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                      |  |   | BROADBAND_CLOUDS: 
                          A TOOL FOR 2D REPRESENTATION OF CLOUDS IN MIPAS/ENVISAT 
                          SCENARIO, DESCRIPTION AND APPLICATIONS. (ASSFTS '09)
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                          The Michelson Interferometer for Passive Atmospheric 
                            Sounding (MIPAS), operating on-board ENVISAT, is a 
                            limb sounding Fourier Transform spectrometer for the 
                            measurement of high resolution gaseous emission spectra. 
                            Studies on MIPAS data have demonstrated its sensitivity 
                            to the radiation emitted from the clouds.The GMTR forward model has been used to create a self-standing 
                            Broad Band (BB) forward model (capable to simulate 
                            extended spectral regions). We have introduced into 
                            the BB forward model the capability to model the effects 
                            of cloud contamination into MIPAS spectra (BB_Clouds). 
                            Exploiting the 2D approach, the cloud is no longer 
                            represented as an infinite cloudy shell, but it is 
                            characterized by both a vertical and a horizontal 
                            extension. BB_Clouds has been used to assess the possibility 
                            to retrieve cloud extension and other parameters from 
                            MIPAS spectra. The developed algorithm and the results 
                            of the tests performed are presented and discussed.
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                      |  |   | RETRIEVAL 
                          OF H15NO3/H14NO3 VERTICAL ATMOSPHERIC DISTRIBUTION FROM 
                          MIPAS/ENVISAT LIMB EMISSION MEASUREMENTS('08)
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                          Atmospheric infrared remote-sensing has the potential 
                            to provide accurate information on the isotopic composition 
                            of several molecular constituents. Since new precise 
                            spectroscopic pa rameters of isotopically substituted 
                            molecules are becoming available, further advances 
                            in the understanding of the mechanisms leading to 
                            atmospheric isotope fractionation are possible. MIPAS 
                            (Michelson Interferometer for Passive Atmospheric 
                            Sounding), on-board the European satellite ENVISAT, 
                            is a mid-infrared emission FT interferometer probing 
                            the Earth's atmosphere with limb- scanning observations. 
                            The detected spectral radiances are routinely inverted 
                            to vertical distributions of pressure, temperature, 
                            and Volume Mixing Ratio (VMR) of H2O, O3, CH4, N2O, 
                            HNO3, and NO2. Non-operational scientific codes have 
                            proven that MIPAS spectra can also provide information 
                            on minor atmospheric trace constituents as well as 
                            on the distribution of the main isotopes in these 
                            gases. The inclusion of H15NO3 spectral line parameters 
                            (relative to the fundamental v5 band) into MIPAS-dedicated 
                            spectro scopic database provided the possibility to 
                            identify, for the first time, H15NO3 in the atmosphere 
                            (near 871 cm-1), and to investigate the behaviour 
                            of 15N in atmospheric nitric acid. Never before has 
                            the heavy-to-light nitrogen isotopic ratio profile 
                            been retrieved from HNO3 spectral signatures.
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                      |  |   | Distribuzioni 
                          verticali di Temperatura, acqua, ozono e acido nitrico 
                          dalle misure di MARSCHALS durante la campagna SCOUT-O3 
                          in Darwin (Nov. - Dic. 2005) 
                          (Ischia '07)
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                          MARSCHALS e' uno spettrometro eterodina che misura 
                            l'emissione termica atmosferica nel lontano infrarosso 
                            (FIR) con la tecnica del sondaggio a lembo. Lo strumento 
                            opera a bordo dell'aereo stratosferico M55 Geophysica.MARC e' il codice di analisi disegnato appositamente 
                            per l'analisi delle misure di MARSCHALS. Fra le sue 
                            caratteristiche ci sono la possibilità di eseguire 
                            l'analisi con la tecnica Multi-Target Retrieval (MTR) 
                            usando tutta la banda misurata e includendo la matrice 
                            degli errori sistematici durante la procedura di analisi.
 Il codice MARC e lo strumento MARSCHALS sono stati 
                            sviluppati durante uno studio ESA il cui obiettivo 
                            era testare la possibilità di usare la tecnica 
                            al lembo nel FIR per misurare la regione dell'alta 
                            troposfera e bassa stratosfera (UTLS).
 I risultati ottenuti analizzando le misure di MARSCHALS 
                            fatte durante la campagna SCOUT-O3 in Darwin, Australia 
                            (Nov. – Dic. 2005) verranno presentati. Sono 
                            state ottenute le distribuzioni verticali di Temperatura, 
                            acqua, ozono e acido nitrico nella regione UTLS lungo 
                            la rotta di volo di Geophysica. I risultati sono stati 
                            validati con le misure di altri strumenti a bordo 
                            dello stesso aereo e con dati ottenuti con un modello 
                            di chimica atmosferica.
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              |  |   | SOLAR INDUCED 
                PERTURBATIONS IN THE MIDDLE ATMOSPHERE: IS IT JUST A MATTER OF 
                MAGNITUDE? (EGU - April '05) 
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              | As a first order approximation, the response 
                  of the middle atmosphere to perturbations that are likely to 
                  occur, is characterized by changes in the O3 distribution. In 
                  fact, because of the peak in the O3 heating profile at about 
                  50 Km, strong variations in the O3 concentration cause a corresponding 
                  change in the heating of the atmosphere. As a consequence, temperature 
                  and wind fields are changed. But what does "strong" 
                  mean? A large drop of ozone concentration in a very stable atmospheric 
                  region can have a weaker response than one in an unstable region. 
                  Thus, "strong" should be considered not on the base 
                  of the perturbation itself, but on the base of the response 
                  to that perturbation. This study attempts to investigate the 
                  characteristics of perturbations that may affect the atmosphere, 
                  showing preliminary results of analyses of the response of a 
                  middle atmospheric model. In this poster, rather than constructing 
                  a complete set of test perturbations, we focus on a few case 
                  studies and will later test our hypothesis on more complete 
                  models (such as the ARPEGE - see DMI Peter Berg, poster X441 
                  this session). Even though not directly involving solar variability, 
                  the different scales we study may as well be considered different 
                  scales of (indirect) solar induced perturbations. 
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                      |  |   | MIPAS-ENVISAT 
                        Validation Measurements with the High Resolution FT-FIR 
                        Spectrometer SAFIRE-A aboard the Stratospheric Aircraft 
                        M-55 Geophysica (QOS - June '04) 
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                      | The SAFIRE-A Fourier transform 
                          Far-infrared spectrometer has been involved in field 
                          campaigns carried out with the M-55 Geophysica stratospheric 
                          aircraft in 2002-2003, aimed at validating the level-2 
                          products of the ENVISAT chemistry instruments. The limb 
                          sounding observations of volume mixing ratio vertical 
                          profiles of Ozone and Nitric Acid were especially focused 
                          on the validation of MIPAS products in the altitude 
                          range 10-20 km. Three campaigns have been conducted with the Geophysica 
                          platform from Forlì, Italy (Lat. 44°N, Lon. 
                          12°E) in July and October 2002 and from Kiruna, 
                          Sweden (Lat. 68°N, Lon. 20°E) in February-March 
                          2003, as part of the ESABC (ENVISAT Stratospheric Aircraft 
                          and Balloon Campaigns) activities. Here, we report the 
                          results of measurements of O3, HNO3 acquired by SAFIRE-A 
                          during the mid-latitude flight on the 24th of October 
                          2002.
 .An attempt to further exploit SAFIRE-A mid-latitude 
                          observations, in order to enlarge the dataset useful 
                          for MIPAS validation has been made with the support 
                          of modelling tools specifically developed by University 
                          of L’Aquila. First results from intercomparison 
                          based on trajectory calculations are presented, showing 
                          the effectiveness of the adopted approach.
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              |  |   | Limb Sounding Emission 
                Measurements of Lower Stratospheric Constituents From High Altitude Aircraft: an Overview of SAFIRE-A Campaigns
 at Mid-latitude and in the Polar Regions
 (QOS - June '04)
 
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              | The SAFIRE-A instrument has been deployed 
                  on the M-55 Geophysica high altitude aircraft in several scientific 
                  campaigns carried out, between the end of 1999 and the beginning 
                  of 2003, at mid-latitudes as well as in the Polar regions (both 
                  Arctic and Antarctica). The measurement capabilities of the 
                  spectrometer allowed the observation of the vertical distribution 
                  of several minor atmospheric constituents between the tropopause 
                  and the flight altitude (approx. 20 km) along the flight route. 
                  Recently, an optimised retrieval code, specifically developed 
                  for the analysis of the airborne instrument data, has been applied 
                  for the re-processing of the data measured during the APE-GAIA 
                  campaign (Ushuaia, Argentina, September-October 1999) and during 
                  ENVISAT validation flights at mid-latitude (Forlì, Italy, 
                  October 2002) and high-latitude flights (Kiruna, Sweden, March 
                  2003). An overview of the main results is presented, highlighting 
                  the instrument capability to simultaneously measure Volume Mixing 
                  Ratio (VMR) vertical profiles of different species such as Ozone, 
                  HNO3, N2O, ClO, HCl, H2O, that play a critical role in lower 
                  stratospheric chemistry and transport. |   
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              |  |   | SF6 Multi-Target Retrieval 
                (ASSFTS - October '03) 
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              | A retrieval approach for the simultaneous 
                  determination of the altitude distributions of pressure (p), 
                  temperature (T) and Volume Mixing Ratio (VMR) of atmospheric 
                  constituents from limb scanning measurements of the atmosphere 
                  has been developed and implemented in a computer code for the 
                  analysis of MIPAS- ENVISAT observations [B.M.Dinelli, D.Alpaslan, 
                  M.Carlotti, .Magnani, M.Ridolfi, 'Multi-target retrieval (MTR): 
                  the simultaneous retrieval of pressure, temperature and volume 
                  mixing ratio profiles from limb-scanning atmospheric measurements', 
                  Journal of Quantum Spectroscopy and Radiative Transfer, in press, 
                  (2003)]. This analysis method, named Multi-Target Retrieval 
                  (MTR), has been used to retrieve the altitude distribution of 
                  the SF6 VMR in the troposphere, from selected MIPAS orbits. 
                  The SF6 profile was retrieved simultaneously with the p, T, 
                  water and ozone profiles analysing selected spectral features 
                  of SF6 jointly with the spectral intervals used by the ESA Level 
                  2 processor for the sequential analysis of the MIPAS key species. |   
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              |  |   | Multi Target 
                Retrieval (EGS - April '03) 
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              | The processes of discretization, interpolation, 
                  and resampling are frequently used in data analysis. Here the 
                  formalism of functional spaces is used as a framework for the 
                  description and characterization of both the measurement operation 
                  and these subsequent processes. The tools provided by this formalism 
                  are applied to the problem of resampling of atmospheric volume 
                  mixing ratio vertical profiles obtained with limb-sounding measurements. 
                  In particular, a resampling method that uses the conservation 
                  of the vertical column as a constraint is presented and compared 
                  with other methods. The effects of the resampling process in 
                  terms of error propagation and loss of vertical resolution are 
                  also evaluated.  |   
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     | ISAC - CNR Gruppo: Remote Sensing of the Stratosphere
 Via P. Gobetti, 101
 40129 Bologna
 ITALY
 Tel.+39 051 6398002
 
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