Scaling Law of Solar Coronal Loops Obtained with YOHKOH

Details Scaling Law of Solar Coronal Loops Obtained with YOHKOH Scaling Law of Solar Coronal Loops Obtained with YOHKOH

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...454..934k&link_type=abstract

Astrophysical Journal v.454, p.934

Astronomy and Astrophysics

Astronomy

84

Magnetohydrodynamics: Mhd, Sun: Corona, Sun: X-Rays, Gamma Rays

Scientific paper

We find a clear correlation among the maximum temperature Tmax (K), the pressure p (dyn cm-2) and the length L (cm) of 32 steady coronal loop structures observed with Yohkoh Soft X-Ray Telescope: Tmax = 3.8 × 104 (pL)1/(5.1±0.5). The best-fit equation, however, systematically deviates from the theoretical scaling law Tmax = 1.4 × 103 (pL)1/3 derived by Rosner, Tucker, & Vaiana. We examine various possibilities for the cause of the discrepancy.

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