2017
DOI: 10.1007/s10509-017-3213-x
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Anti-phase oscillations of H α $\alpha$ line Doppler velocity and width in solar limb spicules

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Cited by 4 publications
(4 citation statements)
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“…The authors determined the properties of spicules and calculated the oscillations present in these structures. The study by Khutsishvili et al (2017) also revealed that the oscillations of Doppler velocity and width appear to be out of phase with one another. This anti-phase relation is determined from the strong Doppler velocity to weaker Doppler width and vice-versa.…”
Section: Wave Phenomena In Solar Jetsmentioning
confidence: 91%
See 1 more Smart Citation
“…The authors determined the properties of spicules and calculated the oscillations present in these structures. The study by Khutsishvili et al (2017) also revealed that the oscillations of Doppler velocity and width appear to be out of phase with one another. This anti-phase relation is determined from the strong Doppler velocity to weaker Doppler width and vice-versa.…”
Section: Wave Phenomena In Solar Jetsmentioning
confidence: 91%
“…This velocity will depend on the location of the observer (or Line-of-Sight) relative to the flux tube's bulk transverse motion (see Figure 11) and the radiative properties of the plasma along the line of sight. Doppler shift oscillations have recently been observed in Hα solar spicules (Zaqarashvili et al, 2007a;De Pontieu et al, 2012;Khutsishvili et al, 2014Khutsishvili et al, , 2017. The authors determined the properties of spicules and calculated the oscillations present in these structures.…”
Section: Wave Phenomena In Solar Jetsmentioning
confidence: 99%
“…Oscillations and waves in solar chromosphere and corona and chromospheric spicules are studied (Khutsishvili et al 2017). Observations of spectral lines in the chromosphere by height and time are made using the 53-cm solar coronagraph of ABAO.…”
Section: Research Topicsmentioning
confidence: 99%
“…Variation of the parameters with the heights need to be measured. Wave motions have been sought in the chromosphere and TR over a wide range of frequencies (Nikolskii 1965;Tavabi et al 2015b;Khutsishvili et al 2017). Fluctuations in Doppler velocity and intensity are also observed in the 10 5 K plasma.…”
Section: Introductionmentioning
confidence: 99%