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- W85738304 abstract "Abstract. In this paper we examine regions of internetwork,network and bright network emission, observed in the quietSun with the Coronal Diagnostic Spectrometer (cds) onboardSoHO. The slopes of the emission measure distributions, be-tween5.4≤logT e ≤6.0,arefoundtodifferineachregion,sug-gesting the presence of different atmospheric structures. Froman analysis of emission area the network is shown to have twopopulations of structures, a low transition region group and acoronal group. Using mdi magnetograms the bright networkemission is shown to originate from regions of strong magneticfield composed of bipolar loops and unipolar funnels, that ex-tend from the low transition region up to the corona. Up to 30%of all radiative losses between 5.7 ≤ log T e ≤ 6.3 are found tocome from these continuous bright network structures. Cross-sectional areas calculated from redshift values suggest that thearea expansion seen in the bright network emission is the resultof flux tube expansion into the corona, accompanied by eithera downflow or upflow of material.Key words: techniques: image processing – methods: observa-tional–Sun:corona–Sun:transitionregion–Sun:UVradiation– Sun: atmosphere1. IntroductionThe simplest picture of the transition region, formed betweentemperatures of ∼10" @default.
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- W85738304 date "2000-06-01" @default.
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- W85738304 title "Transition region and coronal structuring" @default.
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