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Free access article

Issue A&A
Volume 403, Number 2, May IV 2003
Page(s) 725 - 730
Section Diffuse matter in space
DOI http://dx.doi.org/10.1051/0004-6361:20030400



A&A 403, 725-730 (2003)
DOI: 10.1051/0004-6361:20030400

Variability of EUV-spectra from the quiet upper solar atmosphere: Intensity and Doppler shift

A. Brkovic1, 2, H. Peter1 and S. K. Solanki3

1  Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany
2  Institute of Astronomy, ETH-Zentrum, 8092 Zürich, Switzerland
3  Max-Planck-Institut für Aeronomie, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany

(Received 15 May 2002 / Accepted 11 March 2003 )

Abstract
We have studied SUMER and CDS time series of spectra and images of quiet-Sun regions at the solar disc centre. The data contain ultraviolet emission lines sampling temperatures of the chromosphere, transition region and corona. We find a high correlation between average net Doppler shifts and relative brightness variabilities of the studied lines (correlation coefficient of  0.92), suggesting a connection between the two quantities. The anti-correlation between differential emission measures and relative brightness variabilities is weaker (correlation coefficient of -0.78). We discuss the observed relationships on the basis of differential emission measures and linear wave calculations.


Key words: Sun: chromosphere -- Sun: corona -- Sun: transition region -- Sun: UV radiation

Offprint request: A. Brkovic, alen@kis.uni-freiburg.de




© ESO 2003

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