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Self-paced Beginner

Introduction and Solar radiation fundamentals

4(1591)
1 enrolled
561 views
FREE
157 min
Anytime
English
561 views
Team EveryEng
Team EveryEngMechanical Engineering
  • Lifetime access
  • Foundational Learning
  • Access to Study Materials
  • Self-Paced Learning

Why enroll

Unlock the potential of solar radiation! Learn the fundamentals of solar energy, including irradiance, irradiation, and solar zenith angle. Discover how to design and optimize solar energy systems for a sustainable future. Enroll now!

Is this course for you?

You should take this if

  • You work in Energy & Utilities
  • You're a Metallurgy & Material Science professional
  • You prefer self-paced learning you can revisit

You should skip if

  • You need a different specialisation outside Metallurgy & Material Science
  • You need live interaction with an instructor

Course details

This course provides a clear and simple introduction to solar energy and the fundamentals of solar radiation. It helps learners understand how the sun produces energy and how that energy reaches the Earth. You will learn about different types of solar radiation, such as direct, diffuse, and reflected radiation. The course also explains how solar energy is measured and the factors that affect its intensity, like location, time, and weather conditions. Basic concepts like the Earth–Sun relationship, solar angles, and day length are covered in an easy-to-understand way. It introduces tools and methods used to analyze solar radiation for practical applications. Learners will gain knowledge useful for designing solar energy systems like solar panels. Real-world examples are included to make concepts more relatable. This course is suitable for beginners, students, and professionals interested in renewable energy. By the end, you will have a strong foundation in how solar energy works and how it can be used efficiently.

Course suitable for

Key topics covered

  • Introduction to Solar Energy

  • Solar Radiation

  • Atmospheric Effects on Solar Radiation

  • Effects of Location on Time

  • Sun-Earth Angular Relation

Course content

The course is readily available, allowing learners to start and complete it at their own pace.

5 lectures2 hr 37 min
  1. Introduction to Solar Energy
    37 min
  2. Solar Radiation
    30 min
  3. Atmospheric Effects on Solar Radiation
    31 min
  4. Effects of Location on Time
    28 min
  5. Sun-Earth Angular Relation
    31 min

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Questions and Answers

A: A: GHI is tied to a horizontal reference. A normal-to-surface arrow contradicts that definition. B: POA is a calculated result, not a basic radiation component. C: Orientation doesn’t relax the horizontal requirement for GHI. D: Diffuse can be significant, but it doesn’t change the geometric definition.

A: A: Horizontal projection improves as altitude rises. B: DNI is along the beam, not horizontal. C: Air mass drops with altitude, not rises. D: Horizontal projection never equals DNI unless the sun is at 90°.

A: A: The hazard is optical, not electrical or thermal rating. B: LOTO doesn’t mitigate photon exposure. C: Insulation class protects conductors, not eyes or skin. D: Spacing for wind doesn’t stop a mirror redirecting sunlight.

A: A: Standard plots put the equator-facing direction downwards for northern sites. B: East-up isn’t a solar convention. C: Sun position uses true north, not magnetic. D: Symmetry doesn’t fix a flipped reference.