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

 

 

One Mode (l=1,n=20, nu=2.94-3.0 mHz)

Three Modes (l=0,n=21, l=1,n=20, l=2,n=20, nu=2.95-3.05 mHz)

  All Low-Degree Modes (l=0,1,2, and 3)