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Raw Data /net/kana/data/fun/solar/solar.HH
Velocity Model /net/kana/data/fun/solar/solarvel.HH
Usage Passive seismology
(); Unsolved challenge: can you image the
sides/bottom of the sunspot?? Try cross-correlation plus turning
ray-migration.
Geometry
114 skye% In solar.HH
solar.HH:
in="stdin"
expands to in="stdin"
esize=4
n1=256 n2=256 n3=512 n4=1 33554432 elem 134217728 bytes
d1=0.8248 d2=0.8248 d3=0.06 d4=1
o1=0 o2=0 o3=0 o4=0
label1=distance (Mm)
label2=distance (Mm)
label3=time (ks)
Problem
History of Data Given to us by Tom Duvall and
Sasha Kosovichev in the solar physics department at Stanford.
Preprocessing Projection to tangent plane
Proprietary Considerations None, but for courtesy acknowledge
the Solar Oscillations Investigation team (
http://soi.stanford.edu) and/or reference ().
shortcube
Figure 1 Oscillation data
solarvel
Figure 2 Velocity model (note: better check units).
Next: vaillant: REFERENCESSEG-EAGE salt
Up: Vaillant: STANFORD EXPLORATION PROJECTElf
Previous: Rickett: REFERENCESSOHO/MDI solar oscillations
Stanford Exploration Project
1/15/2002