TRACE Observational Consequences of a Synthetic Multithermal Loop

Details TRACE Observational Consequences of a Synthetic Multithermal Loop TRACE Observational Consequences of a Synthetic Multithermal Loop

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..415..295s&link_type=abstract

The Second Hinode Science Meeting: Beyond Discovery-Toward Understanding ASP Conference Series, Vol. 415, proceedings of a meeti

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a global coronal loop as 125 individual strands, with each modelled independently by a one-dimensional hydrodynamic simulation. The strands are coupled together through the frequency distribution of nanoflare energy. The simulated data is then folded through the temperature response function of three different pass-bands of the Transition Region and Coronal Explorer (TRACE) to derive the corresponding intensity. Subsequently, the filter-ratio method is employed to derive the temperature from the deduced synthetic emission. The emission measure (EM) loci method is also employed to determine the loop temperature.

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