Forward Modeling of EIS Spectroscopic Data Emitted by a Vertically Oscillating Loop

Details Forward Modeling of EIS Spectroscopic Data Emitted by a Vertically Oscillating Loop Forward Modeling of EIS Spectroscopic Data Emitted by a Vertically Oscillating Loop

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..397...58d&link_type=abstract

First Results From Hinode ASP Conference Series, Vol. 397, Proceedings of the conference held 20-24 August, 2007, at Trinity Col

Astronomy and Astrophysics

Astronomy

Scientific paper

This paper focuses on forward modeling of spectroscopic data, as would be emitted by a coronal loop oscillating in the vertical fast kink mode. The Doppler shift, broadening and deformation of the observed spectral lines are investigated. It is concluded that the vertical kink mode causes strong line broadening, either inside the loop or at the edges of the loop, depending on the time integration and the oscillatory phase observed.

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