Introducing the piggy back noise problem. This is what we saw visually on the 3D gather data. Strong and persistent +- 50 cps waves riding on very low.
Cavities detection with ground penetrating radar in limestone dominated rock formation
HLK RM02 English
T1 task- update Mike Plissi. 2 Collaboration Groups actively involved INFN-VIRGO MAT IGR-Glasgow Groups that have expressed interest INFN-AURIGA CNRS-LKB.
GG 450 April 29, 2008 Reflection Field Methods. 1. Know your goals: What is the target depth? This is probably the most important question for definition.
Introducing the “piggy back” noise problem.
T1 task- update
