Skip to content

Commit

Permalink
manuscript edits associated with proof corrections
Browse files Browse the repository at this point in the history
  • Loading branch information
Swanson-Hysell committed Jul 23, 2021
1 parent 263d1c3 commit 615e538
Show file tree
Hide file tree
Showing 3 changed files with 18 additions and 10 deletions.
24 changes: 16 additions & 8 deletions Manuscript/Laurentia_Paleogeo_Manuscript.bbl
Original file line number Diff line number Diff line change
@@ -1,4 +1,4 @@
\begin{thebibliography}{305}
\begin{thebibliography}{306}
\providecommand{\natexlab}[1]{#1}
\providecommand{\url}[1]{\texttt{#1}}
\providecommand{\urlprefix}{URL }
Expand Down Expand Up @@ -1310,14 +1310,22 @@ Park, J.~K., Irving, E., and Donaldson, J.~A., 1973. {Paleomagnetism of the
Precambrian Dubawnt Group}. Geological Society of America Bulletin, v.~84, p.
859--870, \doi{10.1130/0016-7606(1973)84<859:potpdg>2.0.co;2}.

\bibitem[{Park et~al.(2021)Park, Swanson-Hysell, Macdonald, and
\bibitem[{Park et~al.(2021{\natexlab{a}})Park, Swanson-Hysell, Macdonald, and
Lisiecki}]{Park2021a}
Park, Y., Swanson-Hysell, N., Macdonald, F., and Lisiecki, L., 2021, Evaluating
the relationship between the area and latitude of large igneous provinces and
earth's long-term climate state. \emph{In} Ernst, R.~E., Dickson, A.~J., and
Bekker, A., eds., Large Igneous Provinces: A Driver of Global Environmental
and Biotic Changes, Geophysical Monograph 255, American Geophysical Union,
\doi{10.1002/9781119507444.ch7}.
Park, Y., Swanson-Hysell, N., Macdonald, F., and Lisiecki, L.,
2021{\natexlab{a}}, Evaluating the relationship between the area and latitude
of large igneous provinces and earth's long-term climate state. \emph{In}
Ernst, R.~E., Dickson, A.~J., and Bekker, A., eds., Large Igneous Provinces:
A Driver of Global Environmental and Biotic Changes, Geophysical Monograph
255, American Geophysical Union, \doi{10.1002/9781119507444.ch7}.

\bibitem[{Park et~al.(2021{\natexlab{b}})Park, Swanson-Hysell, Xian, Zhang,
Condon, Fu, and Macdonald}]{Park2021b}
Park, Y., Swanson-Hysell, N.~L., Xian, H., Zhang, S., Condon, D.~J., Fu, H.,
and Macdonald, F.~A., 2021{\natexlab{b}}. {A consistently high latitude South
China from 820 to 780 Ma: Implications for exclusion from Rodinia and the
feasibility of large-scale true polar wander}. Journal of Geophysical
Research: Solid Earth, v. 126, \doi{10.1029/2020jb021541}.

\bibitem[{Patchett et~al.(1978)Patchett, Bylund, and Upton}]{Patchett1978a}
Patchett, P., Bylund, G., and Upton, B., 1978. {Palaeomagnetism and the
Expand Down
Binary file modified Manuscript/Laurentia_Paleogeo_Manuscript.pdf
Binary file not shown.
4 changes: 2 additions & 2 deletions Manuscript/Laurentia_Paleogeo_Manuscript.tex
Original file line number Diff line number Diff line change
Expand Up @@ -288,7 +288,7 @@ \subsubsection{Paleogeographic connections prior to initial Laurentia assembly}
\begin{figure*}
\centering
\includegraphics[width=\textwidth]{../Figures/Fig8_Rodinia_Reconstruction.pdf}
\caption{\textbf{Paleogeographic reconstructions of Laurentia and other select conjugate Proterozoic continents leading up to Rodinia assembly in the late Mesoproterozoic and to its initial break-up in the Neoproterozoic}. The hypothesized connection between Siberia and Laurentia is implemented following \cite{Evans2016b} who interpret this relationship as persistent from 1.7 to 0.7 Ga. The reconstruction of North China to Laurentia follows \cite{Ding2021a}. The reconstruction implements Kalahari and Amazonia cratons as conjugates with Laurentia in the Grenvillian orogeny \citep{Hoffman1991a}. The Australia-East Antarctica relationship with Laurentia follows \cite{Swanson-Hysell2012a} and is similar to the Neoproterozoic reconstruction between the continents of \cite{Li2011a} and implementing their relative rotation of North Australia relative to South and West Australia. This configuration back to ca. 1140 Ma is consistent with a comparison between the Laurentia poles of that age and the coeval Mt. Isa dikes pole from North Australia and with the Keweenawan Track if the the Nonesuch and Freda poles are interpreted to be ca. 1080 (consistent with chronostratigraphic constraints; \citealp{Slotznick2018b}) with further motion by ca. 1070 Ma. The time slices show the rapid motion of Laurentia implied by the paleomagnetic poles which is consistent with the timing of collisional orogenesis associated with the Grenvillian orogeny. The assembled Rodinia persisted until initial rifting ca. 775 Ma with episodic rifting continuing until ca. 530 Ma.}
\caption{\textbf{Paleogeographic reconstructions of Laurentia and other select conjugate Proterozoic continents leading up to Rodinia assembly in the late Mesoproterozoic and to its initial break-up in the Neoproterozoic}. The hypothesized connection between Siberia and Laurentia is implemented following \cite{Evans2016b} who interpret this relationship as persistent from 1.7 to 0.7 Ga. The reconstruction of North China to Laurentia follows \cite{Ding2021a}. The omission of South China from Rodinia follows ​\cite{Park2021b}​. The reconstruction implements Kalahari and Amazonia cratons as conjugates with Laurentia in the Grenvillian orogeny \citep{Hoffman1991a}. The Australia-East Antarctica relationship with Laurentia follows \cite{Swanson-Hysell2012a} and is similar to the Neoproterozoic reconstruction between the continents of \cite{Li2011a} and implementing their relative rotation of North Australia relative to South and West Australia. This configuration back to ca. 1140 Ma is consistent with a comparison between the Laurentia poles of that age and the coeval Mt. Isa dikes pole from North Australia and with the Keweenawan Track if the the Nonesuch and Freda poles are interpreted to be ca. 1080 (consistent with chronostratigraphic constraints; \citealp{Slotznick2018b}) with further motion by ca. 1070 Ma. The time slices show the rapid motion of Laurentia implied by the paleomagnetic poles which is consistent with the timing of collisional orogenesis associated with the Grenvillian orogeny. The assembled Rodinia persisted until initial rifting ca. 775 Ma with episodic rifting continuing until ca. 530 Ma.}
\label{fig:Grenville_reconstructions}
\end{figure*}

Expand Down Expand Up @@ -355,7 +355,7 @@ \subsection{Conclusion}
%%%%%%%%%%%%% Acknowledgements %%%%%%%%%%%%%
\footnotesize
\subsection*{Acknowledgements}
This work was supported by NSF CAREER Grant EAR-1847277. The manuscript benefited from reviews from Athena Eyster, David Evans, and Lauri Pesonen as well as discussions and manuscript feedback from Francis Macdonald, Yuem Park, Toby Rivers, Sarah Slotznick, Justin Strauss, and Yiming Zhang. Bruce Buffett provided insights on the implications of a stagnant lid regime for the generation of the geomagnetic field. Many participants in the Nordic Paleomagnetism Workshop have contributed to the compilation and evaluation of the pole list utilized herein. Particular acknowledgement goes to David Evans for maintaining and distributing the compiled pole lists. GPlates, and in particular the pyGPlates API, was utilized in this work \citep{Muller2018b}. Figures were made using Matplotlib \citep{Hunter2007a} in conjunction with cartopy \citep{Met-Office2010a} and pmagpy \citep{Tauxe2016a} within an interactive Python environment \citep{Perez2007a}. The chapter text as well as code, data, and reconstructions used in this paper are openly available and licensed for any form of reuse with attribution (CC BY 4.0) in this repository: \url{https://github.com/Swanson-Hysell-Group/Laurentia_Paleogeography} which is also archived on Zenodo.
This work was supported by NSF CAREER Grant EAR-1847277. The manuscript benefited from reviews from Athena Eyster, David Evans, and Lauri Pesonen as well as discussions and manuscript feedback from Francis Macdonald, Yuem Park, Toby Rivers, Sarah Slotznick, Justin Strauss, and Yiming Zhang. Bruce Buffett provided insights on the implications of a stagnant lid regime for the generation of the geomagnetic field. Many participants in the Nordic Paleomagnetism Workshop have contributed to the compilation and evaluation of the pole list utilized herein. Particular acknowledgement goes to David Evans for maintaining and distributing the compiled pole lists. GPlates, and in particular the pyGPlates API, was utilized in this work \citep{Muller2018b}. Figures were made using Matplotlib \citep{Hunter2007a} in conjunction with cartopy \citep{Met-Office2010a} and pmagpy \citep{Tauxe2016a} within an interactive Python environment \citep{Perez2007a}. The chapter text as well as code, data, and reconstructions used in this paper are openly available and licensed for any form of reuse with attribution (CC BY 4.0) in this repository: \url{https://github.com/Swanson-Hysell-Group/Laurentia_Paleogeography} which is also archived on Zenodo (https://doi.org/10.5281/zenodo.5129624).

\printendnotes

Expand Down

0 comments on commit 615e538

Please sign in to comment.