Yer tomonidan bo'sh vaqtning egriligi tufayli ufqdan ko'rish mumkin bo'lgan masofa quyidagi formula yordamida hisoblanadi: d = sqrt { (R_ {text {E}} + h) ^ 2 - R_ {text {E}} ^ 2} bu erda d ufqning hisoblangan masofasi; R_ {text {E}} Yerning radiusi (6,371,000 text {m}); va h kuzatuvchining balandligi. Hisoblangan masofasi sizning ko'zingizdan ufqgacha to'g'ri chiziqdir.
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