|  | 
	
		|  |  
		| Paper: | Physical Conditions in a CME from Hinode, STEREO, and SOHO Observations |  
		| Volume: | 428, SOHO-23: Understanding a Peculiar Solar Minimum |  
		| Page: | 201 |  
		| Authors: | Landi, E.; Raymond, J. C.; Miralles, M. P.; Hara, H. |  
		| Abstract: | In the present work we analyze multiwavelength observations from Hinode, SOHO, and STEREO of the early phases of a CME. We use EIS, UVCS, and XRT to measure the physical properties of the CME ejecta as a function of time at 1.1 and 1.9 Rsun. EUVI, COR 1, EIT, and LASCO images are used to measure the CME trajectory, velocity, and acceleration in 3D up to 5 Rsun. The diagnostic results are used to determine the energy budget of the CME plasma and the heating rate, and to compare it to theoretical predictions. |  
		|  |  
		|  |  |  |