Ephemeral region flares and the diffusion of the network

Details Ephemeral region flares and the diffusion of the network Ephemeral region flares and the diffusion of the network

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...59..105m&link_type=abstract

Solar Physics, vol. 59, Sept. 1978, p. 105-113.

Physics

20

Ephemerides, H Alpha Line, Solar Flares, Solar Granulation, Solar Magnetic Field, Solar X-Rays, Magnetic Signatures, Network Analysis, Plasma Diffusion, Plasma Interactions, Polarity

Scientific paper

Flarelike events which are frequently observed in H-alpha in apparently quiet regions of the solar disk can be in all cases identified with bipolar ephemeral regions (ER) on magnetograms. These events represent the H-alpha counterpart of X-ray bright point flares. Statistically, this phenomenon is associated with the proximity of the bipolar features to the supergranulation network in the sense that an ER is likely to flare during its lifetime if the distance to the nearest network element is less than or equal to its own pole separation.

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