Skip to content

Commit

Permalink
Drop mirror scan step by half
Browse files Browse the repository at this point in the history
Co-authored-by: Talon Chandler <[email protected]>
  • Loading branch information
ieivanov and talonchandler authored Jul 27, 2023
1 parent bacf677 commit 2fb72b9
Showing 1 changed file with 10 additions and 7 deletions.
17 changes: 10 additions & 7 deletions mantis/acquisition/settings/example_acquisition_settings.yaml
Original file line number Diff line number Diff line change
Expand Up @@ -32,13 +32,16 @@ lf_slice_settings:
z_stage_name: 'MCL Piezo'
z_start: -10
z_end: 10
# When using 0.52 NA transmission light illumination, Nyquist sampling of this
# dimension will be achieved by using 300 nm in sample space or by using 420
# nm steps of the mirror due to the 1.4x magnification of the remote volume.
# Here we chose to oversample the data to match the light-sheet axial
# sampling. The 285 nm mirror steps correspond to ~205 nm axial sampling of
# the data, matching the light-sheet sampling after deskew and 3x binning.
z_step: 0.285
# When using 0.52 NA transmission light illumination, Nyquist sampling of the
# axial dimension will be achieved by using (450*1.4)/(1.35^2 + 0.52^2) = 300 nm
# steps in sample space. We can achieve this by using (300 nm)*1.4/2 = 210 nm
# steps of the mirror due to the 1.4x magnification of the remote volume and the
# fact that the optical path length is extended by twice the mirror's motion.
#
# Here we choose to oversample the data to match the light-sheet axial
# sampling. After deskewing and 3x binning, the light-sheet samples are
# spaced by ~205 nm, so we choose (205 nm)*1.4/2 = 143 nm mirror steps.
z_step: 0.143
use_sequencing: True

# Define channel settings for the light-sheet acquisition. Channels may have
Expand Down

0 comments on commit 2fb72b9

Please sign in to comment.