This tutorial shows how to do some simple analysis
of data in a Report window using table re-arrangement and the
Create Plot from Grid command. Here we examine
the effect a cosmic ray event has on
Statistics Measurements of an
Image Set. Some types of measurements may appear in a
Measurement Pane and others may appear in a
Report Window. The statistics measurements in this
tutorial appear in a
Grid Control in a
Report Window.
First,
open an image set for the BL-CAM*.fts sample images provided with the Mira
installation. Use File > Open to open the dialog below,
then select all 5 images as shown:
In the Options box at
the bottom of the dialog, be sure the "Open as Image Set" option is
chosen so that all 5 images will be opened into a single
Image Window.
Move the
Image Cursor to (column,row) position 530,299)
to enclose a cosmic ray that appears in only the first image,
BL-CAM.fts.
You will measure the entire image set, so be sure
the button on the
Image Bar (or
Image Set Toolbar) appears blue as shown, which
indicates "Image Set mode" will be used for measurements.
On the
Image Bar, click to
activate the Image Cursor. Move the
Image Cursor to (column,row) position (530,299) to
enclose a cosmic ray that appears in only the first image,
BL-CAM.fts. To get the same
statistics values as in this tutorial, you should adjust its size
to 46x46 pixels either by dragging its corner or by using the
Image Cursor Properties page (Ctrl+R).
To compute the statistics for all images, click the
button on the
Image Bar. The following grid of measurements then
appears in a
Report Window.
In the picture above you can see that the results
for measuring 5 images. The measurement data are wider than the
visible window. We could see the columns beyond the right border by
residing or scrolling the table. We could click on the column
separator lines and drag each column to a narrow width, but there
is a better way in this situation: Use the
Optimize Grid Columns command in the
View menu. This command shrinks all column widths to
the minimum size that still shows all information. The result shows
all columns within the original table width. If not, we could have
left it alone or enlarged the window simply by pulling the edge or
corner. Reports may be automatically optimized by checking the
Auto-Optimize Grid Columns setting in
the Report's View menu or the Optimize Grid
Columns setting on the
Table Appearance Properties page.
Next, we want to examine how the cosmic ray event
affects the average value inside the cursor rectangle. This
requires comparing the Maximum value (which shows the bright point)
with the Median and Standard Deviation. To make this easy, the
Maximum column will be moved between
the Median and Std Dev columns to put the 3 numbers of interest
together. Moving the column involves dragging the column header to
a new location as described below.
The next two pictures show the effect when you
mouse down on the column header for the Maximum value. With the mouse down, when you
start moving the mouse arrow, the column heading ("Maximum") turns
blue to highlight itself.
As you slide the mouse arrow to the left, the
column under the arrow highlights its left border to show the drop
position. In this example, you will be dropping the Maximum column between the Median and Std Dev
columns:
When you arrive at the drop location for the
Maximum column, release the mouse
button. The table is then reordered as follows:
Next, you will sort the row order by according to
increasing maximum value by clicking on the Maximum column header (a sort triangle appears
next to the "Maximum" column label). This shows that the highest
maximum value, caused by the cosmic ray event, corresponds to the
image having the lowest Median and Minimum values.
The table in the reordered state as shown above is
ready to accept new measurements in the new column order. To put
the rows back into their original measurement order, click the
#column on the left. This column
always lists the sequential order of measurement.