AGU Fall Meeting 2017 in New Orleans

AGU Fall Meeting 2017 in New Orleans

AGU Fall Meeting is the one of largest and preeminent Earth and space science meeting in the world. The 2017 Fall Meeting will take place in New Orleans, Louisiana, offering attendees the chance to discover a new location that features world renowned cuisine, music, arts and culture, and provides access to vital scientific ecosystems. The Crescent City provides attendees access to the world-famous French Quarter, Jackson Square, the Saint Louis Cathedral, and a ride on the historic St. Charles streetcar through the elegant Garden District.

Fall Meeting will offer a unique mix of more than 20,000 oral and poster presentations, a broad range of keynote lectures, various types of formal and informal networking and career advancement opportunities, scientific field trips around New Orleans, and an exhibit hall packed with hundreds of exhibitors.

Fall Meeting brings together the entire Earth and space science community from across the globe for discussions of emerging trends and the latest research. The technical program includes presentations on new and cutting-edge science you can’t get anywhere else. Fall Meeting offers something for everyone, from every scientific discipline, including the opportunity to:

  • Hear about a variety of relevant scientific topics
  • Listen to top-notch speakers
  • Build relationships with peers
  • Gain research inspiration from a new location
  • Stay up to date on the latest innovations in the field
  • Gain visibility and recognition of your work

Geobit is presenting at the AGU Fall Meeting being held in New Orleans, 11-15 December 2017. In addition, Geobit welcomes you to visit our team at our AGU exhibit throughout the week.

Geobit at SEG 2017

Geobit at SEG 2017

Geobit, ISTI and HMSC join together at the SEG Annual Meeting in Houston, Texas this September.  We are a team, (Earth Imaging Seismic Monitoring), providing a complete seismic monitoring solution.

We welcome you to visit us at our booth, #2521, to meet our team and learn about the latest offerings. Paul Friberg & Ilya Driker (ISTI), Mike Hasting (HMSC, Inc.), and Dimitris Mourtzouchos & Nikos Germenis (Geobit) will be available to answer your questions.

More information on the SEG (Society of Exploration Geophysicists) meeting may be found here.

The Earth Imaging team

The Earth Imaging team

With 65+ years of combined experience, GEObit, HMSCinc and ISTI are joining forces to become the most competitive and fastest growing joint venture group in the seismic monitoring services industry.

Providing state-of-the-art seismic instruments, network designed, installation techniques, data monitoring and processing services, our group is able to deliver a cost effective total solution to the energy exploration & production industry, especially to the oil, gas and geothermal sector. Our key benefits are that we produce in-house hardware and software while installing and maintaining the microseismic monitoring network to ensure a high level of data quality and availability. In other words, we make the technology – we apply the technology – we offer the technology.

We have worldwide experience having installed and operated seismic networks all over the world, from Indonesia/Papua jungle to the Middle East desert, from Alaska glaciers to Himalayan Mountains. In the USA, we are currently running many dedicated microseismic monitoring projects with over 200 stations installed in the past 10 years.

GEObit provides high sensitivity wide-band and near broad-band seismic sensors, surface or borehole type, and high dynamic range, low power 32bit ADC data loggers with local data storage and real time telemetry over seedlink protocol. We are focusing to low power and cost efficient solutions so we provide to our customer seismic networks with low installation and maintenance costs. Our instruments are ideal for local and regional seismicity and micro-seismicity monitoring and for seismic events such as those induced by unconventional hydrocarbon extraction. Our high fidelity data-loggers ensure that these signals are recorded with the highest resolution and timing accuracy.

Geobit Instruments Ltd.

Data Loggers and Sensors, Visit the website

HMSCinc has over 30 years’ experience designing, building and installing dedicated microseismic monitoring stations and networks for seismicity monitoring of active geothermal resources, oil and gas fields, and volcanoes. HMSCinc provides integrated seismic station solutions, pre-drilling background monitoring services, installation of bore-hole stations (from a few hundred feet to over 10,000 ft), real-time event detection and location services, as well as expert testimony when needed.

Hasting Micro-Seismic Consulting, Inc (HMSCinc)

Installation and Operations, Visit the website

ISTI specializes in developing custom data acquisition, analysis and processing software for the geophysical sciences.. Micro-seismic data acquisition and processing is performed by custom solutions using existing open source software as a foundation, saving our customers both time and money. ISTI provides several products and services covering all geophysical applications and monitoring needs of the industry.

Instrumental Software Technologies, Inc. (ISTI)

Monitoring and Data Processing, Visit the website

Visit us at booth #2521, SEG2017, Houston Texas, USA

24 – 29 September 2017

Where’s my Earthquake?

Where’s my Earthquake?

The original article was published in LinkedIn on May 17, 2017.

Paige Mamer

Senior Geophysicist - Microseismic and Induced Seismicity, LinkedIn Profile

During fantastic Induced Seismicity sessions at the Calgary GeoConvention, many speakers commented on the inadequate depth accuracy of their data; “700 m uncertainty, that’s unacceptable!” I saw shocked faces, nods, and heads shaking in disagreement.

Well, wait a minute! Why the varied reactions? Is 700 m good or bad?

Indeed we do need to know where induced events are coming from. We need to know this to design better horizontal drilling and completion programs (or disposal programs), to know where to map faults for hazard assessment and mitigation, to build better models, we need to allay fears of ground water contamination (even if faults aren’t slipping kilometers up towards the surface, we still need to be able to prove to the public, and potentially lawmakers, that this isn’t the case).

But while criticizing the event uncertainty, nobody discussed the design of the arrays used to capture the presented data. This, I would argue, is the single, most important factor in deciding if 700 m accuracy is really terrible, quite reasonable, or perhaps even impressive. Yes, picking error and velocity model assumptions contribute to location accuracy, but processing doesn’t mean anything if you don’t have adequate data to process.

We are quite good at figuring out the lateral positioning of event, for the very reason that it is easy for us to put out a spread of sensors on the ground over the affected area. Depth is tricky because it is very difficult to fill an underground volume with sensors – the notable exception being underground mining where sensors can be placed in a 3D volume throughout the mine.  We get around this by putting more and more sensors on the ground in a targeted area – the better accuracy we want, the more sensors we need (think satellites to get a GPS location). Surface arrays with a hundred to thousands of sensors are routinely used to measure fracturing in rock as loud as my fingers typing on this keyboard. Arrays built to monitor for induced seismicity typically use fewer stations because the events are bigger and easy to ‘hear’.

Let’s get back to the question – how good is 700 m uncertainty? The short answer? It’s a question of scale. Let’s consider an array of 5 sensors placed within a 5 km radius of a multilateral pad (ie, many horizontal wellbores). Because the sensors are concentrated where the event is likely to be, we should be able to come up with a good location. In this case, a solution with 700 m resolution would leave us with more questions than answers and may not meet certain government regulations.  So 700 m isn’t great.

Now take those 5 sensors and spread them all over Alberta. The uncertainty is now on the scale of many kilometers because the sensors are far from the event (just like it’s harder for our ears to pinpoint the source of a noise that is far away). So a solution with 700 m uncertainty would be astonishingly fantastic! In fact at this scale seismologists often have to use a fixed depth to get an event epicentre (something to remember the next time you are perusing NRCAN’s Earthquakes Canada site).

What would it take to get that multilateral pad case from 700 m to 10 m? It takes substantially more sensors and a lot more money, which isn’t a scalable solution for companies in the best of times. That scale of uncertainty is even a challenge for denser microseismic monitoring of any kind.

If 700 m seems so outrageous, or even 500 m as is often used as a design target, are we under-designing our arrays or are we simply expecting too much from the arrays we opt to put in the ground?

* Special thanks to Mrs. Mamer who shared this article on our blog.

GEObit participated in 79th EAGE 2017

GEObit participated in 79th EAGE 2017

GEObit participated in 79th EAGE Conference & Exhibition 2017. The event took place in Paris, 12-15 June 2017.

During this event we met with most of our clients, shared our ideas with peers from around the world and we managed to grow our network of invaluable contacts for benchmarking, partnering and expanding our activities.

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