Whitgift School light reflection & refraction demonstration

Dr Jonathan Hare (Sussex University, who was scientist in residence at Whitgift in 2017) and Whitgifts head of Physics, Ian Hanley are currently designing and building a wall mounted exhibit for one of the new science laboratories. It will demonstrate the way light can be manipulated by reflection and refraction. The idea is the participants have to guide a light beam across the apparatus using what they know about reflection (angles of incidence and angles of reflection) by directing the beam via a 'maze' of mirrors randomly distributed (but adjustable) across the apparatus. The demonstration uses special electronics designed to minimise extraneous signals from day light or classroom lights so that the students have the maximum opportunity to peak the signals making it through the array of mirrors - to get the best signal possible. The demonstration highlights how vital signal measurement and the problem of noise are to modern scientific investigations. This fun activity will help to hone the participants experimental skills.


Light Demo diagram

Basic diagram of the light beam demonstration showing the light source (left hand side) which can be set for visible or Infrared light and the mirrors that are used to reflect the light onto the detector (to the right). Both the light source and detector have magnet bases that allow them to be attached to the metal covered board where they can easily be adjusted to any position or angle. The number of LEDs that light the detector electronics (far right) is dependant on the strength of the signal making its way through the mirror refections. - there are two sensitivity settings (high and low).


Light Demo Board 1 mirror Light Demo Board 1 mirror + red line

In these pictures the light source (left hand side) has been switched to visible light and we are only using one mirror to reflect the light onto the detector (to the right). Both the light source and detector have magnetic bases that allows them to be easily adjusted for position and angle.



Light Demo Board 1 mirror Light Demo Board 1 mirror + red line

As above but using two mirrors to reflect the light onto the detector.



Light Demo Board 1 mirror Light Demo Board 1 mirror + red line

As above but using three mirrors to reflect the light onto the detector.



Light Demo Board 1 mirror Light Demo Board 1 mirror + red line

As above but using four mirrors to reflect the light onto the detector.



detector

The photo diode detector in its box - you can see the collar in front of the detector which helps to screen out unwanted light and collimate the responce of the detector.




mirrors & prisms

Two mirrors in their 3D printed mirror supports.
The mirrors rotate on the mount so they can be easily adjusted to the correct angle to reflect the light beam.




mirrors & prisms

Picture of the magnetic mounted prism and mirrors.
The mirrors and prism rotate so can be easily adjusted for the correct angle.




light pipe

Diagram showing how a light beam arriving into the light pipe (within a critical angle) will be internally reflected along it
and delivered to the light detector. In contrast very little signal is detected without the light pipe for this angle. Also see pictures below.




no light pipe

light pipe acceptance angle

Perspex light pipe

Close up of the 3D printed light pipe stand. The light pipe is a 10cm long piece of Perspex with polished ends.



vis & IR light box

The light source box: visible white light or Infrared light can be selected.



LEDs and PSD unit

Picture showing the electronics in the clear plastic box.



gain select

The electronics can be set for low or high gain.
High gain is needed when the signal low such when the light beam is past though many optical devices e.g. four mirrors and the prism.




notebook II

Some early notebook apparatus design ideas I



notebook I

Some early notebook apparatus design ideas II



mains PSUs

The equipment only needs these two small 9V DC power supplies for all the electronics.



DC input

Two DC input sockets from the low voltage mains power supplies



POSSIBLE TEXT FOR SIGNS & PRINTING


The idea of the demonstration:
Detect the light coming from the left hand side LEDs, using the photo diode detector on the right - the Yellow LED bar graph will light up when you have a clear signal path. It's easy to send the light across the board to shine directly onto the light detector, making all the LEDs on the bar graph light up. Your challenge however is to try and use as many mirrors as possible to reflect the light beam by the longest and most complex path you can. You will have to shine the light onto each proceeding mirror using your knowledge of incident and reflection angles. You can also use the glass prism as a reflector and refraction through the light pipe (crude fibre optic) to make the total path more interesting and diverse.


One or two mirrors is easy but can use all the mirrors as well as the prism and light pipe?


Once you have the skill to reliably send a visible beam across the apparatus you can try using the invisible Infrared LEDs!


During this activity you will develop an intuitive feeling for incident reflection angles and acquire experimental skills on how to peak and optimise signals.


About the mirrors - each mirror is fitted to a magnetic stand held onto the board. You can position and rotate the mirrors anywhere on the board to get the correct angles to pass the light beam on. There is light loss from the mirrors so the more mirrors you use, the less light will be passed through the combined system.


There are two sensitivities you can select to help you; however the most sensitive setting also has a slightly longer response time, so you have to be skilled with the settings and patient with the response.


About the light pipe - the light pipe is also fitted to a magnetic stand and so can be positioned where you want it. Light will only pass through if the light entering is near a critical angle (the light is then internally reflected).


About the prism - the prism is fitted to a magnetic stand and can be rotated to any angle. When correctly adjusted the light beam can be internally reflected within the prism - behaving like a high quality mirror.


Phase Sensitive Detector (PSD) - The photo diode detector is sensitive to many kinds of light, including unwanted noise sources such as daylight and the classroom lights. However our LEDs are pulsing using a modulation circuit (500 Hz - 1kHz). The PSD uses this modulation frequency as a reference to 'lock-in' the amplifier only to signals from the LEDs. The noise signals from other sources are not locked-in and are effectively cancelled. This makes the electronics extremely sensitive yet robust and selective. PSDs are used in a range of state-of-the-art science experiments from climate change gas measurements to extremely accurate weights & measures.



diagrams

1 mirror, 2 mirror, 3 mirror
prism as mirror
light pipe critical angle





THE CREATIVE SCIENCE CENTRE

Dr Jonathan Hare, The University of Sussex
Brighton, East Sussex. BN1 9QJ.

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