Speaker: Avto Tkabladze, Nuclear Advisor, Schlumberger

Bio:

Avto Tkabladze is a Nuclear Advisor at Schlumberger’s Houston Formation Evaluation Integration Center in Sugar Land, Texas. He is involved in the design, characterization, and algorithm development for nuclear logging tools. Currently, he is the lead physicist of the X-ray density tool project. Before joining Schlumberger in 2007, he worked in theoretical and experimental particle physics at DESY (Germany) and Jefferson Lab (USA). He received a PhD in theoretical particle physics from Tbilisi State University, Georgia, in 1990.

ABSTRACT:

Formation bulk density is classically measured by irradiating the formation with gamma rays emitted by a source, and counting the Compton scattered photons returning to the gamma ray detectors in the well logging instrument. For at least three decades, service companies and operators have tried to find ways to eliminate the risks of handling, transporting, and storing logging sources and the issues associated with losing a source in a well.

The continued success of sources in density logging shows that attempts at their replacement have been unsuccessful due to the insufficient measurement quality or lack of practicality of alternative logging instruments. An X-ray density pad sonde was engineered to measure bulk density without a radioisotopic source. The pad contains a rugged, compact X-ray generator with an endpoint energy larger than 300 keV. The core of the tool is the generator, which emits a controlled, focused, stable X-ray flux into the formation. The scattered X-rays are detected by strategically placed scintillation detectors.

The pad tool architecture significantly reduces the effects of standoff and borehole rugosity compared to a mandrel design. Modeling and experimental data prove that the physics of the formation density measurement using a sonde with an X-ray generator and scintillation detectors can be described in the same way as the traditional density measurement, which is based on a monoenergetic gamma ray source. Although the ¹³⁷Cs gamma-ray source density measurement and the X-ray density measurement differ in the relative magnitude of the responses to formation density and lithology (photoelectric factor, PEF), the fundamental physics is the same. An endpoint energy above 300 keV ensures that the transport and attenuation of X-rays in the formation are dominated by Compton scattering, like the attenuation of gamma rays from a ¹³⁷Cs source. The contribution of the photoelectric absorption to the attenuation of the X-rays is increased, but it remains much smaller than the effect of Compton scattering, making the corrections for lithology and borehole fluid straightforward.

A characterization database was acquired to probe the physics of the measurement and to derive robust density and PEF algorithms. Plots of near- and far-detector count rates for different mudcake thicknesses and mud types show spine-and-ribs behavior like ¹³⁷Cs -based density tools. Field logs acquired in wellbores give a tantalizing perspective of the benefits of X-ray density measurements. Improved precision and vertical resolution logs in several operator wells show the maturity of this breakthrough technology and its ability to perform successfully in typical oilfield conditions.

There are two identical sessions, please register for only ONE session which fits your schedule. 

Morning - Wednesday, September 26th,    8am – 9am US Central Time; 
Evening - Thursday, September 27th   8pm – 9pm US Central Time.

This event is part of the Member benefit package and is free for Members current in their membership dues. Login to your  account to register. 
Former Members (lapsed dues), Chapter Members (affiliated in local activities) and New Members are encouraged to become active in the Society to take advantage of our monthly webinar series. Receiving this message confirms you have an account in the SPWLA database. If you need assistance in signing in please contact [email protected] .
(PLEASE NOTE: If you just paid your dues. You can not register for this event until your payment posts the next business day)