The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products★
Astronomy & Astrophysics EDP Sciences 666 (2022) a120
The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy★★★
Astronomy & Astrophysics EDP Sciences 666 (2022) a121
Validating and optimizing mismatch tolerance of Doppler backscattering measurements with the beam model (invited).
The Review of scientific instruments 93:10 (2022) 103536
Abstract:
We use the beam model of Doppler backscattering (DBS), which was previously derived from beam tracing and the reciprocity theorem, to shed light on mismatch attenuation. This attenuation of the backscattered signal occurs when the wavevector of the probe beam's electric field is not in the plane perpendicular to the magnetic field. Correcting for this effect is important for determining the amplitude of the actual density fluctuations. Previous preliminary comparisons between the model and Mega-Ampere Spherical Tokamak (MAST) plasmas were promising. In this work, we quantitatively account for this effect on DIII-D, a conventional tokamak. We compare the predicted and measured mismatch attenuation in various DIII-D, MAST, and MAST-U plasmas, showing that the beam model is applicable in a wide variety of situations. Finally, we performed a preliminary parameter sweep and found that the mismatch tolerance can be improved by optimizing the probe beam's width and curvature at launch. This is potentially a design consideration for new DBS systems.Our Galaxy’s youngest disc
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 516:3 (2022) 3454-3469
Prevention of core particle depletion in stellarators by turbulence
(2022)