simultaneous profile measurements of bro, oclo and no 2 in the polar vortex
DESCRIPTION
Simultaneous profile measurements of BrO, OClO and NO 2 in the polar vortex. Chris Sioris and Kelly Chance Smithsonian Astrophysical Observatory. Method: Two-step retrieval. Step 1 : Spectral fit. BrO (Wilmouth et al.) OClO (Wahner et al.) - PowerPoint PPT PresentationTRANSCRIPT
Simultaneous profile measurements of BrO, OClO and
NO2 in the polar vortex
Chris Sioris and Kelly ChanceSmithsonian Astrophysical
Observatory
Method: Two-step retrieval
Step 1: Spectral fit
-2.40
-2.35
-2.30
-2.25
-2.20
-2.15
342 344 346 348 350 352 354 356 358 360 362
Wavelength (nm)
ln(I
0/I)
fit obs
Retrieved gas Interference fitting window (nm) # of pixels polynomial I0 TH range (km)BrO NO2, O3, tilt, -shift 344.09-360.03 146 cubic 33-70OClO BrO, NO2, O3, tilt, -shift 357.37-381.12 224 cubic 33-70NO2 O4, O3, -shift, Ring 434.63-494.87 255 cubic 46-70
BrO (Wilmouth et al.) OClO (Wahner et al.) NO2 and O3 (Bogumil et al., 203, 223, 243 K)tilt (Sioris et al., uses Chance-Kurucz solar spectrum)
-0.02
-0.015
-0.01
-0.005
0
0.005
0.01
0.015
0.02
344 346 348 350 352 354 356 358 360
BrOO3tiltNO2
Sample fitted optical depths, BrO fitting window, at TH=10 km in Arctic vortex
Modelled and measured SCDs
BrO SCD (molec/cm2)
0 1e+14 2e+14 3e+14 4e+14 5e+14 6e+14
TH (k
m)
10
12
14
16
18
20
22
24
26
28
modelledmeasured
Step 2: Vertical “fitting” of SCD profile
-pointing correction: 305 nm knee-Forward RTM: McLinden et al., 2002-inversion: modified Chahine’s method (Sioris et al., 2003)
for OClO, retrieval is done on a 1 km altitude grid using measurement TH grid (~3.3 km sampling)
Retrieved gas TH range (km) z range (km) SCD err #D err VCD errBrO 10-33 15-29 ~20% <55% <30%OClO 15-29 15-27 20% <30% <30%NO2 10-42 11-41 <1% <6% <2%
75 N, Oct. 26th, 2002
NO2 number density (molec/cm3)
0.0 2.0e+8 4.0e+8 6.0e+8 8.0e+8 1.0e+9 1.2e+9 1.4e+9 1.6e+9 1.8e+9
Alti
tude
(km
)
20
22
24
26
28
30
32
34
36
38
40
SAGE III SCIA SZA=90º SCIA w/kn SZA=86º SCIA 86 w/o kn
NO2 Validation
Typical agreement based on comparisons with OSIRIS, SAGE III, SAOZ, and HALOE is 7% on VCD and 14% profile (15-41 km)
Aire sur l'Adour (43.7º N 0.3º E), Oct 1st, 2002
BrO number density (cm-3)0 1e+7 2e+7 3e+7 4e+7 5e+7 6e+7
Alti
tude
(km
)
14
16
18
20
22
24
26
28
30
SCIAMACHY (SZA=58°, am)SCIAMACHY (SZA=83°, pm) SAOZ-BrO (SZA=83°, pm) SAOZ (SZA=83°, pm)
BrO validation
BrO VCD (15-27 km) agrees to <5% and profile to 7% with SAOZ-BrO (despite poor temporal coincidence of ~10 hours)At ~23 km, BrO: 26 pptv (10 am LT), 16-20 pptv (before sunset, ascent)
50
30
20
15
10
7
5
3
80 74 66 59 51 44 36 28 20 13 6 -2 -10
-18
-25
-33
-41
-48
-56
Pre
ssur
e (m
b)
Latitude (º)
0.0E+0
5.0E+8
1.0E+9
1.5E+9
2.0E+9
2.5E+9
50
30
20
15
10
7
5
3
80 74 66 59 51 44 36 28 20 13 6 -2 -10
-18
-25
-33
-41
-48
-56
Pre
ssur
e (m
b)
Latitude (º)
0.0E+0
5.0E+8
1.0E+9
1.5E+9
2.0E+9
2.5E+9
Top: SCIAMACHY NO2 number density,cm-3, on August 5, 2002;
Bottom: Canadian Middle AtmosphereModel NO2 [de Grandpre et al., 1997].
Sample orbit of NO2
Sample orbit of BrO- July 24th
1112131415161718192021222324252627
Latitude (°)
0
5
10
15
20
25
30
35
pptv
-Tropical upper tropospheric BrO at 4 ° S, associated with cirrus-Latitudinal distribution as expected[BrO] 18 pptv in the middle stratosphere
••
• SCIA • OS
•
Feb. 2003: Arctic
••
•••
••
Artic, Feb. 10th, 2003: DeNOxification extends from ~18-28 km
11131517192123252729313335373941
0.E+00 1.E+08 2.E+08 3.E+08 4.E+08 5.E+08 6.E+08 7.E+08 8.E+08 9.E+08 1.E+09
NO2 number density (molec/cm3)
Altit
ude
(km
)
75 N 72 N OS 72 N 68 N
1517192123252729313335373941
75 72 68 60Latitude (°)
0.0E+ 0
1.0E+ 8
2.0E+ 8
3.0E+ 8
4.0E+ 8
5.0E+ 8
6.0E+ 8
OSIRIS (17-37 km)
LT: just after sunrise(SZA 87.5°)
SCIAMACHY (15-41 km)
89.7 87 84 77 SZA (am)
1719
21
23
2527
2931
33
35
37
72 71 67 63 58Latitude (°)
0.0E+ 0
1.0E+ 8
2.0E+ 8
3.0E+ 8
4.0E+ 8
5.0E+ 8
6.0E+ 8
molec/cm3
Effect of differences in across-track and verticalresolution
VCDs from both instruments (Feb. 10th, 2003)
Latitude (°)
5658606264666870727476
NO
2 V
CD
(x 1
014 m
olec
/cm
2 )
2
4
6
8
10
12
OSIRIS (17-37 km)SCIAMACHY (15-41 km)
17
19
21
23
25
27
2931
33
35
37
72 71 67 63 58 53 48Latitude (°)
0.0E+ 0
1.0E+ 8
2.0E+ 8
3.0E+ 8
4.0E+ 8
5.0E+ 8
6.0E+ 8
7.0E+ 8
8.0E+ 8
Noxon cliff at 50° N
---------------------------------SCIA VCD=3.53e13
-------SCIA VCD= 1.02e13
13
15
17
19
21
23
25
27
0 5 10 15 20 25 30
Volume mixing ratio (ppt)
Alti
tude
(km
)
75 N, SZA=89.7° 71.5 N, SZA=86.6°
15
17
19
21
23
25
27
0.E+00 1.E+07 2.E+07 3.E+07 4.E+07 5.E+07 6.E+07 7.E+07 8.E+07
OClO number density (cm-3)
Alti
tude
(km
)
75 N72 N
ArcticOClO,Feb. 10th,2002
Northern hemisphere winter 02/03
OClO volume mixing ratio (pptv)
0 10 20 30 40 50 60
Alti
tude
(km
)
10
15
20
25
30
4225s2 (Dec. 21, 61° N, SZA=85.2), no PSC 4225s1 (Dec. 21, 64° N, SZA=88.6°), no PSC 4956s5 (Feb. 10, 75° N, SZA=86.6°), no PSC 4965s6 (Feb. 10, 72° N, SZA=89.7°) no PSC
15
17
19
21
23
25
27
29
0.E+00 1.E+07 2.E+07 3.E+07 4.E+07 5.E+07 6.E+07 7.E+07 8.E+07 9.E+07
BrO number density (molec/cm3)
Alti
tude
(km
)
68 N 72 N 75 N OS 72 N
Arctic BrO
15
17
19
21
23
25
27
29
0 5 10 15 20 25 30 35 40 45
BrO mixing ratio (pptv)
Alti
tude
(km
)
68 N72 N75 NOS 72 N
VCD (15-27 km, molec/cm2)
61º: 3.4e1368º: 2.3e1372º: 5.3e1375º: 5.7e13
OS VCD3.4e13
Limb radiance profiles at 2 NIR s
0
5
10
15
20
25
30
35
40
0.0E+00 2.0E+03 4.0E+03 6.0E+03 8.0E+03 1.0E+04 1.2E+04 1.4E+04
Radiance (arb. u.)
TH
(km
)
1301.241093.22
PSC observation, 65° S in early August (orbit 2293) Data from Antarctic winter
PSC at ~20-24 km, August 23rd, 61° S (orbit 2508)
0
5
10
15
20
25
30
1.3E+04 1.8E+04 2.3E+04 2.8E+04 3.3E+04 3.8E+04
Radiance at 1196 nm (arb.u.)
TH (
km)
••
•
Lat(°S) SCIA VCD
(11-41 km) 54 1.63e15 61 7.38e14 68 2.43e14
-DeNOxification extends from 1434 km at 68° S, 1730 km at 61° S-local sunrise, so NO2 is at daytime minimum (variation above is partly diurnal)-at 27 km, 68° S, [NO2] at sunrise is 2107 molec/cm3, [OClO] , [BrO]-hint of NOx descending from the mesosphere at 68° S
11131517192123252729313335373941
0.0E+00 2.0E+08 4.0E+08 6.0E+08 8.0E+08 1.0E+09 1.2E+09
NO2 number density (molec/cm3)
Altit
ude
(km
)
54 S, SZA=76 61 S, SZA=83 68 S, SZA=89.9
Southern hemisphere winter, 2002
OClO volume mixing ratio (pptv)
0 5 10 15 20 25 30 35
Alti
tude
(km
)
10
15
20
25
30
35
2794s6 (Sep. 12, 75° S, SZA=89.6°), no PSC 2293s3 (Aug. 8, 65° S, SZA=89.997°), PSC at 23 km 2297s9 (Aug. 8, 65° S, SZA=89.9°), no PSC2337s16 (Aug. 11, 65° S, SZA=89.9°), no PSC2307s3 (Aug. 11, 65° S, SZA=89.96°)2508s4 (Aug. 23, 68° S, SZA=89.77°), no PSC2508s3 (Aug. 23, 61° S, SZA=83.0°), PSC at 23 km2250bs2 (Aug. 5, 59.5° S, SZA=86°), no PSC 2579s5 (Aug. 28, 66° S, SZA=85.3°), no PSC
**
Lat SCIA (°S) VCD (14-28 km)61 7.6e1268 1.5e13
14
16
18
20
22
24
26
28
30
0 5 10 15 20 25 30 35
OClO volume mixing ratio (pptv)
Alti
tude
(km
)
14
16
18
20
22
24
26
28
30
0.0E+00 5.0E+06 1.0E+07 1.5E+07 2.0E+07 2.5E+07
OClO number density (cm-3)
Alti
tude
(km
)
68 S61 S
••
•Lat SCIA(S) VCD (11-30 km)54 5.48e13 61 5.83e1368 3.30e13
Evidence for high BrO mixing ratios in middle stratosphere, at highsouthern latitudes as well
11
13
15
17
19
21
23
25
27
29
0 5 10 15 20 25 30 35
BrO mixing ratio (pptv)
Alti
tude
(km
)
68 S, SZA=89.761 S, SZA=82.854 S, SZA=76
•Direct confirmation of our understanding of BrO photochemistryin the lower stratosphere at sunrise
•[BrO] sharply decreasing with height in the lowermost stratosphere•BrO spike at ~19 km “allowed” by low NO2 at 68° S
11
13
15
17
19
21
23
25
27
29
31
0.0E+00 1.0E+07 2.0E+07 3.0E+07 4.0E+07 5.0E+07 6.0E+07 7.0E+07
BrO number density (molec/cm3)
Alti
tude
(km
)
68 S, SZA=89.761 S, SZA=8361 S, SZA=89.7
ConclusionsConclusions
OClO layer peaks at higher altitude in Antarctic than Arctic
at the vortex edge, OClO shows a very limited vertical extent (sharp layer)
Denoxification is more severe and covers a greater altitude range in Antarctic than Artic
OClO exhibits correlation with BrO and clear anti-correlationwith NO2 ; BrO also anti-correlated with NO2
SCIAMACHY stratospheric BrO is in good agreement with GOME total columns outside of polar PBL enhancements
BrO mixing ratios of 26 pptv in the middle stratosphere!!!
AcknowledgmentsAcknowledgments
Florence Goutail and the SAOZ team, Ghassan Taha and the SAGE IIIteam, Michel van Roozendael (IASB), University of Bremen, and
Chris McLinden (Environment Canada)
Final RemarkFinal Remark
Limb scatter technique can measure scientifically useful profiles of minor trace gases such as BrO and OClO despite
their absorption signatures being at the 10-3 level