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					 PERMAFROST AND GAS HYDRATE BASICS Permafrost exists in cold climates on land. Gas hydrates are
					found in or below permafrost and under deep water coastal
					regions. Gas hydrates are possible offshore the coastlines
					of all continents, even in tropical regions. They cause difficulties when drilling to deeper
					targets. Gas hydrates are reported to be a huge source of
					natural gas, although the technically producible quantity is
					much smaller.
 
					
					Gas hydrate production was reported by the Russians in 1970
					at a rate of
					more than 10 mmcf/d in Siberia. It was called "solid gas" at
					the time  Canadian exploration wells
					encountered them in the early 1970's and also reported some
					of the difficulties in drilling and testing such intervals. 
					There are proven gas hydrate reserves on the North Slope of
					Alaska and much evidence for hydrates all along East Coast
					USA. Floating lumps of "fizzy ice" have been reported
					offshore Oregon.
 
 Much more recently, China has tested some gas hydrate wells
					in the South China Sea and significant exploration effort
					has been undertaken to define areas of interest. This may
					account for some of the political tension in the area, as
					China is looking for ways to obtain natural gas to reduce
					reliance on coal fueled power plants.
 
					
					 PERMAFROST BASICS Permafrost is defined as soil or rock that is permanently
					frozen in all seasons for more than two consecutive years.
					Permafrost covers much of the northern latitudes above 60
					degrees and most of Antarctica.
 
					
					Water in pore space freezes
					when the temperature of the rock is below zero degrees Celsius (32 degrees F),
					A phenomenon called freezing point depression (FPD) causes
					the actual freezing temperature to be somewhat lower than 0
					C. FPD is a function of pressure, salinity, and pore size,
					and is usually about minus 1 to minus 2 degrees Celsius in
					clean coarse grained sandstones. It can be as much as minus
					8 C in very fine grained silts and shales. 
					  View from
					the North Pole showing areas of continuous (blue) and
					discontinuous permafrost (grey) Clay
			bound water in shale does not freeze, so shale properties change
			only slightly, depending on the amount of free water in the
			effective porosity of the shale. Silty shales have more porosity
			than pure shale and are more strongly affected by freezing.  
					
					Studies designed to locate the base of permafrost were
					sponsored by the Geological Survey of Canada in the 1960's, 1970's, and
					again in the early 1980's as more log data became available.
					Permanent temperature recording systems using thermistors 
					equally spaced along a cable were installed in
					numerous observation wells throughout the Arctic.  These
					surveys form the basis for static temperature data that is
					still relied upon today. 
					
					
 Freezing alters the
					physical properties of the composite rock. Ice has a very
					high resistivity and high acoustic velocity compared to
					water, thus resistivity and acoustic travel time logs are
					changed significantly. Many other physical properties are
					much less affected.
 
					
					In a sandstone interval, the base of permafrost is easy to
			pick on the resistivity log. In shales, it is much more difficult.
					The base of permafrost is often picked at the base
			of a frozen sandstone; this depth is called the base of ice-bearing
			permafrost (IBPF). 
			
 
  PERMAFROST ON WELL LOGS 
  The
			depth to the base of permafrost varies considerably by location and
			may reach 1500 meters or more. The base of permafrost is often
			assumed to be the
			depth below which the formation temperature exceeds zero degrees Celsius.
			However freezing point depression can cause confusion since some rocks remain
			unfrozen well below zero Celsius. Gas hydrates remain frozen
			well above zero Celsius, so "base of permafrost is a bit of a moving
			target. 
					
					Long
					spaced sonic log (left) and deep resistivity log (right) are
					used to identify the base of frozen rocks, around 1800 feet
					in this example, based on reduction in resistivity and
					increase in sonic travel time. Frozen rock may contain
					water-ice (permafrost) or gas hydrates (solid gas) or both.  
					  
					  
					  
					  
					 
					 Example of long and
					short spaced sonic logs in a permafrost section. The long
					spaced curve shows the frozen rock velocity (as travel
					time). This curve cannot be used for porosity calculations.
					The short spaced curve shows the  thawed travel time,
					which can be used for porosity calculations after shale
					corrections are applied. In shaly zones, the two curves give
					similar values because the clay bound water does not freeze,
					although any free water in the silt fraction of the shale
					does freeze. 
					  
					  
					  
					  
					  
					  
					  
					  
					  
					. 
					  
					  
					  
					  
					  
					
					  An example of logs in permafrost:
					standard induction and sonic logs, with a 20 foot Normal
					resistivity curve from a modified ES Log. The 20 foot Normal
					curve reads considerably deeper into the formation and is
					less influenced by the thawed near-wellbore interval. All
					resistivity curves show high values in frozen sands.The 20
					foot nonmal reads higher than the induction log in frozen
					shale. Only free water in the shale can freeze; clay bound
					water cannot  freeze. The sonic sees only the thawed
					zone so it is not jelpful in identifyung base of permafrost.
 
					
					
  GAS HYDRATE BASICS  Gas
			hydrates, also called clathrates, are mechanical mixtures of natural gas and water,
					forming a crystalline solid in cold environments. These
					mixtures are called "inclusion compounds". The water molecules
			surround the gas molecules to form "cages" that trap the gas into
			the crystals. There is no chemical bond between the water and the
			gas, so the crystal is not a chemical compound.
  Macro photo of a gas hydrate sample from a core (GSC Bulletin 585)
 
			Gas hydrates are often found in or below permafrost zones on
			land, or in deep water along continental margins. They can extend
			below the base of permafrost, even though formation temperature is
			above 0 C. Hydrates have been discovered or inferred along the
			coastlines of all continents, even at temperate latitudes, and in
			deep water trenches in the Pacific. 
					 The
			quantity of gas in a hydrate does not depend on the depth, pressure,
			or temperature of the reservoir, as is normally the case for natural
			gas. Hydrates
			can contain far more gas at shallow depths than a conventional
			reservoir at the same depth. This can result in unexpectedly high
			pressure in the wellbore as the hydrate thaws, with all the dangers
			of blowouts and damaged equipment that this suggests. 
			A good
			description of gas hydrates is contained in "Naturally Occurring Gas
			Hydrates in the Mackenzie Delta", C. Bily and J. W. L. Dick, CSPG
			Bull., 1974. 
			Gas hydrate
			crystal with water molecules (red) trapping methane molecules (grey) (USGS image)
  
			The various
			phases of water, ice, hydrates. and free gas are determined by a
			phase diagram, which depends on the specific gravity of the gas,
			salinity of the water, temperature, and pressure. The latter two
			factors are functions of depth, so the phase diagrams are often
			plotted versus depth, using assumed pressure and temperature
			gradients. Schematic examples are shown below. 
			   Left:
			Schematic phase
			diagram for water, water-ice, gas hydrates. and free gas. 
			Right: Phase diagram
			with temperature log, showing a situation where temperature is too
			high to permit hydrate formation.
			(USGS images)
 
			 Left:
			Phase diagram for on-shore situation where temperature is low enough
			to permit hydrate formation (blue shading), 
			
			Note base of permafrost at 0 C isotherm.   Right: 
			
			Deep water
			off-shore has distinctly different temperature profile, so hydrates
			can form near seafloor in very recent sediments (blue shaded
			area). Higher specific gravity and higher salinity will move the
			hydrate phase boundary (red line) to the right, increasing the depth
			at which hydrates may form.  
			(USGS image)
 An
                increase in temperature increases the pressure required to form
                hydrates, while small percentages of ethane or propane lower the
                hydrating pressure considerably. Hydrogen sulfide and carbon dioxide
                also decrease the required pressure. 
				   Left:
				Graph showing effect of salinity on hydrate phase. Right: Effect
				of  gas specific
				gravity on hydrate phase.
 (source: Natural
				Gas Engineering Handbook, D.Katz, 1959)
 
				
  DRILLING and Production Hazards IN Gas Hydrates Drilling into permafrost and gas hydrates, or to deeper targets
				below them, is fraught with problems. Thawing of permafrost in
				otherwise unconsolidated sediments will generally mean a large,
				washed-out borehole, with poor logs. Drilling with a chilled mud
				system has been attempted, but this has its own hazards - if NaCl or CaCl2 are used to prevent freezing of the mud, it may
				still freeze if borehole temperature falls outside the liquid
				phase diagram for the mixture.
 
				
				   Left:
				Permanent temperature survey in observation well #20 at
				Resolute Bay, Nunavut showing base of permafrost at about 1200
				feet at 32 F.   Right: Phase diagram for NaCl and CaCL2 showing
				salt concentration "window" for the coldest wellbore temperature
				at Resolute Bay (and similar latitudes). Getting stuck in the hole
				with oversaturated salt mud is really embarrassing. (Source: Marshall and Crain, AIME, 1970)
 
				Thawing of gas hydrates generates gas at pressures well above
				those expected at these shallow depths. It may be impossible to
				raise mud weight sufficiently to prevent a blowout, so chilled
				mud and a quick casing job are indicated. If a well
				is cased and cemented, that gas pressure may cause wormholes in
				the cement, leading to a permanent leak to surface as long as
				borehole temperature is higher than the hydrate stabilization
				temperature. High quality cement jobs in large, cold boreholes
				are notoriously difficult.  
				Continued thawing may cause casing collapse or rock subsidence,
				with loss of wellbore integrity. Successive thaw-freeze cycles
				aggravate these conditions and may cause vertical expansion of
				the rocks during refreezing.. 
				The
				typical production scheme proposed for gas hydrate wells is by
				depressurization. During production, wellhead control is
				difficult due to the high pressure and cold temperatures.
				Hydrates may reform in the plumbing. Produced water must be
				lifted and disposed of before it refreezes. Thawing allows fines
				migration which annoys pumping and compression equipment. Some
				experimental production methods involve the addition of heat or
				methanol to release the gas. Heat may affect non-gas bearing
				intervals in the permafrost, leading to casing collapse or
				movement. 
				
				 Proposed methods for gas hydrate production. (USGS image)
 
				On
				the North Slope of Alaska, the gas hydrate issue is
				further complicated by the presence of oil and free gas with
				hydrates in various combinations.  
				
				 Gas hydrate, free gas, and oil distribution Eileen area, North
				Slope, Alaska.  (USGS image)
 
				
				Deepwater offshore hydrate production has its own issues, and
				although a huge resource is postulated, I am not aware of any
				intentional attempts to produce it. No wonder shale gas is so
				popular! 
				
					
  log analysis IN Gas Hydrate WELLS 
  The
                excess hydrogen in gas hydrates compared to water or water ice, 
				1.10 versus 1.00 for water, and 0.90 for water-ice,  makes neutron
				porosity logs read
                high in gas hydrates. The lower density of ice and hydrate, 900 kg/m3 versus
				1000 kg/m3 compared to water, makes the density porosity read too high also. However, thawing near
                the borehole will reduce this effect and it is seldom seen. Instead
                the zone often looks like a normal water-invaded gas sand. If
				thawing is deep enough, gas crossover could occur. 
				Short
				spaced sonic logs reading the thawed zone can be used to
				calculate porosity, but compaction and gas corrections will be
				required. Long spaced sonic logs reading the frozen zone are
				difficult to analyze for porosity due to an unknown amount of
				excess (unfrozen) water along with the ice or hydrate. 
				
				Logging while drilling is recommended as there is less borehole
				rugosity and less thawing. Resitivity, shear and compressional
				sonic, density, neutron, and gamma ray are the usual logs
				required. If chilled invert mud is used, open hole logging may
				be successful. 
				
				Freezing of water causes salt rejection, leaving some excess
				unfrozen water with moderately high salinity. Higher salinity
				water tends to increase the SP deflection but the higher
				resistivity of the ice tends to reduce SP deflection. The net
				result is low SP deflection in frozen intervals. SP in the
				unfrozen intervals behaves normally. 
			Quantitative
			log analysis of permafrost -gas hydrate interval in Mackenzie Delta,
 run in 1983 using standard porosity and
 Archie saturation models.
			See
 explanation below
  
			Resistivity will read high values in both water ice and gas hydrate
			in sand sequences; shales will show typically low resistivity with
			moderate gamma ray values. Clay bound water does not freeze, so
			shale resistivity does not incresase much when frozen. 
			A long spaced sonic will read the frozen
			rock velocity (or travel time) but short spaced sonics will see the
			thawed zone velocity. Many hydrate zones are poorly consolidated, so
			caliper logs may show large washouts as the rock thaws. In large or
			rough boreholes, both density and sonic logs may show large spikes
			or noise.  
			Neither resistivity nor porosity logs are very helpful in
			distinguishing gas hydrates from water ice. The best indicator is
			the gas mud log because large quantities of disassociated gas are
			released as the hydrate is thawed. No significant gas is released
			from water ice. Free gas and even oil are also possible and gas mud
			logs will show less than in a hydrate zone. 
			 
			Quantitative log analysis is complicated by the inability of
			standard models to differentiate between water ice and gas hydrates.
			Free gas and gas hydrate (if thawed deeply enough) can be distinguished by gas crossover in cleaner sands. 
			By
			treating ice and hydrates as if they were hydrocarbons, standard
			porosity and Archie-type saturation models can give an estimate of ice plus hydrate content (black shading in
			Track 3) and free water (white shading). In this model:1: Shydr = 1 - Sw  provided zone is hydrate bearing and not
			water-ice.
 
			Standard deterministic or probabilistic multi-mineral models using
			quartz, clay, ice (water ice or hydrates) and free water will also
			work. In these models:2: PHIe = Vice + Vwtr
 3: Shydr = Vice / PHie  provided the zone is
			hydrate bearing and not water-ice.
 If a
			nuclear magnetic resonance log is run, the effective porosity from
			this log is the water filled porosity. Ice and hydrates are not
			seen. Thus:4:
			PHInmr = BVI + BVM
 5: SWnmr = PHInmr /
			PHIe
 6: Shydr = 1 – SWnmr
 Where:BVI = bulk volume irreducible from NMR (fractional)
 BVM = bulk volume moveable from NMR (fractional)
 PHIe = effective porosity from conventional logs (fractional)
 PHInmr = effective porosity from NMR (fractional)
 Shydr = hydrate saturation (fractional)
 Sw = water saturation (fractional)
 Vice = volume of ice or hydrate (fractional)
 Vwtr = volume of water (fractional)
 The
			base of permafrost is chosen by a nearby permanent temperature log
			(around 650 feet in this example). Black shading below this depth
			down to 1000feet is gas hydrate and there may be gas hydrates in the permafrost zone.
			Since salt rejection increases water salinity in the excess water,
			the water resistivity is unknown and variable, so the quantities of
			ice, hydrate, and excess water are not very accurate. The mud
			gas log is vital.  In
			older wells, the sonic log was often very noisy and seismic
			reference surveys were used to determine acoustic velocity. The
			beginning of low velocity would indicate the base of permafrost or
			base of gas hydrates, or shales.  These surveys were superseded by crystal cable
			surveys, the forerunner of the vertical seismic profile, which would
			be used today for this purpose. VSP's and their predecessors can be
			run in cased holes provided the shot point is far enough from the
			wellbore, otherwise the velocity derived from the survey will be
			that of the casing. A good description of the use of
			this tool is "Permafrost Investigation by Crystal Cable Surveys, 
			Mackenzie Deltas", I. H. Wallace and A. J. Stuart, CSEG, 1975, from
			which the following two illustrations were taken. 
			                  Crystal cable survey time vs depth plot with interpreted velocity
			values. Base of permafrost could be as shallow as 1400 feet or as
			deep as 2000 feet.
   
			 Crystal cable survey vs depth with other log data. Base of
			permafrost is still unclear due to large, washed-out borehole. Gamma
			ray needs borehole corrections to make shales stand out better.
			Sonic is in general agreement with SRS velocities but induction log
			does not show continuous high resistivity expected for a sand
			interval, so much of the interval is probably shale or shaly sand.
			Permafrost base is probably near 2000 feet because there is only low
			resistivity below this depth.
 
			  This log clearly illustrates a severe case of rock alteration due
			to permafrost. In this case, the short spaced sonic sees the thawed
			zone and the long spaced tool see the frozen zone. Porosity is
			derived from the short spaced log, with appropriate shale and
			compaction corrections, but seismic velocity must be taken from the
			long
 spaced log.
 
				
				
					
				
				
			 Gas Hydrate
			VOLUME IN PLACE Empirically,
                the ratio of water to gas necessary to form a hydrate is as follows:
 
 Excess
                Hydrogen
 1. Methane CH4.6H20            4/12 = 33%
 2. Ethane C2H6.8H20             6/16 = 37%
 3. Propane C3H8.17H20         8/34 = 23%
 The
			volume of hydrocarbon in a gas hydrate is a function of the hydrocarbon
                type only. Water saturation is meaningless. The
                ratio of gas to water would range from 433 scf/bbl for propane
                to 1230 scf/bbl for methane. This
                is equivalent to 170 cubic feet of methane per cubic foot of
                pore space (or 170 m3 per cubic meter of pore space) at standard
                temperature and pressure and 60 cubic feet of propane
                per cubic foot of pore space, regardless of depth of burial. Gas in
			place is derived by converting pore volume to gas volume:7: PV = (PHIe * THICK
 8: HPV = PV * Shydr * KG0
 9: GIPhydr = KV3 * HPV * AREA
 Where:AREA = reservoir area (acres or m2)
 HPV = hydrocarbon volume (feet or meters)
 PHUe = effective porosity (fractional)
 PV = pore volume (feet or meters)
 Shydr = hydrate saturation (fractional)
 Sw = water saturation (fractional)
 GIPhydr = gas in place as hydrates (mcf or m3)
 KV3 = 43.56 for English units
 KV3 = 1 for Metric units
 KG0 =164 for methane
 KG0 = 60 for propane
 NUMERICAL
                EXAMPLE:1. Assume the following data:
 PHIe = 0.35
 Sw = 0.20
 Hydrate is methane
 THICK = 300 feet
 KV3 = 43.56
 KG0 = 164 scf/scf
 AREA = 640 acres
 
 HPV = 0.35 * 300 * (1 - 0.20) * 164 = 13776 ft
 GIPhydr = 43.56 * 13776 * 640 / 1 000 000  = 384 Bcf/section
 
 
					
			
			
			 Gas Hydrate EXAMPLES The original Mallik L-38 well in the Mackenzie Delta was drilled in
			1972 and discovered a major gas hydrate and free gas interval. The
			well sits on a large structure and was suspended pending construction of the Mackenzie Valley
			Pipeline. In 2002, an international
			joint government, industry, academic consortium (Mallik 2002 Gas
			Hydrate Production Research Well Program) was formed to
			investigate alternate methods of producing gas hydrates, using this
			structure as a test platform. Observation wells were drilled and various
			production schemes have been tested. A 34 GB data set can be
			downloaded from the National Research Council (Canada) website as
			Geological Survey of Canada Bulletin 585.
 
			 Original wireline logs and gas log for Mallik L-38. Compare location
			of hydrate zones with log
 response and gas log showing gas hydrates and free gas below 3000
			feet. Permafrost base is around 1900 feet, well above this log
			segment. (USGS image, redrawn from Bily and Dick, 1974).
 The 2002 Production
			Research Project drilled additional wells near Mallik L-38 to test
			various production schemes and evaluation techniques. The logs and a
			computed result are shown below. 
			 Raw logs and computed results for
			Mallik 5L-38 drilled
			in 2002. Logs are (from left to right) array laterolog, array
			induction, shear and compressional sonic, density and neutron with
			gas crossover shaded green, computed results with clay, quartz
			(yellow), hydrate (red) and water (blue). Note depths are in meters
			and cover approximately the same interval as the Mallik L-38 logs
			shown above.
 The above
			illustration is from "FORMATION
			EVALUATION OF GAS HYDRATE BEARINGSEDIMENTS" by Frank Williams, Mike Lovell, Tim Brewer,
			Christian Buecker, Peter Jackson, Ameena
 Camps, SPWLA, 2008.
 
			 Seismic section on Mallik structure, shaded area shows gas hydrate
			over free gas. (USGS image)
 
			   Left:
			Schematic layout of experimental wells at Mallik L-38,  
			Right: Gas
			flare during test of Mallik L-38 and Mallik Project logo. This project is an international joint government,
			industry, academic consortium to investigate alternate methods of
			producing gas hydrates. (GSC
			Bulletin 585)
 
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