Small-scale structures and the density irregularity of the inner corona

Details Small-scale structures and the density irregularity of the inner corona Small-scale structures and the density irregularity of the inner corona

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..395o&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 395-399 (SEE N87-20871 13-92)

Mathematics

3

Anomalies, Electron Density (Concentration), Mathematical Models, Solar Corona, Coronal Holes, Coronal Loops, Emission Spectra, Extreme Ultraviolet Radiation, Solar Cycles

Scientific paper

The authors consider the observational evidence that the electron density irregularity factor >N2N<2 is much greater than unity in the inner corona, in particular, evidence derived from the photometric comparison of K-corona emission pB with the EUV emission from coronal ions. They develop a simple mathematical model for the irregularity having a minimum number of parameters. They use this model to explore some implications of the observations and to show that well-known resolved structures such as polar plumes and coronal loops as presently understood cannot alone explain the irregularity.

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