Total solar energy incident on unit area of horizontal surface on ground Calculator

✖The Direct Solar Radiation is the amount of solar energy received per unit area at a specific location, essential for understanding solar energy potential and environmental impact.ⓘ Direct Solar Radiation [G_D]			+10% -10%
✖The Angle of Incidence is the angle formed between an incoming ray of radiation and a line perpendicular to the surface it strikes.ⓘ Angle of Incidence [i]			+10% -10%

✖The Total Solar Energy is the total amount of solar radiation received by a surface, accounting for atmospheric effects and variations in solar intensity.ⓘ Total solar energy incident on unit area of horizontal surface on ground [G_solar]

⎘ Copy

👎

Formula

LaTeX

Reset

👍

Download Heat and Mass Transfer Formula PDF PDF Image

Total solar energy incident on unit area of horizontal surface on ground Solution

STEP 0: Pre-Calculation Summary

Formula Used

Total Solar Energy = Direct Solar Radiation*cos(Angle of Incidence)+Direct Solar Radiation
G_solar = G_D*cos(i)+G_D
This formula uses 1 Functions, 3 Variables

Functions Used

cos - Cosine of an angle is the ratio of the side adjacent to the angle to the hypotenuse of the triangle., cos(Angle)

Variables Used

Total Solar Energy - (Measured in Watt per Square Meter) - The Total Solar Energy is the total amount of solar radiation received by a surface, accounting for atmospheric effects and variations in solar intensity.
Direct Solar Radiation - (Measured in Watt per Square Meter) - The Direct Solar Radiation is the amount of solar energy received per unit area at a specific location, essential for understanding solar energy potential and environmental impact.
Angle of Incidence - (Measured in Radian) - The Angle of Incidence is the angle formed between an incoming ray of radiation and a line perpendicular to the surface it strikes.

STEP 1: Convert Input(s) to Base Unit

Direct Solar Radiation: 337.1644 Watt per Square Meter --> 337.1644 Watt per Square Meter No Conversion Required
Angle of Incidence: 40 Degree --> 0.698131700797601 Radian (Check conversion here)

STEP 2: Evaluate Formula

Substituting Input Values in Formula

G_solar = G_D*cos(i)+G_D --> 337.1644*cos(0.698131700797601)+337.1644

Evaluating ... ...

G_solar = 595.447315037573

STEP 3: Convert Result to Output's Unit

595.447315037573 Watt per Square Meter --> No Conversion Required

FINAL ANSWER

595.447315037573 ≈ 595.4473 Watt per Square Meter <-- Total Solar Energy

(Calculation completed in 00.005 seconds)

You are here -

Home » Physics » Heat and Mass Transfer » Radiation » Mechanical » Atmospheric and Solar Radiation » Total solar energy incident on unit area of horizontal surface on ground

Credits

Created by Sai Venkata Phanindra Chary Arendra

Vallurupalli Nageswara Rao Vignana Jyothi Institute of Engineering and Technology (VNRVJIET), Hyderabad

Sai Venkata Phanindra Chary Arendra has created this Calculator and 100+ more calculators!

Verified by Rajat Vishwakarma

University Institute of Technology RGPV (UIT - RGPV), Bhopal

Rajat Vishwakarma has verified this Calculator and 400+ more calculators!

< Atmospheric and Solar Radiation Calculators

Effective surface temperature of sun given solar constant

LaTeX Go Effective Surface Temperature = (((Mean Distance between Sun and Planet^2)*Total Solar Irradiance)/((Radius of the Sun^2)*[Stefan-BoltZ]))^0.25

Radius of sun given total solar irradiance

LaTeX Go Radius of the Sun = (((Mean Distance between Sun and Planet^2)*Total Solar Irradiance)/([Stefan-BoltZ]*(Effective Surface Temperature^4)))^0.5

Mean distance between sun or star and earth or planet

LaTeX Go Mean Distance between Sun and Planet = (((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/Total Solar Irradiance)^0.5

Total solar irradiance or solar constant

LaTeX Go Total Solar Irradiance = ((Radius of the Sun^2)*[Stefan-BoltZ]*(Effective Surface Temperature^4))/(Mean Distance between Sun and Planet^2)

Total solar energy incident on unit area of horizontal surface on ground Formula

LaTeX Go

Total Solar Energy = Direct Solar Radiation*cos(Angle of Incidence)+Direct Solar Radiation
G_solar = G_D*cos(i)+G_D

Why the Sky is Blue in Colour?

The sky is blue in clour because the air molecules scatter blue light much more than they do red or other lights. At sunset, the light travels through a thicker layer of the atmosphere, which removes much of the blue from the natural light, allowing the red to dominate.

How to Calculate Total solar energy incident on unit area of horizontal surface on ground?

Total solar energy incident on unit area of horizontal surface on ground calculator uses Total Solar Energy = Direct Solar Radiation*cos(Angle of Incidence)+Direct Solar Radiation to calculate the Total Solar Energy, Total solar energy incident on unit area of horizontal surface on ground formula is defined as the amount of solar radiation that falls on a unit area of a horizontal surface on the ground, which is a critical parameter in understanding the Earth's energy balance and climate dynamics. Total Solar Energy is denoted by G_solar symbol.

How to calculate Total solar energy incident on unit area of horizontal surface on ground using this online calculator? To use this online calculator for Total solar energy incident on unit area of horizontal surface on ground, enter Direct Solar Radiation (G_D) & Angle of Incidence (i) and hit the calculate button. Here is how the Total solar energy incident on unit area of horizontal surface on ground calculation can be explained with given input values -> 595.4473 = 337.1644*cos(0.698131700797601)+337.1644.

FAQ

What is Total solar energy incident on unit area of horizontal surface on ground?

Total solar energy incident on unit area of horizontal surface on ground formula is defined as the amount of solar radiation that falls on a unit area of a horizontal surface on the ground, which is a critical parameter in understanding the Earth's energy balance and climate dynamics and is represented as G_solar = G_D*cos(i)+G_D or Total Solar Energy = Direct Solar Radiation*cos(Angle of Incidence)+Direct Solar Radiation. The Direct Solar Radiation is the amount of solar energy received per unit area at a specific location, essential for understanding solar energy potential and environmental impact & The Angle of Incidence is the angle formed between an incoming ray of radiation and a line perpendicular to the surface it strikes.

How to calculate Total solar energy incident on unit area of horizontal surface on ground?

Total solar energy incident on unit area of horizontal surface on ground formula is defined as the amount of solar radiation that falls on a unit area of a horizontal surface on the ground, which is a critical parameter in understanding the Earth's energy balance and climate dynamics is calculated using Total Solar Energy = Direct Solar Radiation*cos(Angle of Incidence)+Direct Solar Radiation. To calculate Total solar energy incident on unit area of horizontal surface on ground, you need Direct Solar Radiation (G_D) & Angle of Incidence (i). With our tool, you need to enter the respective value for Direct Solar Radiation & Angle of Incidence and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.

Home

FREE PDFs

🔍 Search