From a863e7fc05feb892ffbb7957b4fe74a886992800 Mon Sep 17 00:00:00 2001 From: Thomas White Date: Fri, 12 Jan 2024 14:05:28 +0100 Subject: Update docs about --max-mille-level. --- doc/man/align_detector.1.md | 4 ++++ doc/man/indexamajig.1.md | 7 +++++++ 2 files changed, 11 insertions(+) diff --git a/doc/man/align_detector.1.md b/doc/man/align_detector.1.md index aa5f5061..f5991641 100644 --- a/doc/man/align_detector.1.md +++ b/doc/man/align_detector.1.md @@ -45,6 +45,10 @@ panel "dominoes", and level **3** would refine the individual (roughly square) ASICs. Higher refinement levels will generally require more and higher-resolution diffraction data. +You can use **indexamajig** option **--max-mille-level** to reduce the size of +the calibration data files, at the cost of limiting the maximum refinement +level. + The default behaviour is to refine only the position components in the x-y plane, perpendicular to the beam. In favourable circumstances, you can add option **--out-of-plane** to refine the panel tilts and shifts out of this diff --git a/doc/man/indexamajig.1.md b/doc/man/indexamajig.1.md index 85566240..1955ef76 100644 --- a/doc/man/indexamajig.1.md +++ b/doc/man/indexamajig.1.md @@ -594,6 +594,13 @@ INDEXING OPTIONS **--mille-dir=dirname** : Write the Millepede-II data into _dirname_. +**--max-mille-level=n** +: Write the Millepede-II data up to a maximum hierarchy depth _n_. If _n_ is +: 0, only the overall detector position can be refined. Larger numbers allow +: finer-grained refinement. Set this to a large number (9 is high enough!) +: to disable the limit, although this can make the Millepede-II files quite +: large. + **--wavelength-estimate=m** **--camera-length-estimate=m** : Some indexing algorithms need to know the camera length or the wavelength of : the incident radiation in advance, e.g. to prepare an internal look-up table. -- cgit v1.2.3