Results for the stratosphere Bruno Carli Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 1
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
MIPAS objectives Studies Atmospheric chemistry Atmospheric dynamics Climatology Applications Climate change Ozone losses Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 3
Global picture of the atmospheric composition Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 4
Horizontal section of the 3D distribution Temperature Vertical section of the 3D distribution Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 5
H 2 O Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 6
O 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 7
HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 8
CH 4 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 9
N 2 O Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 10
NO 2 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 11
ClONO 2 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 12
N 2 O 5 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 13
F11 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 14
F12 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 15
25-27 september 2002 O 21 km altitude 3 HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 16
25-27 september 2003 21 km altitude O 3 HNO 3 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 17
2002 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 18
Example of results ANTARCTIC OZONE HOLE 2002 vs 2003: Temperature # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 19
Example of results ANTARCTIC OZONE HOLE 2002 vs 2003: O 3 # 8225 # 2994 26th September 2002 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 20
Example of results: ANTARCTIC OZONE HOLE 2002 vs 2003: HNO 3 # 8225 # 2994 26th September 2002 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 21
Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : CH 4 # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 22
Example of results: ANTARCTIC OZONE HOLE 2002 vs 2003: N 2 O # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 23
Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : ClONO 2 # 2994 26th September 2002 # 8225 26th September 2003 Non-target species Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 24
Example of results ANTARCTIC OZONE HOLE 2002 vs 2003 : N 2 O 5 # 2994 26th September 2002 # 8225 26th September 2003 Non-target species Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 25
Example of MIPAS products ANTARCTIC OZONE HOLE : CFC-12 (2002 vs 2003) # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 26
Example of MIPAS products ANTARCTIC OZONE HOLE : CFC-11 (2002 vs 2003) # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 27
Example of MIPAS products ANTARCTIC OZONE HOLE (2002 vs 2003) # 2994 26th September 2002 # 8225 26th September 2003 Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 28
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
NO 2, Antarctic 2003, 65S-90S, Ngt
NO 2, Arctic 2002/03, 65N-90N, Ngt
N 2 O and CH 4 CORRELATION Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 32
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: 18-35 km: H 7.1 ppmv, 35-50 km: H 7.9 ppmv. Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 33
Effect of PSC clouds Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 34
Day-night variation A region with emissions from: -CO 2 030-000 lines -O 3 101-000 lines - CO lines CO 2 030-000 lines. Larger in the nighttime (warmer temperatures) CO lines. Larger in the daytime (solar pumped) O 3 101-000 lines. Larger in the nighttime (warmer temperatures) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 35
Climatological studies water vapour Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 36
Climatological studies nitric acid Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 37
Climatological studies ozone Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 38
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
NOM. L= 510 km (72 profiles) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 40
S6. L= 125 km (244 profiles) Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 41
In the ASSET project data assimilation of non-standard MIPAS Level 2 products was performed for the test period 20 Sept. - 4 Oct. 2003. Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 42
CFC-11 12 km 18 km 24 km ppmv Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 43
CFC-12 12 km 21 km 30 km ppmv Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 44
ClONO 2 21 km 27 km 33 km ppmv Day Night Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 45
N 2 O 5 24 km 33 km 39 km ppmv Day Night Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 46
Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 47
MIPAS-Model Comparison Ozone distribution at 50 hpa 26.09.02 [top] / 13.10.02 [bottom] CLaMS KASIMA DLR-ROSE Day 6 Lecture 2 Results for the stratosphere - Bruno Carli 48
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