/
SPECTRAL LINE SHAPES  IN THE SPECTRAL LINE SHAPES  IN THE

SPECTRAL LINE SHAPES IN THE - PowerPoint Presentation

conchita-marotz
conchita-marotz . @conchita-marotz
Follow
365 views
Uploaded On 2018-03-07

SPECTRAL LINE SHAPES IN THE - PPT Presentation

ν 3 Q BRANCH OF 12 CH 4 NEAR 33 µm V MALATHY DEVI and D CHRIS BENNER The College of William and Mary Williamsburg VA USA ROBERT R GAMACHE University of Massachusetts Lowell Lowell MA USA ID: 641955

air line broadened spectra line air spectra broadened parameters jqsrt bus ch4 mixing 296 transitions fit coefficients positions measurements

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "SPECTRAL LINE SHAPES IN THE" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

SPECTRAL LINE SHAPES IN THE ν3 Q BRANCH OF 12CH4 NEAR 3.3 µm

V. MALATHY DEVI and D. CHRIS BENNER The College of William and Mary, Williamsburg, VA, U.S.A.ROBERT R. GAMACHE University of Massachusetts Lowell, Lowell, MA, U.S.A.MARY ANN H. SMITH NASA Langley Research Center, Hampton, VA, U.S.A.ROBERT L. SAMS Pacific Northwest National Laboratory, Richland, WA, U.S.A.

FA01

72nd

International Symposium on Molecular Spectroscopy, June

19-23, 2017Slide2

2

Present Work: Analyze air-broadened CH4 spectra recorded at room temperature to determine ν3 Q branch line shape parameters needed for terrestrial atmospheric retrievals. Since air-broadened and N2

-broadened line shape parameters for CH

4

are very similar (within 2% according to Tran et al. [2006]), these results are relevant to all planetary atmospheres that are predominantly N2.

Self- and foreign-broadened CH4 line parameters are needed for quantitative analysis of spectroscopic observations of Earth and planetary atmospheres, both to retrieve atmospheric methane abundances and to model the CH4 absorption overlapping features of other species.

Previous lab studies of CH

4

broadening with line mixing have involved mostly P and R branch manifolds, and only a few studies of Q-branches have been reported: most recently

ν

2

+

ν

3

[

Malathy

Devi

et

al

., JQSRT

152 (2015)

149-165] and

2

ν

3

[

Malathy

Devi

et al

., JQSRT 177 (2016) 152-169].

Previous studies of line shapes in the CH

4

ν

3

band system:

See

review of measurements

in the article of Brown

et al

. [

JQSRT

130 (2013) 201-219

] and references therein.

High-resolution

ν

3

Q-branch line mixing

measurements (N

2

, O

2

, H

2

, He,

Ar

, and CH

4

) by Pine [

J. Chem. Phys.

97 (1992)

773-785

] and Pine and

Gabard

[

J. Mol.

Spectrosc

.

217 (2003) 105-114].

Tran

et al

. [JQSRT 101 (2006) 284-305] have

modeled

line mixing for

N

2

- and air-broadening in the

ν

4

and

ν

3

bands, including Q-branches.Slide3

3Summary of Lab Spectra Used in this Analysis

aSpectrum file names are given for authors’ identification. All spectra except #3 were recorded using the McMath-Pierce FTS at a resolution of 0.01 cm-1. Experimental details are in Benner et al. [JQSRT 50 (1993) 65-89].Spectrum #3

was recorded using the

Bruker IFS 120 HR FTS

at Pacific Northwest National Laboratory at a resolution of 0.0011 cm-1. Details of the spectrometer setup are in Malathy Devi et al. [JQSRT 82 (2003)

319-341].1 atm = 101.3kPa = 760 Torr.Serial #Spectraa

Cell length

(m

)

Total Pressure

(

Torr

)

Sample temperature

(K

)

Volume mixing ratio of CH

4

CH

4

1

150x3000.bus

0.25

1.065

296.95

1.0

2

164x3000.bus

1.5

0.408

296.05

1.0

3

922x3000.ars

0.1995

1.068

298.20

1.0

Air-broadened

CH

4

4

154x3000.bus

0.05

75.3

298.25

0.00954

5

153x3000.bus

0.05

150.51

298.35

0.00954

6

152x3000.bus

0.05

301.0

298.35

0.0097

7

151x3000.bus

0.05

500.20

298.25

0.0097

8

149x3000.bus

0.25

50.30

296.75

0.0098

9

148x3000.bus

0.25

125.30

296.65

0.0098

10

147x3000.bus

0.25

250.50

296.55

0.0098

11

146x3000.bus

0.25

400.60

296.35

0.0098

12

163x3000.bus

1.50

60.60

296.15

0.01

13

162x2000.bus

1.50

110.60

296.15

0.01Slide4

Sample Spectra4Resolution:0.01 cm-1 (upper)0.0011 cm-1 (lower)Slide5

5Analysis

Nonlinear least squares multispectrum fitting [Benner et al., JQSRT 53 (1995) 705-721; Letchworth and Benner, JQSRT 107 (2007) 173-192] is used to retrieve spectroscopic parameters consistent with the entire set of laboratory spectra. All spectra are calibrated to the same wavenumber scale

with reference

to H

2O line positions [Benner et al., JQSRT 50 (1993) 65-89].

Initial line list taken from HITRAN2012 [L. S. Rothman et al., JQSRT 130 (2013) 4-50]. Since natural-abundance CH4 samples were used, both 12CH4 and 13CH4

transitions are included.

Voigt

line shape is initially

assumed, and

quadratic speed dependence

is included if residuals indicate it is necessary;

line mixing

is allowed for pairs of lines expected to

mix, or if residuals show evidence of mixing.

Room-temperature

self-broadened spectra

are fit first; then the

air-broadened spectra are added sequentially in order of increasing pressure.Slide6

6Observed Air- and Self-Broadened CH4 Spectra

and Residuals from the Multispectrum FitA total of 13 spectra were fit.Black tick marks in top panel represent the positions of more than 3160 transitions included in the fit.Parameters were retrieved for about 300 transitions of 12CH4

and

13

CH4.Slide7

7Air- and Self-Broadened CH4 Spectra from the Fit: Expanded Scale

Black tick marks at the top of each panel represent the positions of transitions included in the fit.Slide8

8Spectra and Residuals: HITRAN2012 vs. the Multispectrum Fit

A total of 13 spectra were fit.Top panel: Observed spectra. Black tick marks at top represent the positions of more than 3160 transitions included in the fit.Middle panel: Residuals with all line parameters fixed to HITRAN 2012 values.Bottom panel: Residuals from fit to retrieve line parameters for about 300 transitions, including line mixing for 14 pairs of transitions.Slide9

Summary of measured parameters in the Q branch9

a The number of measured positions (in cm-1) is less than the measured line intensities; positions of some transitions were held fixed due to their weakness, blends and proximity to stronger lines.bLine intensity in cm-1/(molecule cm-2)

at 296 K.

c

Lorentz half-width and pressure-shift coefficients and the off-diagonal relaxation matrix elements in units of cm-1

atm-1 at 296 K.d(CH4-air) collisional line mixing coefficients were measured for 14 transition pairs.Parameters

Number of measurements

(

12

CH

4

)

Parameters

Number of measurements

(

13

CH

4

)

Position

(

ν

)

a

252

Position

(

ν

)

a

50

Intensity (S)

b

274

Intensity (S)b51Lorentz air-broadened half-width coefficientc (bL0)103Air-pressure-shiftcoefficientc (86Off-diagonal relaxation matrix element coefficientsc,d(CH4-air) collisions 14  

Parameters

Number of measurements

(

12

CH

4

)

Parameters

Number of measurements

(

13

CH

4

)

Position

(

ν

)

a

252

Position

(

ν

)

a

50

Intensity (S)

b

274

Intensity (

S)

b

51

Lorentz air-broadened half-width

coefficient

c

(b

L

0

)

103

86

Off-diagonal relaxation matrix element

coefficients

c,d

(CH

4

-air) collisions

14

 

 Slide10

10Results: Comparison with HITRAN2012 parametersSlide11

11Results: Comparison of Air-Broadening Coefficients

References: Rothman et al. [JQSRT 130 (2013) 4-50]; Pine and Gabard [J. Mol. Spectrosc. 217 (2003) 105-114]. Mean ratios are PS/(Other Ref.).Slide12

12Results: Comparison of Line Mixing Parametersa

See Brown et al. [JQSRT 130 (2013) 201-219].bLine positions from present study.cThe off-diagonal relaxation matrix element coefficients measured for the CH4-air collision system in the present study. dThe off-diagonal relaxation matrix element coefficients calculated

for

the CH

4-air collision system using the formalism in Tran et al. [JQSRT 101

(2006) 284-305].Quantum IdentificationaLine positionb

Off-diagonal relaxation matrix elements,

W

ij

(cm

-

1

atm

-

1

at 296 K)

J

C

a

J

C

a

(

cm-1)CH4-air Meas.cCH4-air Calc.d12 F1 4412 F2 4612 F2 112 F1 23012.029219(7)2012.062725(7)0.00166(13)Not available13 F1 5113 F2 5013 F2 313 F1 43012.503417(11)3012.710279(10)0.01797(69)Not available12 F2 4712 F1 4612 F1 312 F2 33013.511448(8)3013.407770(7)0.01778(19)Not available12 A2 1512 A1 1712 A1 212 A2 13013.592598(5)3013.167070(6)0.02735(45)0.0118611 F1 4411 F2 42

11 F2 3

11 F1 3

3014.060488(5)

3014.344097(9)

0.02846(36)

0.01020

10 F1 39

10 F2 39

10 F2 2

10 F1 1

3014.095407(4)

3014.171700(4)

0.00255(11)

0.00058

10 F2 40

10 F1 38

10 F1 2

10 F2 1

3014.838247(4)

3015.091512(4)

0.01794(32)

0.00101

9 F2 35

9 F1 36

9 F1 3

9 F2 2

3015.590760(4)

3015.706192(4)

0.01447(17)

0.00714

6 A1 9

6 A2 8

6 A2 1

6 A1 1

3016.565296(3)

3017.466013(2)

0.00679(29)

0.00723

7 F1 29

7 F2 27

7 F2 2

7 F1 2

3016.640437(3)

3016.939553(3)

0.00658(15)

0.00509

5 F219

5 F1 21

5 F1 1

5 F2 1

3017.163091(4)

3017.266616(3)

0.00381(10)

0.00029

6 F1 23

6 F2 25

6 F2 2

6 F1 1

3017.227925(3)

3017.345780(3)

0.01179(11)

0.00451

2 F1 8

1 F2 5

2 F2 1

1 F1 1

3018.650122(3)

3018.824378(3)

0.00434(10)

0.00433

3 F2 12

3 F1 14

3 F1 1

3 F2 1

3018.242053(3)

3018.358514(3)

0.00309(7)

0.00359Slide13

13SummaryThe present study reports

the first experimental measurements of air-broadened half-width and pressure shift coefficients for the ν3 band Q branch transitions of 12CH4. Also the first experimental measurements of the off-diagonal relaxation matrix element coefficients for line mixing involving CH4-air collisions.Line

positions and intensities

were also measured for

over 250 12CH4 and 50

13CH4 transitions in the Q branch region (3000-3023 cm-1), by applying a multispectrum fitting technique to 13 room-temperature spectra recorded with two different Fourier transform spectrometers.

Future Work

Expand

the

analysis to include other

air- and self-broadened laboratory spectra in

the

ν

3

region recorded at lower temperatures.

Pursue

similar efforts involving other

broadening gases such as H

2

, N

2

,

CO

2

and

He,

including temperature dependences of width, shift and line mixing coefficients.

Final results will be

contributed

future spectroscopic database

updates.Slide14

14Acknowledgments

The research at NASA Langley Research Center, and the College of William and Mary (Grant NNX15AM01G) is supported by the Atmospheric Composition Laboratory Research program of the National Aeronautics and Space Administration. Research performed at the University of Massachusetts Lowell is supported by the National Science Foundation through Grant No. AGS-1622676.We thank Mike Dulick, Detrick Branston, Claude Plymate and the late Jeremy Wagner of the National Solar Observatory for their assistance in recording spectra at Kitt Peak over many years. NSO is operated by the Association of Universities for Research in Astronomy, Inc. (AURA), under contract with the National Science Foundation.