Unclassified - Boulder, CO
posted 7 months ago
As a Research Scientist specializing in Stellar Magnetism, you will play a pivotal role in advancing our understanding of the solar dynamo through numerical modeling and theoretical investigations. Your primary focus will be on magnetohydrodynamic convection, particularly the dynamics associated with angular momentum transport influenced by small-scale magnetism. This position requires a strong foundation in both theoretical and computational aspects of astrophysics, as you will be tasked with developing a theoretical framework to interpret the physical implications of newly discovered inertial waves in the solar photosphere. In this role, you will implement alternative-basis function representations within the Rayleigh convection code, which is essential for facilitating the use of sparse linear solvers. Your contributions will not only enhance our existing models but also pave the way for innovative approaches to studying stellar interiors. You will be expected to develop and grow an independent research program, seeking external funding to support your initiatives and expand the scope of your work. Your responsibilities will include conducting independent numerical experiments and theoretical investigations aimed at examining angular momentum transport and magnetic field generation within stellar interiors. You will also be responsible for presenting and disseminating your research findings to the broader scientific community, which will involve attending professional meetings and conferences, as well as submitting your work for publication in reputable scientific journals.