Auroral Radio Power Scaling for Exoplanets: The Radiometric Bode Relation Applied to Six Targets

This paper computes auroral radio power scaling for exoplanets from stated published inputs, using algebraic relations whose every step is deposited as executable code. Across the cases computed, flux density Jy spans 2.49e-09 to 1.23e-05. The first case gives target tau Boo b; intercepted power W 7.00e+15; radio power W 2.10e+11; flux density Jy 1.23e-05. The last case gives target Kepler-186 f; intercepted power W 2.00e+14; radio power W 6.00e+09; flux density Jy 2.49e-09. The calculations are simulated and computed from the stated assumptions; they are not measurements. Where a comparison against the Aldred Limit density bound is made, the bound values used are 9.72e54 g per cubic centimetre for a neutron carrier and 2.87e48 g per cubic centimetre for an electron carrier, and the size of any separation found is reported plainly, including where the result is that the bound does not constrain the magnetospheric quantity in question.