Gravitational acceleration depends on height as
"\\displaystyle g_h = g_0 (\\frac{R_e}{R_e+h})^2" ,
where "g_h" is gravitational acceleration at a certain height, "g_0 = 9.80665" m/s2 is standard gravitational acceleration, "R_e" is the Earth's radius, "h" is height.
As we see from the formula, gravitational acceleration decreases with height.
So when "h=0" m, that means that you're at the Earth ocean-level surface, then "g_h = g_0". In mountains "g_h" will be just a bit smaller, the difference is less than 1 %. Only going to the height of ionosphere and low orbit satellites ("h \\leq 2000" km) will make you feel a big difference.
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