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Astron. Astrophys. 355, 769-780 (2000) AcknowledgementsMV acknowledges the financial support of ESA during his stay at the
SOHO EOF where a substantial part of this study was carried out. MV is
also indebted to P. C. Martens and A. J. C. Beliïn for many
fruitful discussions and to the whole CDS team for creating the
excellent instrument. AF is supported by the United Kingdom PPARC.
SOHO is a project of international cooperation between ESA and NASA.
We thank B. Schmieder for useful comments. A part of this project was
supported by a grant A3003902 of GA AV
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