coha update jin xu. update 2003 and 2004 back-trajectories – done pmf modeling by groups using...

25
COHA Update Jin Xu

Upload: augustine-pitts

Post on 01-Jan-2016

218 views

Category:

Documents


4 download

TRANSCRIPT

Page 1: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

COHA Update

Jin Xu

Page 2: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Update• 2003 and 2004 back-trajectories – done• PMF modeling by groups using 2000 to 2004

IMPROVE data – done• Analysis of PMF results – ongoing

– General analysis and discussion – decide how many factors are reasonable for each group, will finish soon. More modeling calculation will be done if necessary.

– Trajectory analysis – ongoing– Spatial and temporal analysis – ongoing, may result in

regrouping of the sites and more PMF modeling– Episode analysis– Other analysis – carbon-based factors – ongoing

• 2002 fire database from WRAP, other years from Dr. Tim Brown’s group in DRI. Satellite data and images archived.

• Case study• Similar trajectory analysis as for the causes of dust resultant

haze

Page 3: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results
Page 4: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Receptor Modeling - Positive Matrix Factorization (PMF) and Chemical Mass Balance (CMB)

• Mathematical technique for determining the contributions of various sources to a given sample of air

jijii

j

j

i I

I

I

SPSPSP

SPSPSP

SPSPSP

C

C

C

2

1

21

22221

11211

2

1

SPij – Source Profile: Emissions of compound i from source j (100%).

Ij – Contribution of source j (g/m3).

Ci – Concentration of compound i (g/m3).

CMB PMF

Input Both C and SP Only C

Output Only I Both SP and I

Page 5: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Receptor Modeling - Positive Matrix Factorization (PMF) and Chemical Mass Balance (CMB) (Cont.)

CMB PMF

Assumptions Composition of source emissions is relatively constant

Emissions do not react or selectively deposit between source and receptor (mass is conserved)

Source profiles are linearly independent

For CMB, all major sources should be included in the model

Limitations Reactive compounds

Only identifies categories of sources, not individual sources

Identifies only relative contributions, not mass emission rates

Limitations Must know source profiles

High sensitivity to uncertainty / error in source profiles

Omission of a source can lead to large errors

Pure statistical model

large number of samples (100+) are needed

Need to make arbitrary decision of the number of sources (factors)

Page 6: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Number of Factors – Southern CA

• No negative regression coefficient(s) between PM2.5 mass and G factors.

• The sum of the scaled profiles should be less than unity (well, < 2).

• Other PMF output parameters:

Page 7: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Number of Factors – Southern CA

)(max1

1

..1

n

iijnmjrIM

rij = eij / Sij, while eij = xij - GF

))((max1

211

...1

n

ijijnmjrrIS

Species having the least fit

Species having the most imprecise fit

IM

0

1

2

3

4

5

6

0 5 10 15

IM

IS

0

2

4

6

8

10

12

0 5 10 15

IS

Page 8: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Number of Factors – Southern CA

Rotmat – a matrix resulting from each PMF computation, is used for detecting the degree of rotational freedom of the factorsLargest element in rotational matrix (Mrotmat) is used to show worst case in rotational freedom

Mrotmat

00.010.020.030.040.050.060.070.08

0 5 10 15

Mrotmat

Page 9: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Number of Factors – Southern CA

If there are no outliers, Q should be approximately equal to the number of entries in the data array. Possible reasons for an excessively large Q:1.The original std-dev are too small2.There are many outliers3.More factors are needed4.The data do not obey a bi-linear model, i.e. PMF is not a suitable model5.The iteration did not converge or converged to a local minimum.

Q

0

200000

400000

0 5 10 15

Q

For a 6 factor modeling, 3.6% of the data entries are outliers, i.e. eij/sij > 4.

Page 10: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Number of Factors – Southern CA

• Factor 5 – 7 should be used.

• How many factors between 5 and 7 should we choose? – Judgement based on literature, known source profiles, and experience

Page 11: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

PMF for Southern CA – 6 factors

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

Dust

Smoke

Secondary Nitrate

Sea Salt / Shipping Emissions

Urban/Mobile

Secondary Sulfate

Page 12: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Average Contribution of Each Factor to PM2.5

0

2

4

6

8

PM

2.5

Ma

ss

(u

g/m

3)

Secondary Sulfate 2.09 0.80 0.87 0.93

Urban/Mobile 0.15 0.10 0.14 0.16

Sea Salt/Shipping 1.80 1.65 0.98 1.13

Secondary Nitrate 1.46 1.18 1.15 2.15

Smoke 1.10 0.79 0.84 1.04

Dust 0.94 1.11 0.72 0.83

AGTI1 JOSH1 SAGA1 SAGO1

Page 13: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Time Series of Factor Contributions at JOSH1

0

2

4

6

8

10

12

14

16

18

3/1/

2000

5/1/

2000

7/1/

2000

9/1/

2000

11/1

/200

0

1/1/

2001

3/1/

2001

5/1/

2001

7/1/

2001

9/1/

2001

11/1

/200

1

1/1/

2002

3/1/

2002

5/1/

2002

7/1/

2002

9/1/

2002

11/1

/200

2

1/1/

2003

3/1/

2003

5/1/

2003

7/1/

2003

9/1/

2003

11/1

/200

3

1/1/

2004

3/1/

2004

5/1/

2004

7/1/

2004

Dust

Smoke

Secondary Nitrate

Sea Salt/Shipping

Urban/Mobile

Secondary Sulfate

Dust Episodes Secondary Nitrate Episodes Shipping Pollution Episodes

Page 14: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Comparison of Group Modeling (Blue) and SAGA1 Individual Modeling (Red)

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

AS BR CA EC1 EC2 EC3 OC1 OC2 OC3 OC4 OP CL CR CU H FE PB MG MN NI NO3 P K RB SE SI NA SR S TI V ZN ZR

0.0001

0.001

0.01

0.1

1

Dust

Smoke ?

Secondary Nitrate

Sea Salt / Shipping Emissions ?

Diesel / Urban

Secondary Sulfate

Page 15: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Contribution of Each Factor to PM2.5 Mass in SAGA1

0.00

0.20

0.40

0.60

0.80

1.00

1.20

1.40

1.60

1.80

1 2 3 4 5 6

Group Modeling

SAGA1DustSmoke

Secondary Nitrate

Urban/Mobile

Sea Salt / Shipping

Secondary Sulfate

g/m3

Page 16: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

SAGA1 Trajectory Regression Analysis Results

Page 17: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Trajectory Analysis of SAGA1 Individual PMF Modeling Results

PMF Weighted - Unweighted

PMF Weighted / Unweighted

Page 18: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Trajectory Analysis of SAGA1 Group PMF Modeling Results

PMF Weighted - Unweighted

PMF Weighted / Unweighted

Page 19: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Contribution of Each Factor to PM2.5 Mass in JOSH1

0.00E+00

2.00E-01

4.00E-01

6.00E-01

8.00E-01

1.00E+00

1.20E+00

1.40E+00

1.60E+00

1.80E+00

Dust Smoke SecondaryNitrate

SeaSalt/Shipping

Diesel/Urban SecondarySulfate

Group Modeling

Individual Modeling

g/m3

Page 20: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

JOSH1 Trajectory Regression Analysis Results

Page 21: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Contribution of Each Factor to PM2.5 Mass in AGTI1

0.00E+00

5.00E-01

1.00E+00

1.50E+00

2.00E+00

2.50E+00

Dust Smoke SecondaryNitrate

SeaSalt/Shipping

Urban/Mobile SecondarySulfate

Group Modeling

Individual Modeling

g/m3

Page 22: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

AGTI1 Trajectory Regression Analysis Results

Page 23: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Contribution of Each Factor to PM2.5 Mass in SAGO1

-5.00E-01

0.00E+00

5.00E-01

1.00E+00

1.50E+00

2.00E+00

2.50E+00

3.00E+00

Dust Smoke SecondaryNitrate

SeaSalt/Shipping

Urban/Mobile SecondarySulfate

Group Modeling

Individual Modeling

g/m3

Page 24: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Group modeling is doing a better job

for the Southern CA group?• Clearer factors due to strong source

signatures in certain sites in the group (especially true for IMPROVE sites because they are in remote areas with well mixed pollutions)

• Partially solved the collinearity problem of some sources

• More data

Page 25: COHA Update Jin Xu. Update 2003 and 2004 back-trajectories – done PMF modeling by groups using 2000 to 2004 IMPROVE data – done Analysis of PMF results

Trajectory Analysis of PMF Results