The solar constant is the amount of incoming solar electromagnetic radiation per unit area, measured on the outer surface of Earth's atmosphere in a plane perpendicular to the rays.
See link for formula
K = constant
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The Solar Constant refers to how much energy Earth gets from the Sun, per square meter (or another convenient unit of area). It is approximately 1.3-1.4 kW/m2 at the top of the atmosphere; the amount that reaches the surface is perhaps 2/3 of that value under ideal conditions - for example, no clouds.
Ml2t-1
1cal/cm2/min
its fairly constant,increasing only 0.2% at the peak of each 11 year solar cycle.
K = constant
No but if you replace a constant with a function it will remain a formula
No but if you replace a constant with a function it will remain a formula
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Acceleration with respect to time = a , where 'a' is a constant.
M. Alan Gibson has written: 'Solar constant (SOLCON) experiment' -- subject(s): Solar constant, Aerospace telemetry
The units for Rydberg's constant are [L-1].
There is no formula for Pi, it cannot be represented by any formula. It is a fundamental constant.
The solar constant of Mercury varies as the intensity of the sun changes. This rate of variation is greater than on earth. However, the mean solar constant for Mercury is 9130 W/m^2 or 9.13 kW/m^2.
If you have a constant speed, you are not accelerating.