Article | REF: AF6240 V1

From the photovoltaic effect to photoelectric cells

Author: Pierre-Eymeric JANOLIN

Publication date: July 10, 2013

You do not have access to this resource.
Click here to request your free trial access!

Already subscribed? Log in!


Français

1. From the

The Sun is the energy source for photovoltaic systems. To a first approximation, the Sun can be considered a black body with a temperature close to 6,000 K. The total power it radiates is given by Stefan-Boltzman's law and is not monochromatic, its spectral decomposition obeying Planck's law. In the case of the Sun, maximum emission occurs at 570 nm (in the yellow), and is divided into two wavelength ranges in the visible (380-780 nm) and infrared (780 nm-1 mm); ultraviolet radiation (200-380 nm) accounts for less than 1% of total radiation.

This solar energy is emitted isotropically, so only part of it is radiated towards the Earth. The amount of energy per second emitted by the Sun towards the Earth is approximately 1,360 kW/m 2

You do not have access to this resource.

Exclusive to subscribers. 97% yet to be discovered!

You do not have access to this resource.
Click here to request your free trial access!

Already subscribed? Log in!


The Ultimate Scientific and Technical Reference

A Comprehensive Knowledge Base, with over 1,200 authors and 100 scientific advisors
+ More than 10,000 articles and 1,000 how-to sheets, over 800 new or updated articles every year
From design to prototyping, right through to industrialization, the reference for securing the development of your industrial projects

This article is included in

Physics and chemistry

This offer includes:

Knowledge Base

Updated and enriched with articles validated by our scientific committees

Services

A set of exclusive tools to complement the resources

Practical Path

Operational and didactic, to guarantee the acquisition of transversal skills

Doc & Quiz

Interactive articles with quizzes, for constructive reading

Subscribe now!

Ongoing reading
From the