Flow Meters & Flow Controllers

Magnetic Flow Meters

INFORMATION

SPECIFICATION

Electromagnetic Flow Meters

FTI and Burkert lines of electromagnetic flow meters are cost-effective to measure all electrically conductive liquids (> 5 µS/cm) in process applications. The new generation of meters incorporates improvements to the magnetic distribution elements which allows more accurate operation throughout all flow regimes, allowing up to a 1000:1 turndown.

Industrial process application Mag Meter

	Capacity -Water				Max Pressure		Fluid Temp
Model	lpm	gpm	Accuracy	Repeatability	Bar	Psig	C	F	Construction	Connection
EL 2200 FTI General Purpose	5.22 to 71086	1.38 to 18779	0.2% OR	0.1%	Dependent on flange rating		-40 to 180	-40 to 356	Housing: Acrylic painted carbon steel, optional stainless steel Electrode: Hastelloy C22 / Platinum / Titanium / Tantalum Liner: PTFE / Ebonite	Flanged
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8055 Burkert General Purpose	0.24 to 4666	0.06 to 1232	0.2% OR	0.1%	63	928	-20 to 130	-4 to 266	Housing: Carbon steel Painted Electrode: 316L/ Hastelloy C / Titanium / Tantalium / Platinum-rhodium Liner: PP/ PTFE Gasket: FKM/ EPDM/ PTFE	Wafer & Flanged
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Sanitary applications Mag Meter

	Capacity -Water				Max Pressure		Fluid Temp
Model	lpm	gpm	Accuracy	Repeatability	Bar	Psig	C	F	Construction	Connection
EL 2400 FTI Sanitary	6 to 4997	1.6 to 1320	0.2% OR	0.1%	16	232	-40 to 140	-40 to 284	Housing and Fitting: 304 stainless steel Electrode: 316L / Hastelloy C22 / Titanium Liner: PTFE	Tri-Clamp & DIN 11851
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8056 Burkert Sanitary	0.003 to 4666	0.0009 to 1232	0.2% OR	0.1%	16	232	-20 to 130	-4 to 266	Housing: 304 stainless steel Electrode: 316L SS Liner: PTFE Gasket: FKM/ EPDM/	DIN11851, Clamp ISO2852 or Clamp BS4825
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Low flow & small line Mag Meter

	Capacity -Water				Max Pressure		Fluid Temp
Model	lpm	gpm	Accuracy	Repeatability	Bar	Psig	C	F	Construction	Connection
EL-500 FTI Low flow Measurement	0.083 to 166.6	0.02 to 44	0.2% OR	0.1%	16	232	-20 to 160	-4 to 320	Housing: 304 stainless steel Electrode: 316L SS (standard) / Hastelloy C22 / Titanium Liner: PTFE	NPT, TriClamp, DIN 11851, UNI 338
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8051 Burkert Low flow Measurement	0.003 to 208	0.0008 to 55	0.2% OR	0.1%	40	580	-20 to 130	-4 to 266	Housing: 304 stainless steel Electrode: 316L SS (standard) / Hastelloy C/ Titanium/ Tantalum/ Platinum-rhodium Liner: PTFE/ FKM/ EPDM/ FFKM	Threaded
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Insertion Mag Meter

	Measuring Range			Max Pressure		Fluid Temp
Model	m/s	Accuracy	Repeatability	Bar	Psig	C	F	Wetted parts material	Connection
8041 - 8045 Burkert Insertion Mag Meter	0.2 to 10	0.2% OR	0.25% OR	16	232	-15 to 150	-3 to 302	Sensor armature: PVDF/316L Electrode: 316L/HastelloyC22 Gasket: FKM	Insertion
Data Sheet 8041 Data Sheet 8045 User Manual Sales Support

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	2010-10-15 Signed agreement with the NASA Polycontrols will be contributing to the next mission to Venus, whose objective is to explore its surface which cannot be seen from Earth. An agreement was reached with the NASA Glenn Research Center for the supply of a gas mixing system to simulate the atmosphere of the planet Venus. This system will reproduce the planet’s atmosphere to test the electronic equipment of the exploration module which must withstand thermal stress and a highly acidic and corrosive environment. Venus is known as the Earth's twin because the two planets are similar in ... size. Venus is closer to the sun than any other planet except Mercury. At its closest approach, Venus is about 38.2 million kilometers from Earth. Although Venus is called the Earth twin, its surface conditions appear to be very different from those of the Earth. The planet is surrounded by thick clouds of sulfuric acid, preventing its observation. The surface of Venus is extremely hot and dry. The temperature of the planet's surface is about 870 degrees F (465 degrees C), the temperature is higher than that of any other planet. Most astronomers believe that Venus's high surface temperature can be explained by what is known as the greenhouse effect. A greenhouse lets in radiant energy from the sun, but it prevents much of the heat from escaping. The thick clouds and dense atmosphere of Venus work in much the same way. The sun's radiant energy readily filters into the planet's atmosphere. But the large droplets of sulfuric acid present in Venus's clouds -- and the great quantity of carbon dioxide in the atmosphere -- seem to trap much of the solar energy at the planet's surface. Read more Archives

Signed agreement with the NASA