Introducing VESPA-22: a groundbased microwave spectrometer for measuring middle atmospheric water vapour at polar latitudes 27 April 2012 EGU General Assembly 2012 Pietro Paolo Bertagnolio, Giovanni Muscari, Irene Fiorucci and Massimo Mari Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy Department of Earth Sciences, University of Siena Distributed under Creative Commons Attribution 3.0 Our goal To observe changes in the water vapour concentration profile in the stratosphere and mesosphere in the polar regions Long-term (decadal trends) Short-term (diurnal cycle) With a new ground-based microwave spectrometer to measure the 22.235 GHz transition of water vapour as part of the NDACC network EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 1/14 Outline • Stratospheric H2O and its • • • • • impact on PSCs The observational challenges of the 22-GHz H2O line How does the technique work? Our instrumental setup First measured and calibrated spectra Conclusions and future work EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 2/14 Decadal change in stratospheric H2O as yet not well understood • Steady rise since 1980 • 10% decrease in 2000 • Influence on surface warming 30% of GHG from “Contributions of stratospheric water vapor to decadal changes in the rate of global warming.” S. Solomon et al. – Science - 2010 EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 3/14 Impact of H2O increase on Arctic PSC formation + 1 ppmv H2O from “Quantifying Denitrification and Its Effect on Ozone Recovery”, Tabazadeh at al. – Science - 2000 EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 4/14 The observational challenge thermo meso strato tropo EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 5/14 Balanced Beam-Switching Measurement Technique π»∗π π¨πΉ ππ‘πππ ππ‘πππ,π Stratosphere π»∗π π¨πΊ ππ‘πππ ππ‘πππ,π π»π ππ Receiver π»πππ Troposphere Compensating Sheet • ππ = ππ§∗ π΄π πΌπ‘πππ,π + ππ‘πππ ππ‘πππ,π + ππππ • ππ = ππ§∗ π΄π πΌπ‘πππ,π πΌπ + ππ‘πππ ππ‘πππ,π πΌπ + ππ ππ + ππππ • ππ − ππ = ππ§∗ π΄π πΌπ‘πππ,π − π΄π πΌπ‘πππ,π πΌπ EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 6/14 VESPA-22 (water Vapor Emission Spectrometer for Polar Atmospheres at 22 GHz) EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 7/14 Parabolic antenna Half-Power Beam Width (HPBW) = 3.5° Sidelobes < -40 dB below main lobe Cross-polarization < -24 dB below main polarization EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 8/14 Noise diode calibration ππ − ππ = πΊ ππ − ππ = πππ· π − ππ πππ·+π − ππ π Cold body (LN2) Hot body Calibration sources EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 9/14 Noise diode calibration 8 x 10 "Raw" Calibration Spectra Cold Target (77 K) Hot Target (295 K) Noise Diode 1 (84 K) Noise Diode 2 (131 K) FFT Counts 2 1.5 1 0.5 0 5000 10000 FFT Channels 15000 EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it Trec = 312 K 10/14 Brightness Temperature [mK] Calibrated Spectrum 18-04-2012 13:20-17:20 Effective Integration Time 80' 3000 2000 1000 0 -1000 -2000 22.15 22.2 22.25 Frequency [GHz] 22.3 EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 11/14 Water Vapour Emission Line @ 22.235 GHz 18-19/04/2012 Effective Integration Time 3h40' Brightness Temperature [mK] 300 200 100 0 -100 22.225 22.23 22.235 Frequency [GHz] 22.24 EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 22.245 12/14 Conclusions • Long-term monitoring of polar stratospheric water vapour • • is needed We designed and built a new 22-GHz spectrometer for polar observations We measured the first atmospheric spectra (“first light”) Future work (now the fun starts…) • Improve baseline flatness: – λ/4 wobbler instead of fixed shift – Delrin compensating sheet – Front-end optimization • Improve sensitivity and Trec – Test single-sideband mixer • Test with longer integration times from an high-altitude observatory (Gran Sasso) • Set up inversion algorithm EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 13/14 References • Bertagnolio, P. P., Muscari, G., & Baskaradas, J. (2012). Development of a 22 • • GHz ground-based spectrometer for middle atmospheric water vapour monitoring. European Journal of Remote Sensing, 51-61. doi:10.5721/EuJRS20124506 Solomon, S., Rosenlof, K. H., Portmann, R. W., Daniel, J. S., Davis, S. M., Sanford, T. J., & Plattner, G.-K. (2010). Contributions of stratospheric water vapor to decadal changes in the rate of global warming. Science (New York, N.Y.), 327(5970), 1219-23. doi:10.1126/science.1182488 Tabazadeh, A., Santee, M. L., Danilin, M. Y., Pumphrey, H. C., Newman, P. A., Hamill, P. J., & Mergenthaler, J. L. (2000). Quantifying Denitrification and Its Effect on Ozone Recovery. Science, 288(5470), 1407-1411. doi:10.1126/science.288.5470.1407 Thank you for your attention! EGU GENERAL ASSEMBLY 2012 – 27/04/2012 PIETRO PAOLO BERTAGNOLIO – pietropaolo.bertagnolio@ingv.it 14/14