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Observations of Doppler Shifts of X-Ray Lines in Solar Flare Spectra Based on DIOGENESS Spectrometer Data

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 400))

Abstract

The idea of measurement of X-ray lines Doppler shifts in spectra of the Sun, applied in DIOGENESS spectrometer, was previously developed and verified in rocket experiment with RDR X-ray Dopplerometer (Vertical-11 Rocket, 1981). Upon the obtained results two X-ray DIOGENESS spectrometers have been manufactured; the first one was operated aboard the CORONAS-I satellite (launch in 1994), while the second was operated aboard the CORONAS-F.

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References

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Acknowledgements

The works with DIOGENESS spectrometer have been carried out in the Solar Physics Laboratory of the Space Research Center of Polish Academy of Sciences in Wrocław (Poland), with the support of Polish Scientific Research Fund (project 1.PO3D.017.29 and 2011/01/B/ST9/05861).

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Correspondence to J. Sylwester .

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Kordylewski, Z. et al. (2014). Observations of Doppler Shifts of X-Ray Lines in Solar Flare Spectra Based on DIOGENESS Spectrometer Data. In: Kuznetsov, V. (eds) The Coronas-F Space Mission. Astrophysics and Space Science Library, vol 400. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-39268-9_5

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  • DOI: https://doi.org/10.1007/978-3-642-39268-9_5

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