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Getting started

  • Installation

Instruments

  • Amor
    • Data reduction for Amor
    • Reference
      • ess.amor.beamline
        • ess.amor.beamline.instrument_view_components
        • ess.amor.beamline.make_beamline
      • ess.amor.conversions
        • ess.amor.conversions.incident_beam
        • ess.amor.conversions.specular_reflection
      • ess.amor.tools
        • ess.amor.tools.linlogspace
      • ess.amor.instrument_view.instrument_view
      • ess.amor.load.load

Techniques

  • Reflectometry
    • Reference
      • ess.reflectometry.conversions.specular_reflection
      • ess.reflectometry.corrections.illumination_correction
      • ess.reflectometry.corrections.illumination_of_sample
      • ess.reflectometry.resolution.detector_resolution
      • ess.reflectometry.resolution.z_offset
  • Wavelength frame multiplication
    • Introduction to Wavelength Frame Multiplication
    • Reducing WFM data

About

  • Release Notes
Theme by the Executable Book Project

Wavelength frame multiplication

Wavelength frame multiplication¶

  • Introduction to Wavelength Frame Multiplication
    • The long ESS pulse
    • So what is WFM anyway?
    • A closer look
      • The ESS pulse shape
      • Using a single WFM chopper
      • Using a pair of optically blind choppers
    • A short example
      • Create a beamline
      • Create some neutrons
      • Wrap the neutron counts and the beamline into a DataArray
      • Stitch the frames
  • Reducing WFM data
    • Create beamline components
    • Generate some fake data
    • Visualize the beamline’s chopper cascade
    • Discard neutrons that do not make it through the chopper windows
    • Create a realistic Dataset
    • Stitch the frames
    • Convert to wavelength
    • Normalization
    • Comparing to the raw wavelengths
    • Without WFM choppers
    • Working in event mode

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ess.reflectometry.resolution.z_offset

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Introduction to Wavelength Frame Multiplication

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