The modification of surface radiative properties has been increasingly examined from the perspective of engineering thermophysics, particularly in relation to solar radiation management and its impact on surface energy balance. In this study, a methodological framework, referred to as the radiative forcing (RF)-meter, is introduced to quantify the RF variation induced by high-albedo surfaces under real environmental conditions. The proposed approach integrates ground-based irradiance measurements, astronomical calculations, and satellite observations to reconstruct the time-dependent radiative flux associated with albedo changes. Based on this formulation, the reduction in absorbed solar energy is evaluated and further interpreted in terms of equivalent energy impact, providing a consistent basis for linking radiative effects with thermophysical processes. The framework also allows the cumulative effect of RF reduction to be expressed in CO$_2$-equivalent terms, enabling a quantitative interpretation of long-term environmental and energy-related implications. Potential applications of the method are discussed with reference to high-irradiance regions, where surface reflectivity modification may contribute to both thermal regulation and energy demand reduction. The proposed methodology offers a structured approach for analysing surface energy behaviour within the context of engineering thermophysics, with possible extensions toward building energy efficiency and solar radiation control strategies.
The magnetohydrodynamic flow of a Jeffrey fluid in a vertical channel was numerically investigated, with particular emphasis on the coupled effects of nonlinear thermal radiation, internal heat generation, variable viscosity, chemical reaction, and buoyancy forces. The governing partial differential equations describing momentum, heat, and mass transport were transformed into a system of ordinary differential equations through appropriate similarity transformations and the introduction of a stream function formulation. The resulting boundary value problem was solved numerically using the MATLAB bvp4c solver. The results show that the fluid velocity was significantly reduced with increasing magnetic field strength due to the enhancement of Lorentz forces, while the temperature distribution was elevated as a consequence of Joule heating. Nonlinear thermal radiation was found to substantially intensify the thermal field. Furthermore, an increase in the viscosity variation parameter and Jeffrey fluid parameters led to a suppression of both momentum and thermal boundary layers. In contrast, buoyancy forces were shown to accelerate the flow and enhance heat transfer. The influence of mass transfer was also critically examined, where an increase in the Schmidt number (Sc) and chemical reaction parameter resulted in a marked reduction in species concentration, thereby weakening mass diffusion. The interplay among these thermo-physical parameters demonstrated a complex but physically consistent behavior across momentum, heat, and mass transfer processes. These findings provide deeper insight into the control of transport phenomena in non-Newtonian magnetohydrodynamic flows and are expected to have practical relevance in thermal engineering systems, polymer processing, and energy-related applications involving radiative heat transfer and chemically reactive flows.