C IV emission and magnetic topology. (Slovak Title: Emisia C IV a magnetická topológia)

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The contribution discusses a study of emissions of carbon ion C IV during solar flares. Data on the emission of the "clean" C IV and "clean" UV continuum were obtained from the emission observed in three TRACE UV filters 1550, 1600 and 1700. Their correlation was examined. We also studied the spatial correlation of flare nuclei with images in the calcium ion Ca II line and mainly its relation to quasiseparatrix positions calculated by extrapolation of the photospheric magnetogram assuming linear force-free approximation of the magnetic field. Perticular results were summarized and applied to a selected flare.

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