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Many people love pictures
This is a philosophical problem: epistemology refers to this – in my opinion, exaggeratedly [note SMH 2005] – as the ‘pictorial turn’. Basically, however, communicating with pictures has been common practice for centuries all over the world and is not at all an innovation of postmodernism (as some philosophers believe – let’s leave them to it, maybe they had bad teachers 🙁 ).
People also like to depict the starry sky. You can either stage it romantically – which can be done with fairly simple means – or use all the tools of digital photography to depict it so objectively that scientific insights can be gained from it.
Mood photos can be taken in almost any weather and even during a full moon. During a holiday trip through Spain, for example, I simply placed my digital camera on the roof of my rental car during a night-time break and exposed the constellation Sagittarius for 30 seconds. The rising full moon illuminated the rock (with sunlight, which is why it looks like daytime) and the passing clouds hardly interfere, but rather enliven the image in a more natural way: These images have not been edited and therefore show the original colours.
Film was more complicated, but digital cameras work very simply: a chip is a matrix (table) of light-sensitive cells. Each cell reacts to photons as soon as the camera shutter is opened by the shutter release. [Note: If you don’t know how this works in detail, find out more about the photoelectric effect.
Electronics then read how much light has reached each cell. This produces a black-and-white image. If you want colour images, some of the cells are covered with red filters, some with blue filters and some with green filters. Since the cells (pixels) are very small, they still work even if a few neighbouring cells are combined to form a single image point (pixel binning). This is why you can take true-colour images with black-and-white-sensitive photocells that have been fitted with filters.
Photography literally means ‘drawing with light,’ an art form with only about 150 years of tradition. Modern cameras are based on the CCD technology described above, making them ‘charge-coupled devices’ (electronic devices).
Some very creative teacher training students conducted an experiment to demonstrate this:
Resolution
They filled two fields with photocells at different densities. The field was evenly illuminated with different light sources (daylight, LED torch, halogen lamp). The incident light also triggers electrons (charge carriers) in a photocell n (as enlarged pixels). The more light that shines in, the more charge carriers are triggered.
Using a simple lux meter from a hardware store, we measure the light intensity at the location of the photocells. Then we measure the current generated by the light. [A smaller lux meter would allow us to better detect differences within the illuminated area, but we wanted to keep the experiment as simple as possible.] The results can then be plotted on a graph and analysed for errors.
Colour effects
In the second part of the experiment (shown above left), coloured glass slides from the optics kits used in many schools are placed in front of the LED torch (white). Once again, the voltage between each pair of contacts is measured.
When you record a film with a webcam, it consists of numerous individual images (stills). You can now add all these individual images together and even discard the poor ones (e.g. those blurred by the wind). This gives you a single image from a film (motion pictures) that is significantly better – i.e. sharper and richer in contrast – than the poor individual images in the film.
Amateur astronomer Georg Dittié was a guest at the ASL summer school in Hobbach in 2001, which I helped to organise. There he presented his GIOTTO software, which he now makes available free of charge on the Internet (with a request for donations).
In astrophotography, this has become a very common practice among amateur astronomers since the early 2000s because it allows you to take very beautiful pictures with very simple means.
Tip: GIOTTO software by Georg Dittié.
On the Yellow Tower in Hildesheim, we (my students and fellow astronomy enthusiast Uwe Zurmühl) photographed Jupiter on a very windy evening and produced this image.
The first image was taken in bright light. Then, when the eclipsed moon was high enough, I wanted to capture the mood. Since the moon appears too small in this image and the red discolouration (caused by the atmosphere, as it is only partially eclipsed!) is not visible, I photographed the moon through the eyepiece a few minutes earlier and added it to this image.