On the spicular density enhancement in the region of formation

Details On the spicular density enhancement in the region of formation On the spicular density enhancement in the region of formation

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42...67s&link_type=abstract

Solar Physics, vol. 42, May 1975, p. 67-70.

Physics

Density Distribution, Solar Atmosphere, Spicules, Astronomical Models, Conservation Equations, Solar Activity, Solar Granulation, Solar Magnetic Field

Scientific paper

The possibility is examined of setting an upper limit to the density enhancement of solar spicules relative to their formation region. The total conductive energy per sec available in a spicular region is determined analytically together with the total energy radiated per sec and the maximum density enhancement in the same region. The results indicate that spicules cannot cover more than 8% of the surface in their formation region and that at least 13% of the downward conductive flux must be directed from interspicular regions to rosette centers.

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