Southwest Research Institute

As a recognized leader in space science research and spacecraft instrumentation, we are helping to reveal the secrets of our solar system and the universe.. Independently develop and implement numerical experiments and theoretical investigations designed to examine angular momentum transport and magnetic field generation in stellar interiors.. Requires a PhD in Physics, Astronomy, Astrophysics, Applied Mathematics, Applied Physics, Solar Physics or related degree field.. 2 years: Experience in Python programming and in the use of Python data analysis packages such as NumPy and Matplotlib.. 2 years: Experience in the application of computational fluid dynamics software (e.g., ASH, Rayleigh, Dedelus, Magic) to the study of stellar and planetary convection.

postdoctoral researcher

Who We Are: As a recognized leader in space science research and spacecraft instrumentation, we are helping to reveal the secrets of our solar system and the universe. We are looking for a postdoctoral researcher to join the Department of Solar and Heliospheric Physics who can collaborate with our team in ongoing studies of the solar dynamo.
Objectives of this Role: Conduct numerical modeling of stellar interior convection with a focus on those dynamics associated with small-scale magnetism.
Contribute to the development of a theoretical framework for understanding the physical implications of recently-discovered inertial waves in the solar photosphere.
Contribute to the continued development of open-source fluids software packages such as Rayleigh, Dedelus and Coral.
Develop and grow an independent research program through external program support
Participate in solar group proposals that support the strategic growth of the department.
Daily and Monthly Responsibilities: Independently develop and implement numerical experiments and theoretical investigations designed to examine angular momentum transport and magnetic field generation in stellar interiors.
Perform analysis and visualization of fluids simulation data.
Assess resulting trends in light of physical conditions expected inside stellar interiors.
Present and disseminate research results at professional meetings and conferences.
Submit manuscripts to peer-reviewed journals.
Contribute to weekly SWRI Solar group meetings and Boulder Convection Group meetings.
Actively seek and apply for external support of research activities.
Requirements: Requires a PhD in Physics, Astronomy, Astrophysics, Applied Mathematics, Applied Physics, Solar Physics or related degree field.
2 years: Post PhD experience in scientific software development using compiled languages such as FORTRAN and C/C++.
2 years: Experience in parallel programming using the MPI and OpenMP standards.
2 years: Experience in Python programming and in the use of Python data analysis packages such as NumPy and Matplotlib.
2 years: Experience in the application of computational fluid dynamics software (e.g., ASH, Rayleigh, Dedelus, Magic) to the study of stellar and planetary convection. #J-18808-Ljbffr

START NEW SEARCH