In 1985 it dawned on us that the effect would be most noticeable in LF,
where it would permit "flip-flop" relaxation of the muon and the Cu
in a regime where the muon spin was otherwise strongly decoupled
from local fields, and therefore static.
So the experiment was repeated in LF; this time it worked.
Click on the run-number button for run 5687 and investigate the run header information, especially the names and ordering of the data histograms. Select various Spectrum types and look at the entire time range with (let us say) 300 ns bins. Eventually choose Spectrum type 2, Histograms 1,2 to plot some nice ASY spectra for that series of runs at 20 K.
When you have these runs selected, click Zip & Download Runs at the bottom of the Run List window to bring the selected runs into your computer; then unzip the download into the directory where you want to fit them.
If you are working on bnqrexp.triumf.ca, the zip/unzip step is not required, as all runs are directly accessible in the /data/<beamline>/<year>/ directories on that host; unfortunately this is not available on the workstations in Hennings.
Use musrgui
or (on bnqrexp.triumf.ca) physica ['t0', 'bkgd' and 'early' commands]
to verify the correctness of the t = 0 bin, background bin range and good data bin range.
Checking one run should be sufficient.
Notice that there are additional histograms with no counts; these can be ignored.
Prepare your fit-control template file, for either musrfit (.msr)
or msrfit (.i),
starting from another such file.
Fit to a single stretched-exponential relaxing signal in each case.
You can construct a global fit with common values of
the initial asymmetry and the ALPHA parameter
if you like, but this is not essential.
Should you choose to try global fits, here are some templates
for use with msrfit:
cu_zlf_45k-GKT.IGL and
cu_zlf_45k.IGL; both of these
cover only the ZF to low LF region (well below the qALCR) and so
address only the question of the muon hop rate at 45 K.
They will not show you the resonance at higher LF.
They use two different tables to look up the
dynamic Gzz(t)
corresponding to the fitting model.
If you are keen to "do it right", you can make a global fit of the series of runs taken under Experiment 336 in 1985 on Cu with <110> || B at 45 K (where the muon is most static in the Cu lattice) to a "dynamicized" version of Celio's theoretical Gzz(t) using the table td_cu_110_lf.tbl which Jess will show you where to find.
If you do it this way, you will find it difficult to plot your fit results in a manner that looks like a resonance. Why?