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. Solanki31 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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