Solar Max 2000: Scientific Objectives and Coordinated Observation

Details Solar Max 2000: Scientific Objectives and Coordinated Observation Solar Max 2000: Scientific Objectives and Coordinated Observation

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..453k&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

The solar maximum 2000 will be an unprecedented opportunity for solar physicists to conduct detailed studies of various solar active phenomena with a lineup of advanced, space-borne, and ground-based observing instruments. Of particular importance is a combination of hard X- and gamma-ray imaging made with the High Energy Solar Spectroscopic Imager (HESSI) and radio imaging made with, e.g., the dual-frequency Nobeyama Radioheliograph, with which we anticipate being able to understand magnetic energy release and particle acceleration mechanisms more deeply than so far achieved. The lineup of the observing instruments in the coming Max 2000 and their scientific objectives are discussed from a viewpoint of coordination of observations.

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