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Frantisek Farnik

Academy of Sciences of the Czech Republic

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STIX X-ray microflare observations during the Solar Orbiter commissioning phase

2021 arXiv: Solar and Stellar Astrophysics
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Is it possible to use the green coronal line instead of X rays to cancel an effect of the coronal emissivity deficit in estimation of the prominence total mass from decrease of the EUV-corona intensities?

2016
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X-ray Flare Spectra from the DIOGENESS Spectrometer and Its Concept Applied to ChemiX on the Interhelioprobe Spacecraft

2015 Solar Physics
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KAPPA: Optically thin spectra synthesis for non-Maxwellian kappa-distributions

2015
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KAPPA: A PACKAGE FOR SYNTHESIS OF OPTICALLY THIN SPECTRA FOR THE NON-MAXWELLIAN κ-DISTRIBUTIONS BASED ON THE CHIANTI DATABASE

2015 Astrophysical Journal Supplement Series
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X-ray Flare Spectra from the DIOGENESS Spectrometer and Its Concept Applied to ChemiX on the Interhelioprobe Spacecraft

2015 Solar Physics
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KAPPA: A PACKAGE FOR SYNTHESIS OF OPTICALLY THIN SPECTRA FOR THE NON-MAXWELLIAN κ-DISTRIBUTIONS BASED ON THE CHIANTI DATABASE

2015 Astrophysical Journal Supplement Series
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IMAGING AND SPECTROSCOPIC OBSERVATIONS OF A TRANSIENT CORONAL LOOP: EVIDENCE FOR THE NON-MAXWELLIAN κ-DISTRIBUTIONS

2015 The Astrophysical Journal
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Flat crystal Bragg observations of the X-ray spectra during impulsive phases of solar flares

2014
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Soft X-ray spectra of strong flares seen by Bragg flat crystal spectrometer aboard Coronas-F

2014
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