Solar Equations

0.0(0)
studied byStudied by 0 people
GameKnowt Play
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
Card Sorting

1/16

encourage image

There's no tags or description

Looks like no tags are added yet.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

17 Terms

1
New cards

Q: What is the solar constant E0 and its typical value?

A: Solar constant ≈ 1360–1367 W/m² at 1 AU, measured perpendicular to rays, outside atmosphere

2
New cards

Q: Why is irradiance on Earth lower than in space?

A: Due to atmospheric reflection, absorption (O₃, H₂O, O₂, CO₂), Rayleigh scattering (small particles), and Mie scattering (large particles).

3
New cards

Q: Define air mass ratio (AM) and give its formula.

A: Relative optical path length through atmosphere; m=1/cosψ, where ψ is solar zenith angle.

4
New cards

Q: What is AM 1.5 and why is it important?

A: Standard spectrum for PV testing; represents sunlight at 1.5× vertical path length, typical of mid-latitudes.

5
New cards

Q: What is the declination angle (θd)?

A: Angle between Sun’s rays and Earth’s equatorial plane; ranges from –23.5° to +23.5° annually.

6
New cards

Q: Formula for irradiance normal to a tilted plane (α)?

A: En = Ecos⁡θdsin⁡(θ+α)sin⁡ϕ + Esin⁡θdcos⁡(θ+α)

7
New cards

Q: State the Hottel equation for direct beam irradiance at surface.

A: E=E0(b0+b1e−km)E=E0​(b0​+b1​e−km), where m = air mass ratio and b0,b1,kb0​,b1​,k depend on visibility.

8
New cards

Q: Condition for optimal fixed panel tilt at noon on a given day?

A: θ+α+θd = 90∘ ; where θ is the solar zenith angle and α is the panel tilt angle.

9
New cards

Q: Formula for minimum row spacing to avoid shading at noon?

A: Dmin= Lcos⁡α+(Lsin⁡α)cot⁡β, with β=θ−23.5∘ (NH).

10
New cards

Q: What happens when photon energy < semiconductor band gap?

A: No electron–hole pairs; photon passes through or is reflected.

11
New cards

Q: How does doping change silicon for PV?

A: n-type (Group V) adds electrons; p-type (Group III) creates holes; p–n junction forms depletion region. Doping introduces charge carriers in silicon.

12
New cards

Q: Name the four key PV I–V curve parameters.

13
New cards

: Effect of increasing irradiance on I–V curve?

A: Isc increases; MPP shifts upward; Voc increases slightly.

14
New cards

Q: Formula for PV module efficiency.

15
New cards

Q: How to split energy in a PV-T system?

16
New cards

Q: Formula for power through a vertical window.

A: P= τAEn , with α = 90∘

17
New cards

Q: Why can tracking underperform fixed on overcast days?

A: Diffuse radiation is isotropic; tracking panels may be steep at morning/evening, capturing less diffuse light.