An implementation of the deflection angle in the equitorial plane as a function of the black hole mass, spin, and asymptotic impact parameters, as detailed in Iyer and Hansen (2009).
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Updated
Jul 19, 2023 - Julia
An implementation of the deflection angle in the equitorial plane as a function of the black hole mass, spin, and asymptotic impact parameters, as detailed in Iyer and Hansen (2009).
Semi-analytic frequency- and time-domain CSEM/TEM fields of wires, dipoles and loops over a layered earth with a Gaussian hill or depression and a conductive sphere. Validated against empymod and elfe3D.
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