Multi-Frequency Imaging of the Type U Emission; Unexpected Behaviour

Details Multi-Frequency Imaging of the Type U Emission; Unexpected Behaviour Multi-Frequency Imaging of the Type U Emission; Unexpected Behaviour

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..165..201r&link_type=abstract

Solar Physics, Volume 165, Issue 1, pp.201-204

Physics

Scientific paper

We present here an example of solar type U emission for which the
negative drift and positive drift branches are emitted at the same
location in the corona. This is observed at four frequencies between 435
and 236 MHz. This observation may bring new insights to the dynamics of
the corona in relationship with the acceleration process of particles.

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