Other
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..tsf.b4004r&link_type=abstract
American Physical Society, Joint Fall Meetings of the Texas Sections of the APS, and AAPT, Zone 13 of the SPS, and the National
Other
Scientific paper
The physics department at the University of North Texas is conducting a study of radio signals from our Sun. Radio Signals collected in a range of 1.4125X109Hz to 1.4175X109Hz were examined, along with signals outside this range, to search for a signature of the 21.11-cm hydrogen emission spectra in the sun's output. Monitoring of the sun spot activity of the sun is being conducted with optical telescopes, internet searches and radio telescopes. The data, once collected, were examined to search for any correlation between the sunspot cycle and the change in flux of the 21.11-cm emissions spectra. Two signatures in the data were sought, one that was different from all the rest and another group showing a general trend. Sunspots are highly magnetized portions of the surface of the sun. With the increase in sunspot activity, there is also an increase in the magnetized portions of the surface of the sun and an increase in the 21.11-cm emissions spectra is observed. Equations to predict the increase in flux corresponding to this spectra based on sunspot numbers are given in this work.
Imholt Tim
Roberts James A.
University Of North Texas Team
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