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Geology 5660/6660 Applied Geophysics 29 Feb 2016 © A.R. Lowry 2016 Last Time: Ground Penetrating Radar (GPR) Radar = electromagnetic radiation (light)

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Presentation on theme: "Geology 5660/6660 Applied Geophysics 29 Feb 2016 © A.R. Lowry 2016 Last Time: Ground Penetrating Radar (GPR) Radar = electromagnetic radiation (light)"— Presentation transcript:

1 Geology 5660/6660 Applied Geophysics 29 Feb 2016 © A.R. Lowry 2016 Last Time: Ground Penetrating Radar (GPR) Radar = electromagnetic radiation (light) in the 50-1000 MHz (radio) frequency band  Governed by wave equation (  similar to seismic!)  Source & receiver are dipole antennae  Signal is a single pulse  Processing & display analogous to seismic section  High frequency  high resolution (but also)  High attenuation  Images changes in electromagnetic impedance Z For Wed 2 Mar: Burger 349-378 (§6.1-6.4)

2 Last Time: Ground Penetrating Radar (GPR) Velocity (usually) is not estimated; emphasis is mostly on the the imaging of structure rather than physical properties. Instead TWTT  depth is approximated from rough ~ V Radar reflections image variations in dielectric constant  r ( = relative permittivity )  3-40 for most Earth materials;  higher when H 2 O &/or clay present Geology 5660/6660 Applied Geophysics 29 Feb 2016 © A.R. Lowry 2016 For Wed 2 Mar: Burger 349-378 (§6.1-6.4)

3 For most applications (i.e., near-surface)  1 ≈  2 ≈ 1 ;  (10 -4 –10 -1 ) «  (10 6 –10 10 !), and hence (i.e., we are imaging velocity variations corresponding to changes in dielectric permittivity!) For the water table, R ~ 0.1 Recall seismic waves attenuate as where Q is quality factor; Radar waves attenuate similarly as ; where Attenuation is extremely high for shale, silt, clay, and briny water (which is why GPR rarely penetrates > 10 m!). 

4 Skin depth, or depth of penetration, is ~ 1/ . Hence main applications are in archaeology, environmental, engineering site investigation… Also used for cavity detection and other very near-surface applications GPR freqs

5 Frequency-dependence of the attenuation results in dispersion : High frequencies attenuate more rapidly; pulse appears to “broaden” and the phase is delayed: This has “appearance” of a lower velocity medium. GPR freqs

6 (From a very old cemetery in Alabama…) “Black-box” processing is simplistic so see some of the same features observed in low-level (brute stack) seismic processing:

7 Assuming a constant velocity can introduce a factor of 2 to 3 scale error in converting velocity to depth! ( But one could reduce velocity scaling error if  were calculated from, e.g., NMO or travel-time amplitude decay)…

8 V1V1 Alternatively can use moveout on Diffractions : h1h1 h2h2 x The equations are the same as they were for seismic, but since GPR is (usually) zero offset, x s = x g ! Thus rsrs xgxg

9

10 Note some data processing steps are similar to seismic but lack some tools (such as refraction velocity analysis). Commonly do static corrections for elevation, filtering, automatic gain control; much less common to migrate.

11 Introduction to Gravity Gravity, Magnetic, & DC Electrical methods are all examples of the Laplace equation of the form:  2 u = f (sources), where u is a potential, is the gradient operator Notation : Here, the arrow denotes a vector quantity; the carat denotes a unit direction vector. Hence, the gradient operator is just a vector form of slope… Because Laplace’s eqn always incorporates a potential u, we call these “Potential Field Methods”. → ^

12 Gravity We define the gravitational field as And by Laplace’s equation, (1) given a single body of total mass M ; here G is universal gravitational constant = 6.672x10 -11 Integrating equation (1), we have (2) Nm 2 kg 2

13 IF the body with mass M is spherical with constant density, equation (2) has a solution given by: Here r is distance from the center of mass; is the direction vector pointing toward the center. Newton’s Law of gravitation: So expresses the acceleration of m due to M ! has units of acceleration  Gal in cgs (= 0.01 m/s 2 ) On the Earth’s surface, m/s 2


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