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solar
Figure 9. Raw seismic data on the sun (left). Impulse response of the sun (right) derived by Helix-Kolmogoroff spectral factorization. |
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Solar physicists have learned how to measure the seismic field of the sun surface. If you created an impulsive explosion on the surface of the sun, what would the response be? James Rickett and I applied the helix idea along with Kolmogoroff spectral factorization to find the impulse response of the sun. Figure 9 shows a raw data cube and the derived impulse response. The sun is huge so the distance scale is in megameters (Mm). The United States is 5 Mm wide. Vertical motion of the sun is measured with a video-camera like device that measures vertical motion by doppler shift. From an acoustic/seismic point of view, the surface of the sun is a very noisy place. The figure shows time in kiloseconds (Ks). We see about 15 cycles in 5 Ks which is 1 cycle in about 333 sec. Thus the sun seems to oscillate vertically with about a 5 minute period. The top plane of the raw data in Figure 9 (left panel) happens to have a sun spot in the center. The data analysis here is not affected by the sun spot so please ignore it.
The first step of the data processing is
to transform the raw data to its spectrum.
With the helix assumption, computing the spectrum is
virtually the same thing in 1-D space as in 3-D space.
The resulting spectrum was passed to Kolmogoroff spectral factorization code.
The resulting impulse response is on the right side of
Figure 9.
The plane we see on the right top is not lag time
;
it is lag time
Ks.
It shows circular rings, as ripples on a pond.
Later lag times (not shown) would be the larger circles of expanding waves.
The front and side planes show tent-like shapes.
The slope of the tent gives the (inverse) velocity of the wave
(as seen on the surface of the sun).
The horizontal velocity we see on the sun surface turns out
(by Snell's law)
to be the same as that at the bottom of the ray.
On the front face at early times we see the low velocity (steep) wavefronts
and at later times we see the faster waves.
This is because the later arrivals reach more deeply into the sun.
Look carefully, and you can see two (or even three!) tents inside one another.
These ``inside tents'' are the waves that have bounced once (or more!)
from the surface of the sun.
When a ray goes down and back up to the sun surface,
it reflects and takes off again with the same ray shape.
The result is that a given slope on the traveltime curve
can be found again at twice the distance at twice the time.
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The helical coordinate |