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Esp Fundamentals

Apr 02, 2018

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    ELECTROSTATIC

    PRECIPITATOR

    AN

    ENVIRONMENT

    SAVIOUR

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    SPECIFICATION

    DESIGN CODE : FAA-6*45-78125-2

    FLOW : 296M3/SEC.

    TEMP. : 1290C

    INLET DUST BURDE :73.83gm/m3(78.66T/HR)

    TREATMENT TIME :35.37 SEC.

    PRESSURE DROP :20 MMWCC.E RAPPING FREQ. :1.1RPM

    E.E RAPPING FREQ. :2.5 RPM

    HORIZONTAL FLOW STEEL CASING PYRAMIDAL HOPPER

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    jai maan sharde!

    CORONA EFFECT

    COLLECTING ELECTRODEEMITTING ELECTRODE

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    WHAT IS CORONA ?

    CORONA is an electric discharge phenomenon in which gas molecules

    are ionised by the collision of electron in the region of high strength electric

    field.

    The electron for CORONA initiation is supplied by random source such asnatural radioactivity or cosmic rays. Under the influence of high strength

    electric field these free electrons are accelerated to terminal velocity. The

    rapidly moving electrons collide with the orbital electron of gas molecule

    and release it from the orbit. Hence the gas molecule assumes + VE charge

    and more free electrons are released. The free electrons again collide withother gas molecules, forms +VE ions and releases more free electrons . This

    process continues till the energy of free electrons reduces to the level that it

    can not dislodge the orbital electron of gas molecule,hence these free

    electrons are captured by the gas molecules and assumes -VE charge.Under

    the influence of electric field ,these -Ve charged gas molecules movetowards collecting electrode and charge the dust particles. When dust

    particle gets saturated electric field is exerted on it and move towards

    collecting electrode where it gives up its charge and stick there due to

    intermolecular cohesive/adhesive forces. More the intensity of electric field,

    more fast and more the no. of free electrons, accordingly more ionisation&more efficiency of ESP.

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    LINE DIAGRAM OF ESP EC-HVR CKT.

    VE

    VE

    HVRC

    SHR

    ICE-C

    FIRING CKT.

    ACRHVR

    HFC415 V

    A.C.

    THYRISTER

    FILTER VOLTAGE

    FILTER CURRENT

    ACR-TO LIMIT THE P/CURRENT IN CASE OF FLASH OVER ON D.C.SIDE

    SHR-SHUNT RESISTER,1V=FULL CURRENTHVRC=HIGH VOLTAGE RESISTER CKT.,400MICRO AMPS.

    HFC-HIGH FREQ. CHOKE,PROTECTS HVR FROM SURGE OCCURING DURING SPARKING

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    FACTORS AFFECTING ESP

    PERFORMANCE

    RESISTIVITY OF DUST PARTICLES

    FLUE GAS VELOCITYPARTICLE SIZE & FIELD STRENGTH

    RAPPING FREQUENCY

    SPARKS RATE

    HOPPER EVACUATION

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    RESISTIVITY OF DUST PARTICLES

    Resistivity of dust particles play major role in ESPperformance

    A too high resistive dust does not readilycharge&give up its negative charge to collective electrode

    whereas low resistive dust particle readily gives upits negative charge and assumes positive charge.

    Inlet flue gas temp ,sulpher content & moisturecontent play major role in controlling resistivity of

    flue gas.Low resistivity - 104-107 ohm-cm

    Normal resistivity- 108-1010 ohm-cm

    High resistivity - more than 1010

    ohm-cm

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    RESIST

    IVITY(ohm-cm)

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    FLUE GAS VELOCITY

    There are two forces acting on the dust particles havingperpendicular to each other as shown in above diagram.

    The first one is due to flow of gas and the second one isdue to electric force on the ionized dust particleperpendicular to the motion of gas.

    The path followed by the dust particle will be resultantof two forces as shown above.

    The efficiency of ESP decreases with increase in velocity& decrease in voltage.

    C.E C.EE.E

    ELECTRIC FORCEFORCE

    DUE

    TOV

    EL.

    A

    BC

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    PARTICLE SIZE & FIELD

    STRENGTHThe efficiency of ESP is governed by DEUTSCH- ANDERSON equation :

    Efficiency = 1-[e](-A/Q)

    =Migrationvelocity= r E /2r =Radius of particle

    E =Field strength

    =Viscosity or frictional coefficient of flue gasA = Effective collecting area of ESP

    Q = Gas flow through ESP

    e = 2.718

    RAPPING FREQUENCY

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    RAPPING FREQUENCYRapping is also a complex phenomenon in ESP . If rapping

    frequency is too high then it will not allow the dust todeposit on collecting electrode and hence the collection

    /removal of dust will be difficult. Similarly, if rappingfrequency is too low then very thick layer of ash will

    deposit on C.E. which will cause considerable voltage dropor can cause back corona if resistivity is very high .

    C.E. RAPPING FREQ.FIELDNO.

    START TIME REPEAT TIME RAPS/HR.

    01 00,00 00,04 15

    02 00,01 00,05 12

    03 00,02 00,06 10

    04 00,03 00,07 08

    05 00,04 00,12 05

    06 00,00 00,30 02

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    SPARK RATERECOMMENDED :5-10 SPM

    Field strength is adjusted in such a way

    that limited sparks takes place. Withsome sparks/min. , we are able tocreate more strong field . The outagedue to spark is offset by achieving morestrong electric field with limited spark.However, if spark is too high thenfrequent collapse of field will reduce theefficiency and increase the erosion ofemitting electrode.

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    ASH COLLECTION DATA PERPASS

    FIELD STAGE% RAP./HR ASH

    COLLECTION(KG/

    RAP.)

    ASH

    COLLECTION(MT/

    HR)

    01 78.00 20 837 16.74

    02 17.14 10 340 3.40

    03 3.20 06 114 0.684

    04 1.10 04 58 0.232

    05 0.40 03 28 0.084

    06 0.16 02 17 0.034

    TOTAL=21.74MT/HR

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    BACK CORONABack corona is the emission of +ve ions from collected dust

    layer that occurs when voltage drop across the collected dust

    layer exceeds the electrical breakdown strength of interstitialgases in the dust layer.

    As the high resistive dust layer builds upon the collecting electrodes ,

    the the dust layer and collecting electrode form a high strength

    electric field. The surface of the dust layer is negatively charged ,the

    interior is neutral and collecting electrode is grounded (+ ve) .Under

    this condition all the ion current must pass through the dust layer to

    reach the collecting electrode . This current creates an electric field

    in the dust layer & when it becomes large enough the local electrical

    breakdown of interstitial gases occurs. As this happens ,+ve ions aregenerated within the dust layer and are accelerated towards emitting

    electrode .On the way it neutralizes the -ve charged particles and

    reduces the ESP efficiency.This breakdown condn. is BACK

    CORONA.The voltage reduces and current increases in thiscondition.. Resistivity 2*1011 ohm-cm

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    CHARGING DURINGCOLD START UP

    ESP fields should not be charged below 1000c asmoisture present will cause ash cake formation oncollecting electrode which is difficult to dislodge.

    Also ESP temp.should be sufficiently higher thanthe acid dew point temp. (90-1000c)beforecharging to avoid stress corrosion cracking ofelectrodes.

    Switch on the heaters 24 hrs. before BLU.Start rapping motors on intermittent mode justbefore BLU..

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    CHARGING DURING OIL

    FIRINGIt is recommended to charge ESP fieldsduring oil firing at ~ 50 mA.

    In the charged condn., the electric fieldrepels the chloride vapour of the flue gaseswhich if comes in contact with E.E. causesbrittleness in E.E. and it may snap duringoperation.

    The current during oil firing should be limitedbelow spark level as spark in oil firing maycause fire hazard.

    ESP RETROFIT ACTIONS IN

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    ESP RETROFIT ACTIONS INNTPC

    Various ESP performance improvement programmes

    have been followed in NTPC stations where SPMemissions were reported to be high.The modificationprogrammes followed are:

    Additional ESPs have been retrofitted at BADARPUR TPSSt.-I, TALCHER TPS St-II & BALCO CPP (All four units).

    EPMS have been installed at following stations :SINGRAULI STPS (St-I& II) , KORBA STPS (St I&II) ,RAMAGUNDAM STPS (St-I&II) , RIHAND STPS ,VINDHYACHAL STPS , FGUTPS & FARAKKA STPS (St I ).

    Also dummy fields filling done at SINGRAULI (St I) andRAMAGUNDAM (St I) UNITS .

    By providing EPMS in above seven stations , there hasbeen very high reduction in energy consumption (Up to70 %) and marginal reduction in SPM emission (Up to

    22%).

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    STACK SPM EMISSIONS BEFOREAND AFTER RETROFITTING

    ADDITIONAL ESPs

    SL.

    NO.

    STATION SPM BEFORE

    RETROFITTING

    SPM AFTER

    RETROFITTING

    1. Badarpur

    (st I)

    AROUND 5000 136-142

    2. TALCHER TPS(St -II)

    1400-1800 105-130

    3. BALCO 1100-1500 160-290

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    PERFORMANCE OF ESPsIn spite of retrofitting/renovation programmes , the SPM

    emission of following stations are still exceeding thestatutory limit of 150mg/NM3 as per EP-AIR ACT 1981:

    STATION DESIGN

    SPM

    PRESENT

    SPM

    DESIGN

    EFFICIENCY

    RIHAND I 100 200-350 99.81

    BALCO 150 160-290 99.6

    KORBA I 300 180-264 99.51

    KORBA II 396 180-264 99.52

    FARAKKA I 550 180-290 99.53

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    REMEDIAL TECHNOLOGIESTO BE ADOPTED

    STATION UNITS TECHNOLOGY

    RIHAND 2*500 MW WF , FGC

    KORBA 1*200 MW2*200 +3*500 MW

    SCFGC

    BALCO 4*67.5 MW FGC

    FARAKKA 3*200 MW

    2*500 MW

    FGC

    MODIFICATIONTHROUGH ANSALDO

    LEGEND:WF :WATER FOGGING

    FGC : FLUE GAS CONDITIONING

    SC : SODIUM CONDITIONING