\relax 
\@writefile{toc}{\contentsline {section}{\numberline {1}Near Infrared System}{1}}
\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces Sunspot observed in the infrared at 1.56\nobreakspace  {}$\mu $m on August 8th, 1998.}}{2}}
\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces Stokes V image depicting the line-of-sight magnetic field in an active region with the Fe line pairs at 1.56\nobreakspace  {}$\mu $m.}}{3}}
\@writefile{toc}{\contentsline {section}{\numberline {2}Correlation Tracker}{3}}
\@writefile{toc}{\contentsline {section}{\numberline {3}New Visible-Light Magnetograph System}{4}}
\@writefile{lof}{\contentsline {figure}{\numberline {3}{\ignorespaces (a) Quiet sun magnetogram (400 integrations) of the solar disk center, obtained on March 17th, 1997. (b) Magnetogram resulting from a single pair subtraction to demonstrate noise and sensitivity. The field of view is to $256^{\prime \prime } \times 256^{\prime \prime }$.}}{5}}
\@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces (a) Granulation observed at disk center and (b) a samll sunspot observed in the G-band at 430.6\nobreakspace  {}nm with SMD CCD camera on September 11th, 1998. The field of view is approximately $90^{\prime \prime } \times 90^{\prime \prime }$ and the exposure time is 8\nobreakspace  {}ms.}}{5}}