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These fluxes were scaled to Mars orbit.
These fluxes are scaled to Mars orbit at 1.5 AU.
These fluxes arise from ion-neutral reactions in the plasmasphere.
These fluxes are all columns or M[HS] k, n.
These fluxes were passed to FISPACT for the activation calculation.
Homogeneous streambed hydraulic conductivities were calibrated to reproduce these fluxes.
A theorem establishing the monotonicity of these fluxes is provided.
Due to these fluxes, the refractive index and the optical clarity of the medium are changed.
These fluxes were approximately equal during the first and second FTCs (Table 3).
Theoretical ionospheric model based on the closed geomagnetic tubes can self-consistently calculate these fluxes.
The advantages and disadvantages associated with these fluxes are discussed by [8].
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