# Read e-book online A Search for an Einstein Relativity-Gravitational Effect in PDF

By St. John C.E.

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NOTES You can select both seismic and auxiliary traces. The Uphole trace is not available. Click APPLY to save and activate your settings. (Clicking OK does the same and also closes the window). 0311386 5-16 Issue : June 1999 OPERATING INSTRUCTIONS PLOT OPTIONS SETUP (Test window) PLOT OPTIONS SETUP (Test window) Selecting SETUP from the menu bar in a Test SQC-PRO window opens a dialog box that allows you to choose the following options for the trace display: If you choose this option, the same gain is applied to all traces.

Close the dialog box. - Select "SHUTDOWN" (mouse right button). - Select "Quit Mwm" (mouse left button). 2 - When the prompt “OK” appears, type boot -r (

Metres/second, see NOTE below) This text box is used to specify the quadratic velocity (Vrms) of the analysis window. The RMS velocity is the assumed mean propagation velocity of the wave through the different layers deep in the ground and back to the surface. This determines a hyperbolic window. The time (t) of the first sample to be processed is given by the formula: t = (metres/second) This text box is used to specify the assumed velocity of the First Break (i. e. the wave propagation velocity through near-surface ground).

### A Search for an Einstein Relativity-Gravitational Effect in the Sun (1917)(en)(3s) by St. John C.E.

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