Paul_Wright_AcademicCV_1page.tex

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%%%%%%%%%%%%%%%%%%%%%%%%% Begin CV Document %%%%%%%%%%%%%%%%%%%%%%%%%%%%

\begin{document}
\makeheading{Paul James Wright}

\section{Contact Information}

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{-- ------ ----- \hfill Mobile: +44 (0)---- ------ \\
-----, ---- \hfill{Web: \href{http://www.pauljwright.co.uk}{www.pauljwright.co.uk}} \\ 
---- --- \hfill{Email: paul@pauljwright.co.uk} \\ 
United Kingdom \hfill{Publication List: \href{https://ui.adsabs.harvard.edu/#search/q=orcid\%3A0000-0001-9021-611X&sort=date+desc}{SAO/NASA ADS}}}

%\hfill{GitHub: \href{http://www.github.com/pauljwright}{www.github.com/pauljwright}} }


%\end{tabular}

%%
%% In modern CV's, it seems like ``Objective'' is frowned upon. Instead,
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%% information'' can go at the end of the CV, but it should not distract
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% Placement in an academic position (i.e., faculty, postdoctoral, or
% research scientist) that allows for advanced research in distributed
% complex adaptive systems (i.e., modeling, analysis, design, and
% verification) with a particular focus on the control of engineered
% agents (e.g., for communications, control, software, electronics, and
% sustainability) and the analysis of biological phenomena (e.g.,
% self-organization, ecological rationality)
% \begin{innerlist}
% \item More information and auxiliary documents can be found at\\\url{http://www.tedpavlic.com/facjobsearch/}
% \end{innerlist}

%\section{Research Summary}

%My interests range from stellar to solar physics; my main interests lie in the heating of the solar atmosphere, including active regions and loops. I have expertise in the analysis of spectroscopic and narrowband Extreme Ultra-Violet (EUV) and X-ray data from the {\it Solar Dynamics Observatory} and {\it Hinode}, in addition to the hard X-ray (HXR) observations from {\it NuSTAR}'s heliophysics campaign. I am currently using a hydrodynamics code (Enthalpy-Based Thermal Evolution of Loop, EBTEL) to model light curves from coronal loops. I am particularly interested in the weak bremsstrahlung emission, with a view to understanding the requirements for future X-ray instrumentation to study the coronal heating problem.

%My research interests range from solar to stellar physics, with the majority of my research concentrating on the heating of the solar corona. I have expertise in the analysis of spectroscopic and narrowband Extreme Ultra-Violet (EUV) and X-ray data from the {\it Solar Dynamics Observatory} and {\it Hinode}, in addition to the hard X-ray (HXR) observations from {\it NuSTAR}'s heliophysics campaign. I am currently using a hydrodynamics code (Enthalpy-Based Thermal Evolution of Loops, EBTEL) to model light curves from coronal loops. In particular, I am interested in the weak bremsstrahlung emission, with a view to understanding the requirements for future X-ray instrumentation to study the coronal heating problem.


%My research interests are in the fields of solar and stellar flares, and my Ph.D. research has concentrated on one of the unsolved questions in Heliophysics -- the coronal heating problem. I have expertise of image and spectroscopic data analysis from EUV and X-ray data from the {\it Solar Dynamics Observatory} and {\it Hinode} in addition to expertise in analysing the hard X-ray data obtained during {\it NuSTAR}'s heliophysics campaign, and observations of stellar flares observed by {\it Kepler}. I am also currently using a hydrodynamics code (Enthalpy-Based Thermal Evolution of Loops, EBTEL) to model light curves from coronal loops. %%% --- 17th March

%My research interests are in solar and stellar physics, and my Ph.D. research has concentrated on one of the unsolved problems in Heliophysics---the coronal heating problem. During my Ph.D. I have gained expertise in numerous time-series analysis techniques and methods for recovering the differential emission measure (an ill-posed inverse problem) from a wide range of spectroscopic and narrowband data. I am a member of the {\it NuSTAR} Heliophysics working group and I led the analysis of the first solar flare observed by the {\it NuSTAR} hard X-ray {\it astrophysics} imaging spectrometer. I have also developed a stellar flare detection algorithm based on the observations obtained by the {\it Kepler} space telescope to determine the superflare rate of the Sun.


%My research interests range from solar to stellar physics with the majority of my Ph.D. research concentrating on the heating of the solar corona. I have expertise in the analysis of spectroscopic and narrowband Extreme Ultra-Violet (EUV) and X-ray data from the {\it Solar Dynamics Observatory} and {\it Hinode}, in addition to the hard X-ray (HXR) observations from {\it NuSTAR}'s heliophysics campaign, and white-light observations from {\it Kepler}. I am also currently using a hydrodynamics code (Enthalpy-Based Thermal Evolution of Loops, EBTEL) to model light curves from coronal loops.


%My interests range from stellar to solar physics; my main interests lie in the heating of the solar atmosphere, including active regions and loops. I have expertise in the analysis of Extreme Ultra-Violet (EUV) and X-ray data from the {\it SDO}, and {\it Hinode} satellites, in addition to the hard X-ray (HXR) imaging/spectroscopic observations from \textit{NuSTAR}'s heliophysics campaign. Furthermore, I am currently modelling coronal light-curves using the \texttt{EBTEL} (Enthalpy-Based Thermal Evolution of Loops) hydrodynamics code with particular interest in the weak bremmstrahlung components.

%My interests range from stellar to solar physics; my main interests lie in the heating of the solar atmosphere, including active regions and loops. I have expertise in analysis of data from \textit{Kepler}, \textit{SDO}/AIA, \textit{Hinode}/EIS, \textit{Hinode}/XRT, and \textit{NuSTAR}'s heliophysics observations. In addition, I am currently modelling coronal light-curves using the \texttt{EBTEL} (Enthalpy-Based Thermal Evolution of Loops) hydrodynamics code.

%%%% EDUCATION %%%%
\section{Education}

\href{http://www.gla.ac.uk/}{\textbf{University of Glasgow}},
Glasgow, UK \hfill {10/2014 -- 04/2019}
\begin{innerlist}
\item[] Ph.D.
        \href{}
             {Solar Physics}
        \begin{innerlist}
        \item[] Thesis Title: \emph{The Energetics of Small Solar Flares and Brightenings}
        \item[] Advisers: Dr Iain G. Hannah, Dr Alexander MacKinnon
        \end{innerlist}

\end{innerlist}

%\halfblankline

\href{http://www.soton.ac.uk/}{\textbf{University of Southampton}},
Southampton, UK \hfill {10/2010 -- 06/2014}
\begin{innerlist}
\item[] MPhys
        \href{http://www.phys.soton.ac.uk/programmes/f3fm-mphys-astronomy-year-abroad-4-yrs/}
             {Astrophysics with a year abroad}
        \begin{innerlist}
        	   \item[] First-class honours (1:1)
%        \end{innerlist}
%\end{innerlist}
%
%\href{https://www.cfa.harvard.edu/}{\textbf{Smithsonian Astrophysical Observatory}},
%Cambridge, MA, USA 
%\hfill {10/2013 -- 06/2014}
%\begin{innerlist}
%\item[] MPhys
%        \href{http://www.phys.soton.ac.uk/programmes/f3fm-mphys-astronomy-year-abroad-4-yrs/}
%             {Astrophysics with a year abroad}
%        \begin{innerlist}
        \item[] Thesis Title: \emph{The Superflare Rates of Solar-Like Stars}
        \item[] Advisers: Dr Steven H. Saar, Dr Jeremy J. Drake
        \end{innerlist}
\end{innerlist}

\section{Current Appointments}

\textbf{Postdoctoral Research Fellow},
            \href{http://www.stanford.edu}{Stanford University}
            \hfill {06/2019 -- }
\begin{innerlist}
    \item[] \href{http://hepl.stanford.edu/}{W. W. Hansen Experimental Physics Laboratory}
\end{innerlist}

%\halfblankline

\textbf{Mentor},
            \href{http://www.frontierdevelopmentlab.org/}{NASA Frontier Development Lab (FDL)}
            \hfill {06/2019 -- }
\begin{innerlist}
\item[] \href{http://seti.org/}{SETI Institute}/\href{}{NASA Ames Research Center, Mountain View, CA}
    \begin{innerlist}
    \item[] Project: {\it Super-resolution magnetograms}
\end{innerlist}            
\end{innerlist}            

\section{Selected Previous Appointments}
\textbf{Affiliate Staff Member},
            \href{http://www.gla.ac.uk/}{University of Glasgow}
            \hfill {10/2017 -- 04/2019}
\begin{innerlist}
\begin{innerlist}
  	\item{} Used the EBTEL hydrodynamics code to model light curves from coronal loops. The parameter space of these simulations will be constrained by observations obtained during the {\it NuSTAR} heliophysics campaign, and to test a variety of coronal analysis techniques.
\end{innerlist}
\end{innerlist}
%\halfblankline

\textbf{Researcher},
            \href{http://www.frontierdevelopmentlab.org/}{NASA Frontier Development Lab (FDL)}
            \hfill {06/2018 - 08/2018}
    	   \begin{innerlist} 
%    	\item[] \href{http://seti.org/}{SETI Institute}/\href{}{NASA Ames Research Center, Mountain View, CA}
  	    \begin{innerlist}
  	    \item{} Predicted MEGS-A Solar Spectral Irradiance (SSI) with median absolute relative uncertainties of less than $1.6\%$ per emission line using a Convolutional Neural Network (CNN) augmented with a Multi-Layer Perceptron (MLP).
  	\item{} Used a 1x1 CNN to improve the computational speed ($10^{3}\times$ increase) for differential emission measure (DEM) inversion. 
    	   \end{innerlist}
    	   \end{innerlist}

%\halfblankline
    
\textbf{Post-Graduate Research Assistant},
            \href{http://www.gla.ac.uk/}{University of Glasgow}
            \hfill {10/2014 -- 07/2017}
\begin{innerlist}
%    \item[] \href{http://www.astro.gla.ac.uk/}{SUPA School of Physics and Astronomy}
    \begin{innerlist}
    	    	\item{} Analysed observations of the Sun with {\it NuSTAR}, a telescope not designed for heliophysics. These observations are the most sensitive of their kind and have resulted in numerous, wide-ranging, highly-collaborative peer-reviewed publications.
    	    	    	\item{} Studied the temperature distribution of the solar atmosphere through the recovery of an ill-posed inverse problem (the differential emission measure, DEM) using techniques such as Tikhonov regularisation, Markov-chain Monte Carlo, Spline fitting, and Sparse Inversion (by Basis Pursuit).
    \end{innerlist}
\end{innerlist}

%\halfblankline

\textbf{Visiting Researcher}, \href{https://www.nasa.gov/goddard}{NASA Goddard Space Flight Center (GSFC)} 
\hfill {04/2016}
\begin{innerlist}\begin{innerlist}
    	\item{} Explored the possibility of implementing DEM maps in the \href{www.helioviewer.org}{Helioviewer} project, and their usefulness as an input for various established time-series analysis techniques.
    	\end{innerlist}\end{innerlist}
    	
%\halfblankline
    	
\textbf{Research Scholar},
\href{https://www.cfa.harvard.edu/}{Center for Astrophysics | Harvard \& Smithsonian} 
\hfill {10/2013 -- 06/2014}
\begin{innerlist}\begin{innerlist}
    	\item{} Designed and implemented a sophisticated stellar flare detection routine for long-cadence (30 mins) {\it Kepler} data obtained from a proprietary set of spectroscopically verified solar-type stars in three open clusters: this work had coverage by \href{http://www.sciencemag.org/news/2015/08/when-sun-s-next-superflare-due?rss=1}{Science} and \href{http://www.smithsonianmag.com/smart-news/when-next-solar-superflare-hit-earth-180956288/}{the Smithsonian}. % Magazine}.
    	\end{innerlist}\end{innerlist}
%
%\textbf{Summer Research Intern},
%\href{http://www.soton.ac.uk/}{University of Southampton} 
%\hfill {07/2013}

\section{Memberships}
     \href{https://www.nustar.caltech.edu/page/sun}{\textbf{\textit{NuSTAR} Heliophysics Working Group}}, Member \hfill {2015 -- present} \\
     \href{https://www.ras.org.uk/}{\textbf{Royal Astronomical Society}}, RAS Fellow \hfill {2014 -- present} \\
     \href{http://www.issibern.ch/}{\textbf{International Space Science Institute (ISSI)}}, Young Scientist Member \hfill {2015 -- 2018}
    \begin{innerlist}
     \item[] Member of Paola Testa's ISSI Team: \href{http://helio.cfa.harvard.edu/ISSI/welcome_pt.html}{\textit{New Diagnostics of Particle Acceleration in Solar Coronal Nanoflares from Chromospheric Observations and Modelling}}
    \end{innerlist}
% 
%\section{Technical Skills:} {\it Computing:} IDL (5+ years), Python (2+ years), PyTorch, R, Bash, $\LaTeX$, PyCharm, IRAF, git (GitHub, Gitlab), Microsoft Office, Adobe Creative Cloud, Linux/Unix, Mac OSX%, Microsoft Windows
%
%%\halfblankline
%
%{\it General:} Data Analysis, Data Visualisation, Interdisciplinary Collaboration, Public Speaking, Teaching, Writing (Technical \& Lay) 
%
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\newpage
\makeheading{Paul James Wright \hfill {List of Publications}} 

\section{Refereed Journal Publications}
\begin{bibenum}
	\item{} Marsh, A.~J., Smith, D.~M., Glesener, L. \textit{et al} 2017. {\it First NuSTAR Limits on Quiet Sun Hard X-Ray Transient Events}, \MYhref[magenta]{https://doi.org/10.3847/1538-4357/aa9122}{{\it ApJ}}, \href{https://ui.adsabs.harvard.edu/?#abs/2017ApJ...849..131M}{849, 131}
	\item{} Wang, J., Sim{\~o}es, P.~J.~A., Jeffrey, N.~L.~S. \textit{et al} 2017. {\it Observations of Reconnection Flows in a Flare on The Solar Disk}, \MYhref[magenta]{https://doi.org/10.3847/2041-8213/aa8904}{{\it ApJL}}, \href{http://adsabs.harvard.edu/abs/2017arXiv170808706W}{847, L1}
	\item{} {\bf Wright, P. J.}, Hannah, I.~G., Grefenstette, B. W., \textit{et al} 2017. {\it Microflare Heating of a Solar Active Region Observed with {\it NuSTAR}, {\it Hinode}/XRT, and {\it SDO}/AIA}, \MYhref[magenta]{https://doi.org/10.3847/1538-4357/aa7a59}{{\it ApJ}}, \href{http://adsabs.harvard.edu/abs/2017ApJ...844..132W}{844, 132}
	\item{} Kuhar, M., Krucker, S., Hannah, I. G., \textit{et al} 2017. {\it Evidence of Significant Energy Input in the Late Phase of a Solar Flare from NuSTAR X-ray Observations}, \MYhref[magenta]{http://doi:10.3847/1538-4357/835/1/6}{{\it ApJ}}, \href{http://adsabs.harvard.edu/abs/2017ApJ...835....6K}{835, 6}
	\item{} Galvez, R., Fouhey, D. F., Jin, M., \textit{et al} 2019. {\it A Machine Learning Dataset Prepared From the NASA Solar Dynamics Observatory Mission}, \MYhref[magenta]{http://doi:10.3847/1538-4357/835/1/6}{{\it ApJS}}, \href{https://iopscience.iop.org/article/10.3847/1538-4365/ab1005}{242, 7}	
\end{bibenum}

\section{Book Chapters}
\begin{bibenum}
 	\item{} {\bf Wright, P. J.}, Cheung, M.~C.~M., Thomas, R., \textit{et al} 2018 {\it DeepEM: A Deep Learning Approach to DEM Inversion}. In M. Bobra \& J. Mason, eds., {\it Machine Learning, Statistics, and Data Mining for Heliophysics}, \href{https://helioml.github.io/HelioML/}{Chapter 4}
\end{bibenum}

\section{First Author Publications in Preparation (Working Titles)}
\begin{bibenum}
 	\item{} {\bf Wright, P. J.}, Galvez, R., \textit{et al} 2019. {\it DeepEM: A Deep Learning Approach to DEM Inversion}
% 	\item{} {\bf Wright, P. J.}, MacKinnon, A., Hannah, I.~G., and Sim{\~o}es, P.~J.~A. 2019. {\it Local Intermittency Measure: The Application to Active Region Light Curves}
	\item{} {\bf Wright, P. J.}, Hannah, I.~G., Viall, N.~M., \textit{et al} 2019. {\it The Thermal Time Evolution of Active Regions Determined by SDO/AIA}
	\item{} {\bf Wright, P. J.}, Saar, S.~H., Meibom, S., \textit{et al} 2019. {\it  The Age-Dependent Superflare Rates of G-Type Dwarfs In Three {\it Kepler} Clusters}
%	\item{} {\bf Wright, P. J.}, Saar, S.~H., Meibom, S., \textit{et al} 2019. {\it An Extension of The Age-Dependent Superflare Rates to F- and K-Type Dwarfs}
\end{bibenum}

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