Designing control software and graphical user interfaces for vi sp mechanisms
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The document outlines the design and development of control software and graphical user interfaces for the Visible Spectro-Polarimeter (ViSP) used in solar physics research. It highlights the need for robust software to operate various mechanisms and subsystems within the instrument, detailing the functionality of components like the slit and grating stations. The ViSP will provide precise measurements for solar observations, contributing to improved understanding of solar dynamics and space weather predictions.
Designing control software and graphical user interfaces for vi sp mechanisms
- 1. July 8, 2015 Designing Control Software and Graphical User Interfaces for ViSP Mechanisms Alan Sánchez University of Colorado Boulder - Aerospace Engineering Sciences High Altitude Observatory - Instrumentation Group
- 2. 2 New instrumental capabilities are needed to meet the challenge of validating sophisticated models and theories in the field of solar physics A coronal mass ejection (CME) in a model; the CME is the gray cloud toward the lower right. Credit: Dusan Odstrcil, George Mason University This Center for Integrated Space Weather Modeling display is used to predict space weather. Credit: NOAA
- 3. The Daniel K. Inouye Solar Telescope is set for completion in 2019. It will have broad impacts on astronomy, plasma physics, and solar- terrestrial relations http://dkist.nso.edu/node/2220 3 http://dkist.nso.edu/node/2764
- 4. 4 http://dkist.nso.edu/node/2739 A total of five science instruments receive light from the First Light Coudé Beamsplitter, including the Visible Spectro-Polarimeter (ViSP)
- 5. The ViSP will provide precise measurements of all four Stokes parameters (I, Q, U, & V) at wavelengths from 380-900 nm 5 The wavelength range of optical radiation, with ViSP capabilities labeled. Credit: http://light-measurement.com/wavelength-range/
- 6. All four ViSP-unique mechanisms require robust software to run properly 6
- 7. ViSP mechanisms can be activated either through the Instrument GUI or the Engineering GUI 7 5263-TN-6003 5263-TN-6003. Courtesy of A. Lecinski, P. Oakley, and R. Casini
- 8. ViSP distributes tasks to several managers that then delegate tasks to the workers they control. 8 5263-TN-6003. Courtesy of A. Lecinski, P. Oakley, and R. Casini
- 9. ViSP Main Engineering GUI provides monitoring and control capabilities for every subsystem in the instrument. 5263-TN-6003. Courtesy of A. Lecinski, P. Oakley, and R. Casini 9
- 10. 10 Slit Station Very narrow entrance slit to be placed in the ViSP optical beam; slit is then physically moved laterally over the image plane in order to capture the desired field of view. Grating Station Used to hold and position the diffraction grating in the optical path of the ViSP instrument Optical Design Overview illustrating mechanical requirements of slit and grating stations ViSP Critical Science Plan. Courtesy of R. Casini
- 11. Slit Station Top Level Components Slit Substation, FM Substation, and Slit Stage Selector move simultaneously ● Slit Substation moves the same distance as the desired slit aperture, while the FM substation moves half this distance Desired slit aperture is selected and slit selection stage moves desired slit in front of a mask. This mask blocks all light from non-active slits, while allowing light through the active slit to pass. Slit Selection Stage Slit and Fold Mirror (FM) Substations 5263-TN-4031. Courtesy of R. Summers, F. Lawson, and G. Card5263-TN-4031. Courtesy of R. Summers, F. Lawson, and G. Card 11
- 12. ViSP Slit Station GUI ● Identifies limit switch status via EtherCAT I/O connection ○ Notifies user if limit switch is triggered, stops all movement ● Delegates movement to SlitSelect if current slit width is not desired slit width ● Delegates movement to SlitTransit and MirrorTransit, respectively, if current slit and FM substation positions are not required slit and FM substation positions (for desired slit width) Slit Manager SlitSelect SlitTransit MirrorTransit ❏ Moves desired slit in front of mask ❏ Moves slit substation to required position ❏ Moves FM substation to required position 12
- 13. Slit Station simulated with two motors via Delta Tau PPMAC and Beckhoff I/O connections on EtherCAT 13
- 14. 5263-TN-202000. Courtesy of R. Summers, F. Lawson, and G. Card 5263-TN-202000. Courtesy of R. Summers, F. Lawson, and G. Card Essential functions of Grating Station: Verify current diffraction grating ‘ID’ Position and hold the diffraction grating in the optical path of the ViSP Grating Station Top Level Components 14
- 15. ViSP Grating Station GUI ● Identifies grating via EtherCAT I/O connection ○ Notifies user if grating is not in place, stops all movement ● Identifies limit switch status via EtherCAT I/O connection ○ Notifies user if limit switch is triggered, stops all movement ● Delegates movement to GratingRotate if expected grating is present and current angle is not desired angle Grating Manager GratingRotate ❏ Rotates to desired angle 15
- 16. We completed several fundamental, overarching goals of the HAO Prototyping Plan, and also made significant progress in specific mechanism software ● Test Setup and Robustness of Copley Amplifiers on EtherCAT ○ Network has been scheduled and is up and running ○ Controlling 2 Axes on EtherCAT ● Test Setup and Robustness of Beckhoff I/O on EtherCAT ● Test switch communications from Copley to Delta Tau ✓ ✓ ✓ HAO Prototyping Plan (2014), A. Lecinski and B. Larson Next steps: ● Finalize Slit Station software ○ step size, number of steps, intensity mode ● Focus Station software 16
- 17. Acknowledgments ● Partner: Anthony Anglin ● Mentors: Alice Lecinski and Brandon Larson ● Support: Scott Sewell and Val Sloan ● Interns: Jamie Weiss and Isis Peguero ● JES: DKIST software team 17