Results for the stratosphere
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1 Results for the stratosphere Bruno Carli Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 1
2 Table of Contents MIPAS objectives Multidimensional coverage of MIPAS measurements New observations of processes and budgets PSC and non-lte observations Climatology Improved horizontal resolution Data assimilation Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 2
3 MIPAS objectives Studies Atmospheric chemistry Atmospheric dynamics Climatology Applications Climate change Ozone losses Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 3
4 Global picture of the atmospheric composition Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 4
5 Horizontal section of the 3D distribution Temperature Vertical section of the 3D distribution Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 5
6 H 2 O Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 6
7 O 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 7
8 HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 8
9 CH 4 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 9
10 N 2 O Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 10
11 NO 2 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 11
12 ClONO 2 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 12
13 N 2 O 5 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 13
14 F11 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 14
15 F12 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 15
16 25-27 september 2002 O 21 km altitude 3 HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 16
17 25-27 september km altitude O 3 HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 17
18 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 18
19 Example of results ANTARCTIC OZONE HOLE 2002 vs 2003: Temperature # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 19
20 Example of results ANTARCTIC OZONE HOLE 2002 vs 2003: O 3 # 8225 # th September th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 20
21 Example of results: ANTARCTIC OZONE HOLE 2002 vs 2003: HNO 3 # 8225 # th September th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 21
22 Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : CH 4 # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 22
23 Example of results: ANTARCTIC OZONE HOLE 2002 vs 2003: N 2 O # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 23
24 Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : ClONO 2 # th September 2002 # th September 2003 Non-target species Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 24
25 Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : N 2 O 5 # th September 2002 # th September 2003 Non-target species Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 25
26 Example of MIPAS products ANTARCTIC OZONE HOLE : CFC-12 (2002 vs 2003) # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 26
27 Example of MIPAS products ANTARCTIC OZONE HOLE : CFC-11 (2002 vs 2003) # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 27
28 Example of MIPAS products ANTARCTIC OZONE HOLE (2002 vs 2003) # th September 2002 # th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 28
29 27/09/2002 No y chemistry DRAGON ADVANCED TRAINING COURSE IN ATMOSPHERE REMOTE SENSING N 2 O NO 2 NO 2 HNO 3 NO NO ClONO 2 N 2 O 5 ClONO 2 N 2 O 5 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 29
30 NO 2, Antarctic 2003, 65S-90S, Ngt
31 NO 2, Arctic 2002/03, 65N-90N, Ngt
32 N 2 O and CH 4 CORRELATION Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 32
33 Conservation of hydrogen budget Maps of the quantity H=H 2 O+2*CH 4 for 6 latitude bands, for the time period starting July 2002 and ending March 2004, obtained with MIPAS monthly mean VMR profile There is a significant seasonal variability, but two nearly constant horizontal bands are visible in all maps: km: H 7.1 ppmv, km: H 7.9 ppmv. Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 33
34 Effect of PSC clouds Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 34
35 Day-night variation A region with emissions from: -CO lines -O lines - CO lines CO lines. Larger in the nighttime (warmer temperatures) CO lines. Larger in the daytime (solar pumped) O lines. Larger in the nighttime (warmer temperatures) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 35
36 Climatological studies water vapour Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 36
37 Climatological studies nitric acid Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 37
38 Climatological studies ozone Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 38
39 Analysis of S6 observation mode In MIPAS S6 observation mode the along track sampling is 125 km. The analysis was performed with a 2D retrieval set at an horizontal resolution of either 510 km (equal to nominal mode along track sampling) or 125 km. Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 39
40 NOM. L= 510 km (72 profiles) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 40
41 S6. L= 125 km (244 profiles) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 41
42 In the ASSET project data assimilation of non-standard MIPAS Level 2 products was performed for the test period 20 Sept. - 4 Oct Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 42
43 CFC km 18 km 24 km ppmv Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 43
44 CFC km 21 km 30 km ppmv Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 44
45 ClONO 2 21 km 27 km 33 km ppmv Day Night Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 45
46 N 2 O 5 24 km 33 km 39 km ppmv Day Night Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 46
47 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 47
![MIPAS-Model Comparison Ozone distribution at 50 hpa 26.09.02 [top] / 13.10.](/docs-images/91/105701800/images/48-0.jpg "02 [bottom] CLaMS KASIMA DLR-ROSE Day 6 Lecture 2 Results for the stratosphere -")
48 MIPAS-Model Comparison Ozone distribution at 50 hpa [top] / [bottom] CLaMS KASIMA DLR-ROSE Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 48
49 Conclusions MIPAS is providing multidimensional information of atmospheric composition. MIPAS data can be used to study climatology, chemical and dynamical processes, PSC and non-lte conditions. With MIPAS it is possible to identify sources and sinks of the molecules in the stratosphere. MIPAS data have been successfully assimilated in weather prediction (NWP) models and chemical and transport models (CTM). Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 49
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