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) |
|