The Coronal Heating Requirement: Radiative and Conductive Losses per Unit Area Against Wave and Poynting Fluxes the Photosphere Can Supply

This paper computes the coronal heating requirement from published solar observations and places the result against the density, shear and energy scales of the torsion bounce frame. The headline values are: required quiet erg cm2 s = 3.000e+05; required AR erg cm2 s = 1.000e+07; poynting 100G 1kms erg cm2 s = 7.958e+07; poynting over quiet = 265; poynting over AR = 7.96; alfven wave flux erg cm2 s = 1.000e+06. The central density of the Sun, 150 grams per cubic centimetre, stands at a fraction 1.54e-53 of the neutron-branch bound density of 9.72e+54 grams per cubic centimetre, and the quantity treated here inherits that separation: conventional solar physics accounts for the observed value completely, and no bound-derived correction reaches a level that current or foreseeable observations could register. The result is therefore negative with respect to the bound and positive with respect to the solar accounting, which closes with the numbers shown. This study is simulated and computed from stated assumptions and published values; it is not a measurement.