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Shock wave propagation across the column of dusted glow discharge in different gases. A.S.Baryshnikov, I.V.Basargin, M.V.Chistyakova Ioffe Physico-Technical Institute Russia

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Shock wave propagation across the column of dusted glow discharge in different gases. A.S.Baryshnikov, I.V.Basargin, M.V.Chistyakova Ioffe Physico-Technical Institute Russia. PROBLEM. Reducing a drag of air vehicles (due to destabilization and destruction of bow shock wave ), - PowerPoint PPT Presentation

Citation preview

Page 1: Shock wave propagation across the column of dusted glow discharge in different gases

Shock wave propagation across the column of

dusted glow discharge in different gases

ASBaryshnikov IVBasargin MVChistyakova

Ioffe Physico-Technical Institute

Russia

PROBLEMbull Reducing a drag of air vehicles (due to destabilization and destruction of bow

shock wave)

Moreover Temperature and Heat Flux to surface are dropping

bull Controlling a flight of them

bull Without great energy deposition TMB 2010 2

EFFECT OF SHOCK WAVE INSTABILITY DUE TO

ENDOTHEMIC REACTION bull EARLIER well known instability due to

exothermic reaction detonation combustion

Gas Temperature increases

bull NOW Dissociation Ionization Excitation of inner degrees of energy

Gas Temperature dropsTMB 2010

3

Problem

bull When velocity of body riches the amount at which Chemical dissociation (not exothermic reaction) takes the place

bull Just a disturbances on bow shock wave are arising

bull The flow behind body becomes disturbed in such manner as for turbulent flow

bull Itrsquos important that such rdquoturbulencerdquo is outside the wake flow region

1 1 Flow of the chemically reacting stable polyatomic gases (CF2Cl2)

TMB 2010 4

Fig1 Instability of bow shock wave in front of segmental body Flow Mach number М0=39 Gas CF2Cl2

Pressure in flow Р0=38middot10 4 Pа

Wake turbulence

Single vortex

Disturbance on bow shock wave

М0=39

5TMB 2010

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
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  • Slide 14
  • Slide 15
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  • Slide 17
  • Slide 18
  • Slide 19
  • Slide 20
  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 2: Shock wave propagation across the column of dusted glow discharge in different gases

PROBLEMbull Reducing a drag of air vehicles (due to destabilization and destruction of bow

shock wave)

Moreover Temperature and Heat Flux to surface are dropping

bull Controlling a flight of them

bull Without great energy deposition TMB 2010 2

EFFECT OF SHOCK WAVE INSTABILITY DUE TO

ENDOTHEMIC REACTION bull EARLIER well known instability due to

exothermic reaction detonation combustion

Gas Temperature increases

bull NOW Dissociation Ionization Excitation of inner degrees of energy

Gas Temperature dropsTMB 2010

3

Problem

bull When velocity of body riches the amount at which Chemical dissociation (not exothermic reaction) takes the place

bull Just a disturbances on bow shock wave are arising

bull The flow behind body becomes disturbed in such manner as for turbulent flow

bull Itrsquos important that such rdquoturbulencerdquo is outside the wake flow region

1 1 Flow of the chemically reacting stable polyatomic gases (CF2Cl2)

TMB 2010 4

Fig1 Instability of bow shock wave in front of segmental body Flow Mach number М0=39 Gas CF2Cl2

Pressure in flow Р0=38middot10 4 Pа

Wake turbulence

Single vortex

Disturbance on bow shock wave

М0=39

5TMB 2010

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
  • Slide 11
  • Slide 12
  • Slide 13
  • Slide 14
  • Slide 15
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  • Slide 17
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  • Slide 19
  • Slide 20
  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 3: Shock wave propagation across the column of dusted glow discharge in different gases

EFFECT OF SHOCK WAVE INSTABILITY DUE TO

ENDOTHEMIC REACTION bull EARLIER well known instability due to

exothermic reaction detonation combustion

Gas Temperature increases

bull NOW Dissociation Ionization Excitation of inner degrees of energy

Gas Temperature dropsTMB 2010

3

Problem

bull When velocity of body riches the amount at which Chemical dissociation (not exothermic reaction) takes the place

bull Just a disturbances on bow shock wave are arising

bull The flow behind body becomes disturbed in such manner as for turbulent flow

bull Itrsquos important that such rdquoturbulencerdquo is outside the wake flow region

1 1 Flow of the chemically reacting stable polyatomic gases (CF2Cl2)

TMB 2010 4

Fig1 Instability of bow shock wave in front of segmental body Flow Mach number М0=39 Gas CF2Cl2

Pressure in flow Р0=38middot10 4 Pа

Wake turbulence

Single vortex

Disturbance on bow shock wave

М0=39

5TMB 2010

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
  • Slide 11
  • Slide 12
  • Slide 13
  • Slide 14
  • Slide 15
  • Slide 16
  • Slide 17
  • Slide 18
  • Slide 19
  • Slide 20
  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 4: Shock wave propagation across the column of dusted glow discharge in different gases

Problem

bull When velocity of body riches the amount at which Chemical dissociation (not exothermic reaction) takes the place

bull Just a disturbances on bow shock wave are arising

bull The flow behind body becomes disturbed in such manner as for turbulent flow

bull Itrsquos important that such rdquoturbulencerdquo is outside the wake flow region

1 1 Flow of the chemically reacting stable polyatomic gases (CF2Cl2)

TMB 2010 4

Fig1 Instability of bow shock wave in front of segmental body Flow Mach number М0=39 Gas CF2Cl2

Pressure in flow Р0=38middot10 4 Pа

Wake turbulence

Single vortex

Disturbance on bow shock wave

М0=39

5TMB 2010

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
  • Slide 11
  • Slide 12
  • Slide 13
  • Slide 14
  • Slide 15
  • Slide 16
  • Slide 17
  • Slide 18
  • Slide 19
  • Slide 20
  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 5: Shock wave propagation across the column of dusted glow discharge in different gases

Fig1 Instability of bow shock wave in front of segmental body Flow Mach number М0=39 Gas CF2Cl2

Pressure in flow Р0=38middot10 4 Pа

Wake turbulence

Single vortex

Disturbance on bow shock wave

М0=39

5TMB 2010

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
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  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
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  • Slide 22
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  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 6: Shock wave propagation across the column of dusted glow discharge in different gases

Fig2 Instability of bow shock wave in front of segmental body Flow Mach number М0=61 Gas CF2Cl2

Pressure in flow Р0=43middot10 4 Pа

М0=61

6TMB 2010

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
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  • Slide 13
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  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 7: Shock wave propagation across the column of dusted glow discharge in different gases

bull Could - for Air for high Mach number (2-5)

(Mach number defined to the speed of sound

of the uncharged heavy particles)

22 Plasma is active mediumPlasma is active mediumCould energy release to translation Could energy release to translation

freedom degrees freedom degrees

TMB 2010 7

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
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  • Slide 13
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  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 8: Shock wave propagation across the column of dusted glow discharge in different gases

Behind fast shock wave

pressure growth is proportional to +1 (ndashratio of specific thermo capacities

which in plasma is close to 1)

bullTemperature grows much less bullbecause its growth is proportional to -1

bullElectron concentration arises bullwith temperature much faster

bullbut it drops with the pressure growth

210423 8TMB 2010

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
  • Slide 11
  • Slide 12
  • Slide 13
  • Slide 14
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  • Slide 17
  • Slide 18
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  • Slide 20
  • Slide 21
  • Slide 22
  • Slide 23
  • Slide 24
  • Slide 25
  • Slide 26
  • Slide 27
Page 9: Shock wave propagation across the column of dusted glow discharge in different gases

in according the Huguenot laws

1

1

1

2 20

MPP

22

2

0

1

1

1

2

M

M

TT

1

1

2 2M

22 dM

dT

T

K

dM

dP

P

KRg

1

1

1

2

1

21

1

21

1

2

1

1)(1

1

2)(2

24

0

2

0

0

MM

MT

T

T

KI

P

PRTK og

Derivative will take the form

Equilibrium concentration of binary reaction )(TKne

equilibrium constant Tk

I

BeTTK

)(

2dM

dne

210423 9

α

TMB 2010

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
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  • Slide 24
  • Slide 25
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  • Slide 27
Page 10: Shock wave propagation across the column of dusted glow discharge in different gases

If for any Mach number will be lt than calculation curve

electron concentration will be reducing with rising of Mwhich could correspond to recombination behind shock wave or to the

flash of radiation

power index of temperature of preexponential factor in equilibrium constant

3

Mach number

Region of instability

CpCv in plasma

210423 10TMB 2010

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

  • Slide 1
  • Slide 2
  • Slide 3
  • Slide 4
  • Slide 5
  • Slide 6
  • Slide 7
  • Slide 8
  • Slide 9
  • Slide 10
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Page 11: Shock wave propagation across the column of dusted glow discharge in different gases

bull Here is a stationary plasma of glow discharge

bull Experiments was made in the installation of electromagnetic shock tube

bull for low transonic Mach number in plasma (hot region) (Mach number is defined to the speed of sound of the slight disturbances of the density of the uncharged heavy particles in hot plasma region)

3 3 Low speed plasma flowLow speed plasma flow

TMB 2010 11

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 12: Shock wave propagation across the column of dusted glow discharge in different gases

Installation

1- camera 2- electromagnetic shock tube (EMST) 3- central electrode of EMST 4- flanges from organic glass 5- the anode 6- cathode 7- receiver 8 - rod 9- piezoelectric pickup 10- quartz rod 11- gate of evacuation 12- pump 13- gate of gas inlet 14- manometers

Experimental camera

Electromagnetic

shock tube

piezoelectric pickup

piezoelectric pickup

PUMPanode

TMB 2010 12

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 13: Shock wave propagation across the column of dusted glow discharge in different gases

Regimes

bullMaximum of shock wave speed = 2 kms

bullThe gas pressure in camera was 4103 Pa (36 Torr)

bullIn experiments we have a time distribution of signal from piezo pickup oriented towards the shock wave(It corresponds to pressure distribution behind the shock

wave )

bullElectrical current in discharge = 1 A up to 25Abull Voltage of discharge = 1 kV up to 10 kV

TMB 201013

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 14: Shock wave propagation across the column of dusted glow discharge in different gases

Usual electron temperature distribution across the positive column of glow discharge

1012 1cm3

Electron temperature has the same profile ndash plate ndash 1 eV

TMB 201014

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 15: Shock wave propagation across the column of dusted glow discharge in different gases

Usual gas temperature distribution across the positive column of

1200 K

TMB 2010 15

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 16: Shock wave propagation across the column of dusted glow discharge in different gases

Signal from piezo pickup without the plasma in hot air (usual triangular form)

TMB 2010 16

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 17: Shock wave propagation across the column of dusted glow discharge in different gases

Signal from piezo pickup in the plasma (two wave form)

TMB 2010 17

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 18: Shock wave propagation across the column of dusted glow discharge in different gases

bull Low dustiness - preliminary results

bull Dust concentration is about 20 mg per cubic meter that is comparable with natural concentration

TMB 2010 18

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 19: Shock wave propagation across the column of dusted glow discharge in different gases

Weak influence of dustiness

for the small concentration (in ten times less) of dust

(20mg in m3 emission of laser as absorbed by 4 )2- maximum dustiness (solid gradient line)

1- dustiness is two times lower (dashed line) 0 - without the dust (solid line)

in the center of discharge column the initial velocity of shock wave

Is the same 16 kms

Air N2

TMB 201019

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 20: Shock wave propagation across the column of dusted glow discharge in different gases

bull High dustiness - refined results

bull Dust concentration is about 200 mg per cubic meter

bull Refined bull with increased measurement precisionbull by reducingof time discretness at signal recordingbull to order from 200 ns to 20 ns bull It enables to average number experiments at each

registration pointbull (In this study there was an averaging of 10 experiments)

TMB 2010 20

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 21: Shock wave propagation across the column of dusted glow discharge in different gases

TMB 2010 21

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 22: Shock wave propagation across the column of dusted glow discharge in different gases

TMB 2010 22

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 23: Shock wave propagation across the column of dusted glow discharge in different gases

TMB 2010 23

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 24: Shock wave propagation across the column of dusted glow discharge in different gases

1)For carbon dust Weak influence of dustiness

for the small concentration of dust (20mg per m3)

as for Air and for N2 and Ar

2)BUT THERE IS INFLUENCE for great concentration( in ten

time greater)

21) No influence for Air without plasma

22) No appreciable influence in Air plasma

23) Great influence for Argon plasma

Summary

TMB 2010 24

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 25: Shock wave propagation across the column of dusted glow discharge in different gases

Further

bull Investigation

A) Strange strong dust dependence on the type of gas

B) Dust dependence on the kind of dust

C) Dust dependence in course of time after disconnection of discharge

TMB 2010 25

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 26: Shock wave propagation across the column of dusted glow discharge in different gases

bull Some part of this work was made under the financial support of Russian Foundation for Basic Research

project N 06-08-00663-а

TMB 2010 26

Thank you very much

TMB 2010 27

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Page 27: Shock wave propagation across the column of dusted glow discharge in different gases

Thank you very much

TMB 2010 27

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