Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8314031a&link_type=abstract
Unknown
Astronomy and Astrophysics
Astronomy
Galactic Structure, Image Processing, Millimeter Waves, Radio Astronomy, Sun, Color Coding, Computer Techniques, Imaging Techniques, Remote Sensing, Solar Activity, Stellar Structure, Temperature Distribution
Scientific paper
A technique for mapping astrophysical objects with millimeter microwaves and using image processing techniques used in remote sensing is described. Combination of the two techniques provides an image of the structure of astrophysical objects in a form produced by no other method. The mapping was performed using the large 14 m microwave antenna at Itapetinga at frequencies of 22 and 44 GHz. The data software is produced in a I-100 computer using the SERE program. The data were converted into temperature form and the temperatures associated with five colors, each divided into seven color tones from red to violet in ascending temperatures. Image of the Galactic center and of the active and quiescent Sun are presented.
Abraham Zulema
Costa Joaquim E. Rezende
Kaufmann Patrik
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