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### What is the problem this feature will solve?
With the newly supported `require(esm)` we have the ability to require ES modules into CommonJS contexts.
One thing that might be useful is that …
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Hi Korbinian,
Moving the dialog here....the clear SWI portion of things is all resolved. I've moved the newer ROMEO & Laplacian unwrapping stuff here, so you can close the SWI part at your leisure.…
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Just a general query Eric,
can we use gmtsar for PS analysis rather than SBAS technique.
If yes then how??
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e.g., the wrapped phase, phase offset, blurred ready image. not using the hud, which is buggy.
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The reconstruction process of an off-axis hologram could be divided into following steps.
1. Find the location of the first order terms, and apply spatial filtering method.
2. Shift the frequency cen…
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The [realtime_zshimming.m](https://github.com/shimming-toolbox/shimming-toolbox/blob/master/example/realtime_zshim.m) script uses a time series of B0 maps to compute the static and dynamic shim gradie…
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#
# This is an example configuration file for p2p_processing.csh
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# all the comments or explanation…
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attached is a plot of LST binned closure spectra for all triads at
different times. the times are single 10s records every 250 seconds around
fornax transit (empirically fornax transit looks to be a…
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The original implementation of FITACF3 produces a seemingly excessive amount of "grainy" echoes in low-power ground scatter (e.g. above range gate 50 in the velocity plot below):
![image](https://c…
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Which preprocessing steps would you suggest for the phase and magnitude data before using them for the ROMEO?