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In this lesson, students will analyze data from solar magnetogram images collected over 25 years at the National Solar Observatory Vacuum Telescope at Kitt Peak, AZ. Students construct a movie of solar images for a year's worth of data. From this movie, the approximate dates of perihelion and aphelion can be estimated from changes in the relative size of the solar images viewed. You should be able to answer the following when you have completed this exercise:
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Start the ImageJ program. From the toolbar, choose File from the menu bar and Import Image Sequence from the list of options. |
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Navigate to the disk drive that contains the DASL disk. A list of options similar to those you see to the left will appear. Choose Magnetograms and open that folder. |
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Inside the Magnetograms folder are data folders with images from the years 1977 through 2002. Choose a year by double clicking on the folder, or single clicking on it and choosing Open. |
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Inside each folder are magnetogram images for each date for which an image was taken. The file names indicate the year, month and date in the following format: 900101MA is the magnetogram png file for January 1, 1990. Open any image by double clicking on the file name. |
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A Sequence Options window similar to the one to the left will open. The information you can learn includes:
Choose OK to build the Image Sequence. |
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When the image sequence has been constructed, view the year from the Stack image that appears. View the year by holding down the right arrow on the scroll bar of the image window. Notice that the size of the solar disk gradually changes over the course of the year. |
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| RASL is a project supported by funds from National Solar Observatory Research Experience for Teachers, NASA, and in part by the Office of Naval Research. The NSO is operated by AURA under cooperative agreement with the National Science Foundation. | |||