标题：The Coronal Global Evolutionary Model: Using HMI Vector Magnetogram and Doppler Data to Model the Buildup of Free Magnetic Energy in the Solar Corona
摘要：Acknowledgments This work is supported by NSF and NASA through grants AGS-1321474, NNX13AJ96G, and NNX13AK39G to UC Berkeley, Lockheed Martin, and Stanford University. We thank the U.S. taxpayers for their support. We thank the anonymous referees for improving the readability and accuracy of this paper. The input data used for CGEM are available from NASA's JSOC website http://jsoc.stanford.edu/, and the output data from CGEM will be made available as a part of the project.
