School/phy-4660
1
0
Fork 0
mirror of https://asciireactor.com/otho/phy-4660.git synced 2024-11-22 10:05:06 +00:00
Code Issues Packages Projects Releases Wiki Activity

images

Browse Source
This commit is contained in:
caes 2017-03-22 03:30:45 -04:00
parent bb0998fce4
commit f873d5e5d3
2 changed files with 2 additions and 2 deletions
Show Stats Download Patch File Download Diff File Expand all files Collapse all files

0
accelerator/collision.png → accelerator/report/collision.png
View File

Side by Side Swipe Overlay

Before

Width:  |  Height:  |  Size: 21 KiB

After

Width:  |  Height:  |  Size: 21 KiB

4
accelerator/report/report.tex
View File

@ -56,7 +56,7 @@
\begin{figure} \begin{figure}
\center \center
\includegraphics[width=4.5in]{../abundances.png} \includegraphics[width=4.5in]{abundances.png}
\caption{Relative elemental abundances in the sun's photosphere. Lithium and fluorine are much less abundant than their neighbour elements. It is thought this is due to large probability cross-sections for a proton collision with these nuclei. \cite{Carroll&Ostlie}} \caption{Relative elemental abundances in the sun's photosphere. Lithium and fluorine are much less abundant than their neighbour elements. It is thought this is due to large probability cross-sections for a proton collision with these nuclei. \cite{Carroll&Ostlie}}
\label{fig:abundances} \label{fig:abundances}
\end{figure} \end{figure}
@ -72,7 +72,7 @@
\begin{figure} \begin{figure}
\center \center
\includegraphics{} \includegraphics[width=4.5in]{detector.jpg}
\end{figure} \end{figure}