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  1. Rayleigh: An Open-Source, Pseudo-Spectral MHD Code for O(10^5) cores...and beyond

    28 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh: An Open-Source, Pseudo-Spectral MHD Code for O(10^5) cores...and beyond. February 5-6, 2015. Nick Featherstone. 

  2. Rayleigh Tutorial Module 7: Custom Diagnostics

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 7: Custom Diagnostics. June 19-20, 2016. Nick Featherstone. 

  3. Rayleigh Tutorial Module 6: Plotting Output

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial 6: Plotting Output. June 19-20, 2016. Nick Featherstone. 

  4. Rayleigh Tutorial Module 5: Diagnostic Outputs

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 5: Diagnostic Outputs. June 19-20, 2019. Nick Featherstone. 

  5. Rayleigh Tutorial Module 4: Ensemble Mode

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 4: Ensemble Mode. June 19-20, 2016. Nick Featherstone. 

  6. Rayleigh Tutorial Module 3: Controlling Physics in Rayleigh

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 3: Controlling Physics in Rayleigh. June 19-20, 2016. Nick Featherstone. 

  7. Rayleigh Tutorial Module 2: Running the Code & Best Practices

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 2: Running the Code & Best Practices. June 19-20, 2016. Nick Featherstone. 

  8. Rayleigh Tutorial Module 1: Building and Porting the Code

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Module 1: Building and Porting the Code. June 19-20, 2016. Nick Featherstone. 

  9. Rayleigh Tutorial Overview

    26 Mar 2021 | Contributor(s):: Nick Featherstone

    Rayleigh Tutorial Overview. June 19-20, 2016. Nick Featherstone. 

  10. May 16 2013

    2013 Stellar Scalable Pseudospectral Methods and the Geodynamo

    Nick Featherstone, Ph.D. CU BoulderThis webinar will begin with a brief overview of recent efforts to model convection and dynamos in the Sun and other stars. Such models (massive stars in...

    https://geodynamics.org/events/details/155