Detecting physical variables of am herculis by optical region photometric analysis results

In this study period analysis of Am Herculis cataclysmic variable star was applied by String-Length method, which is performed as an web application. The data of light curves was obtained from the observations of the AM Herculis star which was performed by Ulupınar Observatory in 25-26 June 2012 and TUBITAK National Observatory in 02-24-25 and 26 May 2014. Also same method was applied on some AAVSO data. All analysis results are compared each other. It was seen that the obtained period values of light curves is not high accuracy results. However, results can be obtained in short time by the application. The orbital period of Am Herculis was seen in most results. The diffrence of objects of Am Herculis also can be seen in results.