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\begin{center}
{\LARGE \bf PHYS:7730 Example of Annotated Bibliography} \\
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Publications relevant to the study of space physics processes in the laboratory.
\begin{enumerate}
\item \emph{Laboratory measurements of the physics of auroral electron acceleration by \Alfven waves}\\
 Schroeder, J.~W.~R.,  {\bf  Howes, G. G.},  Kletzing, C.~A., Skiff, F., Carter, T.~A., Vincena, S., and Dorfman, S.\\
 Nat. Comm.,  {\bf 12}, 3103 (2021).\\
 \citep{Schroeder:2021}

 This paper describes experimental measurements on the Large Plasma Device (LAPD) at UCLA, in agreement with analytical calculations and numerical modeling, which confirm the hypothesis  that \Alfven waves can accelerate electrons under conditions corresponding to the auroral magnetosphere  \citep{Hasegawa:1976c,Goertz:1979}, settling a long-standing question about the physical mechanisms governing the generation of discrete auroral arcs.  The field-particle correlation technique  \citep{Klein:2016a,Howes:2017a,Klein:2017b} provided the theoretical basis for a definitive confirmation that the \Alfven wave launched in the plasma was responsible for the resonant acceleration of the electrons measured in the experiment.

\item \emph{Measuring Collisionless Damping Using Field-Particle Correlations}\\
 Klein, K.~G. and {\bf Howes, G.~G.} \\
 Astrophys. J. Lett., {\bf 826}, L30 (2016).\\
 \citep{Klein:2016a}

This paper introduced the novel field-particle correlation technique
as a means to assess the particle energization in the weakly
collisional plasma turbulence that plays an important role in
regulating the transport of energy in astrophysical plasmas throughout
the universe.
  
\item \emph{Diagnosing Collisionless Energy Transfer Using Field-Particle Correlations: Vlasov-Poisson Plasmas}\\
   {\bf Howes, G.~G.}, Klein, K.~G., and  Li, T.~C.\\
   J. Plasma Phys., {\bf 83 }, 705830102  (2017). \\
   \citep{Howes:2017a}

This paper provides a detailed derivation of the  field-particle correlation technique, characterizing its advantages and limitations, and shows the results of the technique when applied to explore the Landau damping of Langmuir waves in an electrostatic plasma.

\item \emph{Diagnosing collisionless energy transfer using field-particle correlations: gyrokinetic turbulence}\\
 Klein, K.~G., {\bf Howes, G. G.}, and TenBarge, J.~M.\\
J. Plasma Phys.,   {\bf 83 }, 705830102  (2017). \\
   \citep{Klein:2017b}

This paper provides the first field-particle correlation analysis of gyrokinetic simulations of weakly collisional, astrophysical plasma turbulence, showing definitively that Landau damping plays a role in the dissipation of the turbulence and consequent  heating of the ions in the plasma.

\item \emph{Evidence for electron Landau damping in space plasma turbulence}\\
Chen, C.~H.~K., Klein, K.~G., and {\bf Howes, G.~G.}\\
Nat. Comm.,  {\bf 10}, 740 (2019).\\
   \citep{Chen:2019}

This paper analyzes measurements from NASA's \emph{Magnetospheric Multiscale} mission to provide the first observational identification of a particular mechanism for the dissipation of turbulence in any space plasma, specifically electron Landau damping in the Earth's turbulent magnetosheath plasma.

\item \emph{Toward Astrophysical Turbulence in the Laboratory}\\
{\bf Howes, G. G.}, Drake, D.~J., Nielson, K.~D., Carter, T.~A., Kletzing, C.~A., and Skiff, F. \\
Phys. Rev. Lett., {\bf 109}, 255001  (2012).\\
   \citep{Howes:2012b}

This paper presents experimental results from the Iowa-UCLA collaboration led by Professor Howes that demonstrate for the first time how counterpropagating \Alfven waves can interact nonlinearly and transfer energy to a daughter \Alfven wave with a smaller perpendicular wavelength.  Denoted an ``\Alfven wave collision,'' this nonlinear interaction represents the fundamental building block of astrophysical plasma turbulence.

\item \emph{Alfven Wave Collisions, The Fundamental 
Building Block of Plasma Turbulence I: Asymptotic Solution}\\
{\bf Howes, G.~G.} and  Nielson, K.~D.\\
Phys. Plasmas, {\bf 20}, 072302  (2013).\\
   \citep{Howes:2013a}

This paper presents a detailed asymptotic analytical solution for the
nonlinear evolution of \Alfven wave collisions in the weakly nonlinear limit.

\item \emph{Alfven Wave Collisions, The Fundamental 
Building Block of Plasma Turbulence II: Numerical Solution}\\
Nielson, K. D., {\bf Howes, G. G.} and Dorland, W.\\
Phys. Plasmas, {\bf 20}, 072303  (2013).\\
   \citep{Nielson:2013a}

This paper presents a gyrokinetic numerical simulation that confirms
the analytical solution \citep{Howes:2013a} for the nonlinear evolution
of \Alfven wave collisions.


\item \emph{The Dynamical Generation of Current Sheets in Astrophysical Plasma Turbulence}\\
   {\bf Howes, G.~G.}, \\
   Astrophys. J. Lett., {\bf 827}, L28  (2016).\\
   \citep{Howes:2016b}

This paper shows numerically, and explains theoretically, how  \Alfven wave collisions in the strongly nonlinear limit naturally generate current sheets. The development of current sheets in plasma turbulence has gained a significant amount of attention in recent years \citep{Uritsky:2010,Osman:2011,Zhdankin:2013}, with no previous theoretical explanation for their generation.

\item \emph{Spatially localized particle energization by Landau damping in current sheets produced by strong \Alfven wave collisions}\\
 {\bf Howes, G. G.}, McCubbin, A.~J., and Klein, K.~G.\\
 J. Plasma Phys.,  {\bf 84},  905840105    (2018).\\
   \citep{Howes:2018a}

This paper uses the field-particle correlation technique to show that spatially localized dissipation in the vicinity of current sheets generated by strong \Alfven wave collisions is governed by ion and electron Landau damping.

\end{enumerate}

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