Wave reflection and wave disorder in the solar transition zone and corona

Solar Physics ◽  
1978 ◽  
Vol 58 (2) ◽  
pp. 307-318 ◽  
Author(s):  
Donat G. Wentzel
Solar Physics ◽  
1976 ◽  
Vol 50 (1) ◽  
pp. 99-108 ◽  
Author(s):  
D. Vanbeveren ◽  
C. De Loore

1982 ◽  
Vol 259 ◽  
pp. 366 ◽  
Author(s):  
K. P. Dere ◽  
J.-D. F. Bartoe ◽  
G. E. Brueckner

1977 ◽  
Vol 216 ◽  
pp. L119 ◽  
Author(s):  
U. Feldman ◽  
G. A. Doschek

1981 ◽  
Vol 195 (2) ◽  
pp. 107-113 ◽  
Author(s):  
G. A. Doschek ◽  
John T. Mariska ◽  
U. Feldman

Solar Physics ◽  
1978 ◽  
Vol 58 (1) ◽  
pp. 31-36 ◽  
Author(s):  
Edward J. Eadon ◽  
Donald E. Billings

1979 ◽  
Vol 233 ◽  
pp. 741 ◽  
Author(s):  
K. R. Nicolas ◽  
J.-D. F. Bartoe ◽  
G. E. Brueckner ◽  
M. E. Vanhoosier

Solar Physics ◽  
1989 ◽  
Vol 123 (1) ◽  
pp. 41-68 ◽  
Author(s):  
K. P. Dere ◽  
J. -D. F. Bartoe ◽  
G. E. Brueckner

1986 ◽  
Vol 310 ◽  
pp. 456 ◽  
Author(s):  
K. P. Dere ◽  
J.-D. F. Bartoe ◽  
G. E. Brueckner

Geophysics ◽  
1992 ◽  
Vol 57 (1) ◽  
pp. 161-170 ◽  
Author(s):  
N. W. Kim ◽  
A. J. Seriff

Marine shear‐wave reflection methods using the conventional data acquisition system (i.e., source and receiver in water) rely on two mode conversions at the water bottom to produce shear reflections such as PSSP. Some theoretical considerations and the results of a marine check shot survey conducted in the Gulf of Mexico demonstrate that the difficulty in observing PSSP events is attributable to weak P-S and S-P conversion at the bottom in regions with very low shear velocity (a few hundred ft/s or less) sediments at the bottom. For a simple water bottom with a low shear‐wave velocity, water over a uniform half space, the PS conversion factor is proportional to [Formula: see text] and the SP conversion factor is proportional to [Formula: see text], where [Formula: see text] is the bottom shear velocity. For [Formula: see text] their product gives PSSP reflections that can be comparable in amplitude to typical PPPP events. For [Formula: see text], the PSSP events should be about 30 dB weaker and probably not visible. For typical Gulf of Mexico sediments with a shear velocity transition zone several tens of feet thick at the bottom, the situation is even worse, since the velocities start near zero and may not reach 500 ft/s. This condition is common in many areas of recent sedimentations.


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