FASR Flare Science: Lessons from the Nobeyama Radioheliograph

Details FASR Flare Science: Lessons from the Nobeyama Radioheliograph FASR Flare Science: Lessons from the Nobeyama Radioheliograph

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spnr.conf..121g&link_type=abstract

Solar Physics with the Nobeyama Radioheliograph, Proceedings of Nobeyama Symposium 2004, held in Kiyosato, Japan, October 26- 29

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Scientific paper

We compare and contrast the instrumental parameters of the Nobeyama Radioheliograph (NoRH) and the future Frequency Agile Solar Radiotelescope (FASR) with an emphasis on flare research. The primary results and discoveries of NoRH in the realm of flare science are presented and used to motivate many of the choices for design parameters and science goals for FASR. Key parameters of NoRH for flare science are its dual-frequency, dual-polarization, excellent image quality, solar-dedicated and solar-optimized design, and high time resolution. Its main limitations are spatial resolution, frequency coverage, and frequency resolution. FASR's design makes use of the strengths of NoRH, and adds these three missing elements: a factor of 10 improvement in spatial resolution, broad frequency coverage and high frequency resolution. We discuss the manner in which these improvements extend the legacy of NoRH for flare science.

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