Physics
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..135r&link_type=abstract
In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 135-142 (SEE N87-20871 13-92)
Physics
8
Chromosphere, Conductive Heat Transfer, Interfaces, Plasmas (Physics), Solar Corona, Solar Magnetic Field, Solar Physics, Solar Prominences, Sun, Emission Spectra, Mathematical Models
Scientific paper
The classical model of the chromosphere-corona transition does not account for the observed behavior of the differential emission measure for T approx. less than 100,000 K. Several models have been proposed to resolve this discrepancy in physically different ways. Because the observed differential emission measure at the prominence-corona interface is on average nearly the same as in the chromosphere-corona transition, prominences offer a fresh testing ground for models tailored to the chromosphere-corona transition. The researcher considered three such models and concluded that none extends in a natural way to the environment of prominences. The researcher advanced a simple idea involving thermal conduction both along and across the magnetic field from the corona into cool threads.
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