Infrared Studies of Solar Convection

Details Infrared Studies of Solar Convection Infrared Studies of Solar Convection

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stin...0137723g&link_type=abstract

Technical Report, AD-A386915; AFRL-SR-BL-TR-01-0134 Big Bear Solar Observatory

Physics

Solar Corona, Solar Magnetic Field, Magnetic Flux, Infrared Radiation, Magnetic Signatures, Solar Cycles

Scientific paper

This ASSERT grant was to support the Ph.D. work of Tom Spirock who is a native of New Jersey. Tom will finish his Ph.D. this year, thanks in large part to ASSERT support. His work was to build an infrared magnetograph and use it for scientific work. Solar magnetic fields are concentrated in flux tubes, and appear on different scales: sunspots, pores (small sunspots without penumbra) and magnetic network flux elements. The magnetic network elements are the detritus of decaying active regions and play an important part in the solar cycle. They are very long lived.

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