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	These are solar sounds generated from 40 days of Michelson Doppler 
	Imager data and processed by 
	
	A. Kosovichev.  
	 
	The procedure he used for generating these sounds was the following: 
		
			- 
			
			He started with doppler velocity data, averaged over the solar disk, so that 
		only modes of low angular degree (l = 0, 1, 2) remained  
			- 
			
			Subsequent processing 
		removed the spacecraft motion effects, instrument tuning, and some 
		spurious points  
			- 
			
			Then Kosovichev 
		filtered the data at about 3 mHz to select clean sound waves (and not 
		super-granulation and instrumental noise)  
			- 
			
			Finally, he interpolated 
		over the missing data and scaled the data (speeded it up a factor 42,000 
		to bring it into the audible human-hearing range (kHz))  
		 
	 
	
	  
	  
	Listen the Solar Sounds 
	  
	  
		
			
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				One Mode 
				(l=1,n=20, nu=2.94-3.0 
				mHz)  | 
			 
			
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				Three Modes 
				(l=0,n=21, l=1,n=20, 
				l=2,n=20, nu=2.95-3.05 mHz)  | 
			 
			
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				 | 
				
				  All Low-Degree Modes
				(l=0,1,2, and 
				3) | 
			 
		 
	 
	
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