Cancelling Magnetic Features Associated with EUV Bright Points

S.-Y. Park (Chungnam National University) and J. Chae

Observations have shown that magnetic reconnection may occur frequently in 
the low atmosphere as well as in the solar corona. Most of cancelling magnetic 
features and EUV bright points seem to result from magnetic reconnection in 
the low atmosphere. For better understanding of the process of magnetic 
reconnection, we have studied in detail a cancelling magnetic feature and its 
associated EUV bright point using the data taken  on 2 May 2000 by the MDI  
and EIT onboard SOHO, respectively. In this paper, we will present the results 
on the correlation between the variation of magnetic flux in the cancelling 
magnetic feature and the EUV brightness variation.