institutet fÖr rymdfysik swedish institute of space physics u. raffalski, ndsc mw workshop, kos,...
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![Page 1: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/1.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
KIMRAKiruna Microwave Radiometer
U. Raffalski(1)
G. Hochschild and G. Kopp (2)
(1) Swedish Institute of Space Physics, Kiruna(2) Institute of Meteorology and Climate Research,
Forschungszentrum und Universität Karlsruhe, Germany
![Page 2: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/2.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
The KIMRA instrument at IRF Kiruna
• Location above polar circle (67.8 N, 21.4 E)– Cold and dry winter troposphere
transmissivity 0.53±0.18 (1σ) during period Nov - Apr 2003/04– Polar vortex – Vicinity to PSC
• Target species: O3, ClO, N2O, HNO3
• Continuous measurements since Jan 2002 (ozone)• Data retrieval by G. Kopp, IMK
![Page 3: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/3.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
The KIMRA instrument at IRF Kiruna
![Page 4: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/4.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
The KIMRA instrument at IRF Kiruna
Definition of edge region according to Equivalent Latitude Method
![Page 5: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/5.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
The KIMRA instrument at IRF KirunaGrid symbols
+45°
0° (vertical)
90° (horizontal)
Rotatable
A O S
Single sideband filterrotatingmirror I
rotatingmirror II
sidebandtermination
coldcalibration
load
Adjustablereferenceload
schottkymixer
293 K
120 K
Cryostat30 K
horn-antenna
1.6-2.6 GHz
Path length modulator
PLL
f
2f
Diplexer
Localoscillator
212 GHz
Acousto-Optical Spectrometer (AOS)
Data acquisition
crosspolarisationfilter
Periscope
Atmosphere
azimuthmirror
elevationmirror
Polarizer
warmcalibrationload
lownoiseamplifier
gunn106
GHzA O S
Single sideband filterrotatingmirror I
rotatingmirror II
sidebandtermination
coldcalibration
load
Adjustablereferenceload
schottkymixer
293 K
120 K
Cryostat30 K
horn-antenna
1.6-2.6 GHz
Path length modulator
PLL
f
2f
Diplexer
Localoscillator
212 GHz
Acousto-Optical Spectrometer (AOS)
Data acquisition
crosspolarisationfilter
Periscope
Atmosphere
azimuthmirror
elevationmirror
Polarizer
warmcalibrationload
lownoiseamplifier
gunn106
GHzA O S
Single sideband filterrotatingmirror I
rotatingmirror II
sidebandtermination
coldcalibration
load
Adjustablereferenceload
schottkymixer
293 K
120 K
Cryostat30 K
horn-antenna
1.6-2.6 GHz
Path length modulator
PLL
f
2f
Diplexer
Localoscillator
212 GHz
Acousto-Optical Spectrometer (AOS)
Data acquisition
crosspolarisationfilter
Periscope
Atmosphere
azimuthmirror
elevationmirror
Polarizer
warmcalibrationload
lownoiseamplifier
gunn106
GHzA O S
Single sideband filterrotatingmirror I
rotatingmirror II
sidebandtermination
coldcalibration
load
Adjustablereferenceload
schottkymixer
293 K
120 K
Cryostat30 K
horn-antenna
1.6-2.6 GHz
Path length modulator
PLL
f
2f
Diplexer
Localoscillator
212 GHz
Acousto-Optical Spectrometer (AOS)
Data acquisition
crosspolarisationfilter
Periscope
Atmosphere
azimuthmirror
elevationmirror
Polarizer
warmcalibrationload
lownoiseamplifier
gunn106
GHz
![Page 6: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/6.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
The KIMRA instrument at IRF Kiruna
![Page 7: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/7.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Vertical resolution and sensitivity of KIMRA
![Page 8: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/8.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Comparison radiometer/FTIR/sonde
• Data from 030205 - 030321• 14 Ozone sondes from Sodankylä• 16 FTIR ozone profiles• 28 millimetre wave ozone profiles
![Page 9: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/9.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Comparison KIMRA/FTIR/sonde
![Page 10: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/10.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Comparison KIMRA/FTIR
![Page 11: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/11.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Summary
• A new mm-wave radiometer is operated at IRF
• Target species O3, ClO, N2O, HNO3
• Frequency range 192 – 225 GHz• Cryogenically cooled Schottky-mixer (25 K)• Continuous ozone observations since Jan 2002
![Page 12: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/12.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Problems
• Strong baseline of the order of 2-3 K …– quite stable– most likely between LO and mixer
– impairs measurements of ClO, N2O, HNO3
• Cold calibration load temperature (value, drift)• …
![Page 13: INSTITUTET FÖR RYMDFYSIK Swedish Institute of Space Physics U. Raffalski, NDSC MW workshop, KOS, 2004-05-31 KIMRA Kiruna Microwave Radiometer U. Raffalski](https://reader036.vdocuments.mx/reader036/viewer/2022062421/56649d5d5503460f94a3c0c1/html5/thumbnails/13.jpg)
U. Raffalski, NDSC MW workshop, KOS, 2004-05-31
INSTITUTET FÖR RYMDFYSIKSwedish Institute of Space Physics
Further work
• Baseline effects have to be reduced– measurements of ClO, N2O, and HNO3
• Upgrade to higher resolution in the line center– ozone at high altitudes
– time sharing with a future (?) H2O radiometer