Projetos do DR5
     - Diagrama de Hubble
     - Cor
     - Tipos Espectrais
     - Diagrama H-R
     - Galáxias
     - Mapeamentos do Céu
     - Quasares
     - Processamento de Imagem
 Para Crianças
 Jogos e Competições
 Links para Outros
Image Processing
 What is an Image?
 Retrieving Images
 Analyzing Images
 Tricolor Images
 Other Images
 Other Features
 Alternate Views
     - Isophotes
     - 3-D Views
 Your Results

Alternate Views of Images


Another interesting way to view an image is through the use of isophotes. Isophotes are lines drawn through areas of constant brightness. Isophote images are very similar to contour maps, which show lines through areas of constant elevation.

Click on View and then Isophotes. The following window will appear:

X-Dim and Y-Dim are the size of the picture. High and low are the highest intensity and lowest intensity for which you want isophotes drawn. Step is how far in between isophotes. For the values shown above, Iris will draw isophotes where the intensity is 100, 200, 300, 400, 500, etc, up to 32,700. It is important to choose these numbers wisely.

Exercise 10. Open the green image of NGC 1087, the galaxy you used earlier. Click on View and then Isophotes. For the high value, you want to enter the intensity of the brightest pixel. To find this intensity, draw a box around the brightest area of the diagram. Right-click on the box and select Statistics. Enter the number for the maximum value in the high box (you may round to the nearest 100). Enter the image's minimum brightness value in the Low box. Select a step size that will give you 15 to 20 isophotes. Click OK.

Question 6. Where are the isophotes widely spaced? Where are the closely spaced? What does the distance between isophotes tell you?

3-D Views

Another way to view an image is with a 3-D view - a 3-D picture where the height represents the brightness of each pixel. Below you can see a 3-D view of two stars.

The dialog box for 3D view is shown below.

X Dim and Y Dim are the size of the picture and will usually not need to be changed. High and Low are the counts of the brightest and dimmest pixel you want to observe. Azimuth and elevation determine the viewing angle of the plot. Step is the size of the bins, in pixels, on the x and y axis used to make the 3-D graph. A smaller step size will give you a smoother, more detailed graph, but the graph will take longer to make.

Exercise 11. Once again, open the green image of NGC 1087. Click on View and 3D. You may adjust the High and Low to correspond to your max and min values. Click OK. You will see the 3D view. You may experiment with the azimuth and elevation. These values change the angle at which you view the display. The defaults will give you a good view, but you may find different angles better for a particular image.

Question 7. What parts of the image correspond to the highest peaks?