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M. Rinner

Publications and source records attributed to M. Rinner.

3 recordsLinked to original sources

Gyrofluid Magnetic Reconnection Beyond the {\delta} F Approximation

Magnetic reconnection in a two-dimensional system is studied employing a novel Full-F gyrofluid model with arbitrary- wavelength polarization. In strongly magnetized plasmas, the long wavelength dimension parallel to the magnetic field can be separated from the much smaller perpendicular scales, motivating an isolated two-dimensional description. While previous studies have predominantly employed delta- F gyrofluid models, the present Full-F formulation is applied to simulate Harris-sheet magnetic reconnection with domain aspect ratios L_y/L_x <= 16, investigating tearing-mode growth, plasmoid formation, and the influence of finite ion Larmor radius (FLR) effects. In addition to a linear tearing-mode analysis, a non-modal stability analysis of the linearized system is performed. The evolution operator is shown to be strongly non-normal, exhibiting large condition numbers and extended pseudospectra that indicate the possibility of significant transient amplification, even in marginally stable regimes. Such transient amplification may facilitate the transition from linear tearing growth to rapid nonlinear acceleration. We focus on low-plasma-beta magnetic reconnection on the scale of the drift scale and incorporate ion FLR effects, placing the simulations in the context of magneti- cally confined fusion plasmas such as tokamaks. After discussing numerical resolution and convergence, we present a parameter scan varying the normalized electron skin depth and the ion-to-electron temperature ratio. Finally, the influence of aspect ratio, polarization model, and FLR effects on the reconnection dynamics and plasmoid formation is investigated.

physics.plasm-ph

The SRG/eROSITA All-Sky Survey $J$-Band Follow-Up Observations for Selected High-Redshift Galaxy Cluster Candidates

We select galaxy cluster candidates from the high-redshift (BEST_Z > 0.9) end of the first SRG/eROSITA All-Sky Survey (eRASS1) galaxy cluster catalogue, for which we obtain moderately deep J-band imaging data with the OMEGA2000 camera at the 3.5m telescope of the Calar Alto Observatory. We include J-band data of four additional targets obtained with the three-channel camera at the 2m Fraunhofer telescope at the Wendelstein Observatory. We complement the new J-band photometric catalogue with forced photometry in the i- and z-bands of the tenth data release of the Legacy Survey (LSDR10) to derive the radial colour distribution around the eRASS1 clusters. Without assuming a priori to find a cluster red sequence at a specific colour, we try to find a radially weighted colour over-density to confirm the presence of high-redshift optical counterparts for the X-ray emission. We compare our confirmation with optical properties derived in earlier works based on LSDR10 data to refine the existing high-redshift cluster confirmation of eROSITA-selected clusters. We attempt to calibrate the colour-redshift-relation including the new J-band data by comparing our obtained photometric redshift estimate with the spectroscopic redshift of a confirmed, optically selected, high-redshift galaxy cluster. We confirm 9 out of 18 of the selected galaxy cluster candidates with a radial over-density of similar coloured galaxies for which we provide a photometric redshift estimate. We can report an increase in the relative colour measurement precision from 8% to 4% when including J-band data. In conclusion, our findings indicate a not insignificant spurious contaminant fraction at the high-redshift end (BEST_Z > 0.9) of the eROSITA/eRASS1 galaxy cluster catalogue, as well as it underlines the necessity for wide and deep near infrared imaging data for confirmation and characterisation of high-$z$ galaxy clusters.

astro-ph.CO

GREENY: A Full-F 2D Gyrofluid Reconnection Code

We present the 2D gyrofluid magnetic reconnection code GREENY (Gyrofluid Reconnection with Extended Electromagnetic Nonlinearity). After a brief introduction to gyrofluids, magnetic reconnection, and the implemented models, we discuss the numerical framework and the algorithmic treatment of the quasi-neutrality condition and Amper\`e's law. Next, we present solver tests, conservation laws, and the influence of artificial subgrid dissipation on Harris-sheet magnetic reconnection. Finally, we show different applications, initial conditions and present example simulations.

physics.plasm-ph