\begin{thebibliography}{25}
\providecommand{\natexlab}[1]{#1}

\bibitem[\protect\citeauthoryear{{Brandenburg}
  {\itshape{et~al.}}}{2024{\natexlab{a}}}]{2024arXiv240108569B}
{Brandenburg}, A., {Neronov}, A. and {Vazza}, F., {Resistively controlled
  primordial magnetic turbulence decay}. {\itshape arXiv e-prints},
  2024{\natexlab{a}}, arXiv:2401.08569.

\bibitem[\protect\citeauthoryear{{Brandenburg}
  {\itshape{et~al.}}}{2024{\natexlab{b}}}]{2024PhRvD.109d3534B}
{Brandenburg}, A., {Clarke}, E., {Kahniashvili}, T., {Long}, A.J. and {Sun},
  G., {Relic gravitational waves from the chiral plasma instability in the
  standard cosmological model}. {\itshape \prd}, 2024{\natexlab{b}},
  \textbf{109}, 043534.

\bibitem[\protect\citeauthoryear{{Ca{\~n}as}
  {\itshape{et~al.}}}{2024}]{2024PSJ.....5...55C}
{Ca{\~n}as}, M.H., {Lyra}, W., {Carrera}, D., {Krapp}, L., {Sengupta}, D.,
  {Simon}, J.B., {Umurhan}, O.M., {Yang}, C.C. and {Youdin}, A.N., {A Solution
  for the Density Dichotomy Problem of Kuiper Belt Objects with Multispecies
  Streaming Instability and Pebble Accretion}. {\itshape \psj}, 2024,
  \textbf{5}, 55.

\bibitem[\protect\citeauthoryear{{Dey}
  {\itshape{et~al.}}}{2024}]{2024arXiv240416096D}
{Dey}, S., {Chatterjee}, P. and {Erdelyi}, R., {Spinning solar jets explained
  through the interplay between plasma sheets and vortex columns}. {\itshape
  arXiv e-prints}, 2024, arXiv:2404.16096.

\bibitem[\protect\citeauthoryear{{Dwivedi}
  {\itshape{et~al.}}}{2024}]{2024arXiv240101965D}
{Dwivedi}, S., {Anandavijayan}, C. and {Bhat}, P., {Quasi-two-dimensionality of
  three-dimensional, magnetically dominated, decaying turbulence}. {\itshape
  arXiv e-prints}, 2024, arXiv:2401.01965.

\bibitem[\protect\citeauthoryear{{Elias-L{\'o}pez}
  {\itshape{et~al.}}}{2024}]{2024arXiv240410804E}
{Elias-L{\'o}pez}, A., {del Sordo}, F. and {Vigan{\`o}}, D., {Vorticity and
  magnetic dynamo from subsonic expansion waves II: Dependence on magnetic
  Prandtl number, forcing scale, cooling time}. {\itshape arXiv e-prints},
  2024, arXiv:2404.10804.

\bibitem[\protect\citeauthoryear{{Gent}
  {\itshape{et~al.}}}{2024}]{2024ApJ...961....7G}
{Gent}, F.A., {Mac Low}, M.M. and {Korpi-Lagg}, M.J., {Transition from
  Small-scale to Large-scale Dynamo in a Supernova-driven, Multiphase Medium}.
  {\itshape \apj}, 2024, \textbf{961}, 7.

\bibitem[\protect\citeauthoryear{{Hackman}
  {\itshape{et~al.}}}{2024}]{2024A&A...682A.156H}
{Hackman}, T., {Kochukhov}, O., {Viviani}, M., {Warnecke}, J., {Korpi-Lagg},
  M.J. and {Lehtinen}, J.J., {From convective stellar dynamo simulations to
  Zeeman-Doppler images}. {\itshape \aap}, 2024, \textbf{682}, A156.

\bibitem[\protect\citeauthoryear{{Hosking}
  {\itshape{et~al.}}}{2024}]{2024arXiv240101336H}
{Hosking}, D.N., {Wasserman}, D. and {Cowley}, S.C., {Metastability of
  stratified magnetohydrostatic equilibria and their relaxation}. {\itshape
  arXiv e-prints}, 2024, arXiv:2401.01336.

\bibitem[\protect\citeauthoryear{{Iarygina}
  {\itshape{et~al.}}}{2024}]{2024JCAP...04..018I}
{Iarygina}, O., {Sfakianakis}, E.I., {Sharma}, R. and {Brandenburg}, A.,
  {Backreaction of axion-SU(2) dynamics during inflation}. {\itshape \jcap},
  2024, \textbf{2024}, 018.

\bibitem[\protect\citeauthoryear{{K{\"a}pyl{\"a}}}{2024}]{2024A&A...683A.221K}
{K{\"a}pyl{\"a}}, P.J., {Convective scale and subadiabatic layers in
  simulations of rotating compressible convection}. {\itshape \aap}, 2024,
  \textbf{683}, A221.

\bibitem[\protect\citeauthoryear{{Kesri}
  {\itshape{et~al.}}}{2024}]{2024arXiv240410720K}
{Kesri}, K., {Dey}, S., {Chatterjee}, P. and {Erdelyi}, R., {Dependence of
  spicule properties on magnetic field -- results from Magnetohydrodynamics
  simulations}. {\itshape arXiv e-prints}, 2024, arXiv:2404.10720.

\bibitem[\protect\citeauthoryear{{Kirchschlager}
  {\itshape{et~al.}}}{2024}]{2024NatCo..15.1841K}
{Kirchschlager}, F., {Mattsson}, L. and {Gent}, F.A., {Supernova dust
  destruction in the magnetized turbulent ISM}. {\itshape Nat. Comm.}, 2024,
  \textbf{15}, 1841.

\bibitem[\protect\citeauthoryear{{Korpi-Lagg}
  {\itshape{et~al.}}}{2024}]{2024arXiv240104015K}
{Korpi-Lagg}, M.J., {Mac Low}, M.M. and {Gent}, F.A., {Computational approaches
  to modeling dynamos in galaxies}. {\itshape arXiv e-prints}, 2024,
  arXiv:2401.04015.

\bibitem[\protect\citeauthoryear{{Maity}
  {\itshape{et~al.}}}{2024}]{2024ApJ...962...86M}
{Maity}, S.S., {Sarkar}, R., {Chatterjee}, P. and {Srivastava}, N., {Changes in
  Photospheric Lorentz Force in Eruptive and Confined Solar Flares}. {\itshape
  \apj}, 2024, \textbf{962}, 86.

\bibitem[\protect\citeauthoryear{{Qazi}
  {\itshape{et~al.}}}{2024}]{2024MNRAS.527.7994Q}
{Qazi}, Y., {Shukurov}, A., {Tharakkal}, D., {Gent}, F.A. and {Bendre}, A.B.,
  {Non-linear magnetic buoyancy instability and turbulent dynamo}. {\itshape
  \mnras}, 2024, \textbf{527}, 7994--8005.

\bibitem[\protect\citeauthoryear{{Schober}
  {\itshape{et~al.}}}{2024{\natexlab{a}}}]{2024PhRvL.132f5101S}
{Schober}, J., {Rogachevskii}, I. and {Brandenburg}, A., {Chiral Anomaly and
  Dynamos from Inhomogeneous Chemical Potential Fluctuations}. {\itshape \prl},
  2024{\natexlab{a}}, \textbf{132}, 065101.

\bibitem[\protect\citeauthoryear{{Schober}
  {\itshape{et~al.}}}{2024{\natexlab{b}}}]{2024arXiv240407845S}
{Schober}, J., {Rogachevskii}, I. and {Brandenburg}, A., {Efficiency of dynamos
  from autonomous generation of chiral asymmetry}. {\itshape arXiv e-prints},
  2024{\natexlab{b}}, arXiv:2404.07845.

\bibitem[\protect\citeauthoryear{{Sengupta}
  {\itshape{et~al.}}}{2024}]{2024arXiv240215475S}
{Sengupta}, D., {Cuzzi}, J.N., {Umurhan}, O.M. and {Lyra}, W., {Length and
  Velocity Scales in Protoplanetary Disk Turbulence}. {\itshape arXiv
  e-prints}, 2024, arXiv:2402.15475.

\bibitem[\protect\citeauthoryear{{Sharma}
  {\itshape{et~al.}}}{2023}]{2023JCAP...12..042S}
{Sharma}, R., {Dahl}, J., {Brandenburg}, A. and {Hindmarsh}, M., {Shallow relic
  gravitational wave spectrum with acoustic peak}. {\itshape \jcap}, 2023,
  \textbf{2023}, 042.

\bibitem[\protect\citeauthoryear{{V{\"a}is{\"a}l{\"a}}
  {\itshape{et~al.}}}{2023}]{2023ApJ...959...32V}
{V{\"a}is{\"a}l{\"a}}, M.S., {Shang}, H., {Galli}, D., {Lizano}, S. and
  {Krasnopolsky}, R., {Exploring the Formation of Resistive Pseudodisks with
  the GPU Code Astaroth}. {\itshape \apj}, 2023, \textbf{959}, 32.

\bibitem[\protect\citeauthoryear{{Vemareddy}
  {\itshape{et~al.}}}{2024}]{2024RAA....24b5007V}
{Vemareddy}, P., {Warnecke}, J. and {Bourdin}, P.A., {Data-driven Simulations
  of Magnetic Field Evolution in Active Region 11429: Magneto-frictional Method
  Using \textsc{Pencil Code}}. {\itshape Res. Astron. Astrophys.}, 2024,
  \textbf{24}, 025007.

\bibitem[\protect\citeauthoryear{{Zhou}}{2024}]{2024MNRAS.527.3018Z}
{Zhou}, H., {Helical and non-helical large-scale dynamos in thin accretion
  discs}. {\itshape \mnras}, 2024, \textbf{527}, 3018--3028.

\bibitem[\protect\citeauthoryear{{Zhou} and
  {Blackman}}{2024}]{2024PhRvE.109a5206Z}
{Zhou}, H. and {Blackman}, E.G., {Helical dynamo growth and saturation at
  modest versus extreme magnetic Reynolds numbers}. {\itshape \pre}, 2024,
  \textbf{109}, 015206.

\bibitem[\protect\citeauthoryear{{Zhou} and
  {Jingade}}{2024}]{2024arXiv240115860Z}
{Zhou}, H. and {Jingade}, N., {Correlation times of velocity and kinetic
  helicity fluctuations in nonhelical hydrodynamic turbulence}. {\itshape arXiv
  e-prints}, 2024, arXiv:2401.15860.

\end{thebibliography}
