quite unrestricted. For example, it is possible to sit on one band for 0.8 s and then tune to 10 other bands at a 0.02 s rate to finish out the 1-s cycle, with this cycle repeating every second. Many other combinations are possible.
Hittite LO Command File
The first requirement of the system is the local oscillator (LO) tuning itself, which is performed by a Hittite 40 GHz signal generator. An example control file (called an FSEQ file, a text file with extention .fsq) is shown below:
- LIST:DWELL
- 0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,
- 0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.8,
- 0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,
- 0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,
- 0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,0.01975,
- 0.01975,0.01975
- LIST:SEQUENCE 1, 2, 5, 6, 9, 13, 19, 20, 26, 37, 51
The first command, LIST:DWELL, gives a list of 52 durations, one for each of our possible tuning bands. Most bands have a duration of 19.75 ms, slightly less than the target 20 ms in order to account for some overhead in tuning. Note that the 20th band has a duration of 0.8 s (I have highlighted it in bold). In the actual file, the LIST:DWELL command is on a single line, but here I have broken it into lines of 10 numbers each for clarity. The second command, LIST:SEQUENCE, specifies the bands to be used in the sequence, here a roughly logarithmically spaced set of bands over the whole range, but with band 20 (the dwell band) inserted. Note that the sum of durations for these 11 bands must add to 1 s (or slightly less due to the overhead).