The first operations at the new High-altitude Maïdo Observatory at La Réunion began in 2013. The Maïdo Lidar Calibration Campaign (MALICCA) was organized there in April 2013 and has focused on the validation of the thermodynamic parameters (temperature, water vapor, and wind) measured with many instruments including the new very large lidar for water vapor and temperature profiles. The aim of this publication consists of providing an overview of the different instruments deployed during this campaign and their status, some of the targeted scientific questions and associated instrumental issues. Some specific detailed studies for some individual techniques were addressed elsewhere. This study shows that temperature profiles were obtained from the ground to the mesopause (80 km) thanks to the lidar and regular meteorological balloon-borne sondes with an overlap range showing good agreement. Water vapor is also monitored from the ground to the mesopause by using the Raman lidar and microwave techniques. Both techniques need to be pushed to their limit to reduce the missing range in the lower stratosphere. Total columns obtained from global positioning system or spectrometers are valuable for checking the calibration and ensuring vertical continuity. The lidar can also provide the vertical cloud structure that is a valuable complementary piece of information when investigating the water vapor cycle. Finally, wind vertical profiles, which were obtained from sondes, are now also retrieved at Maïdo from the newly implemented microwave technique and the lidar. Stable calibrations as well as a small-scale dynamical structure are required to monitor the thermodynamic state of the middle atmosphere, ensure validation of satellite sensors, study the transport of water vapor in the vicinity of the tropical tropopause and study their link with cirrus clouds and cyclones and the impact of small-scale dynamics (gravity waves) and their link with the mean state of the mesosphere.
Water vapor is the strongest natural greenhouse gas in the atmosphere. It is most abundant in the troposphere at low
altitudes, due to evaporation at the ocean surface, with maximum values of around 6 g/kg. The amount of water vapor
reaches a minimum at tropopause level and increases again in the middle atmosphere through oxidation of methane and
vertical transport. Water vapor has both positive and negative effects on global warming, and we need to study how it
works on climate change by monitoring water vapor concentration in the middle atmosphere.
In this paper, we focus on the 22 GHz ground-based radiometer called SWARA (Seoul Water vapor Radiometer) which
has been operated at Sookmyung women's university in Seoul, Korea since Oct. 2006. It is a joint project of the
University of Bern, Switzerland, and the Sookmyung Women's University of Seoul, South Korea. The SWARA receives
22.235 GHz emitted from water vapor spontaneously and converts down to 1.5 GHz with +/- 0.5 GHz band width in 61
kHz resolution.
To represent 22.235 GHz water vapor spectrum precisely, we need some calibration methods because the signal shows
very weak intensity in ~0.1 K on the ground. For SWARA, we have used the balancing and the tipping curve methods
for a calibration. To retrieve the water vapor profile, we have applied ARTS and Qpack software. In this paper, we will
present the calibration methods and water vapor variation over Seoul for the last 4 years.
The Institute of Applied Physics of the University of Berne is active in the filed of remote sensing of middle atmospheric trace gases such as ozone and water vapor by microwave radiometry. From the measured pressure broadened spectral lines it is possible to retrieve the vertical distribution of the observed species. One of the radiometers is operating from an aircraft of the Swiss Air Force. For the spectral analysis it uses a broadband acousto-optical spectrometer with a total bandwidth of 1 GHz with 1725 channels, which allows retrievals of altitude profiles from about the flight height up to 60 km. Unfortunately acousto-optical spectrometers proved to be critical under conditions encountered in an aircraft. For this reason the novel approach of using digital Fast Fourier Transform (FFT) spectrometers with a total bandwidth of 25 MHz and with the option to select either 2048 or 4096 channels and another FFT spectrometer with 16384 channels on 1 GHz bandwidth was chosen. In this paper we present first measurements of atmospheric trace constituents using this novel approach with digital FFT spectrometers. We report on critical instrumental aspects such as system stability and linearity that are of fundamental importance for this application.
The Institute of Applied Physics has developed a new ground-based radiometer for measurements of water vapour profiles in the stratosphere and mesosphere. The uncooled instrument, called MIAWARA, has a very good sensitivity and is calibrated using a combination of tipping curve and balancing calibration. Using this combination the instrument can operate as a self calibrating system without the need for routine maintenance. We present a validation technique for the tipping curve calibration and a new approach for the reference absorber design used in the balancing calibration. The uncommon design of the reference absorbers decreases standing wave artifacts and thus enhances the sensitivity of the instrument, leading to a very good altitude coverage in the range of 20 - 80 kilometres.
The Institute of Applied Physics has developed a new model, called BEAM, for the simulation of microwave propagation in the atmosphere. The model is very flexible and can be used for simulations as well as operational retrievals. Microwave spectra are calculated using data from the JPL and HITRAN spectroscopic databases as well as the millimeter wave propagation model MPM-93. An new automatic frequency selection algorithm can increase the speed of the calculations by a factor of 10-100 under certain conditions.
Doris Maier, Niklaus Kaempfer, W. Amacher, M. Wuethrich, J. de la Noe, P. Ricaud, P. Baron, Gerard Beaudin, C. Viguerie, J.-R. Pardo, Juan Gallego-Puyol, Alberto Barcia, J. Cernicharo, Brian Ellison, Richard Siddans, David Matheson, Klaus Kuenzi, U. Klein, B. Franke, J. Louhi, J. Mallat, M. Gustafsson, A. Raeisaenen, Alexandre Karpov
The objective of the European project EMCOR was the development of a heterodyne receiver for the frequency range of 201 to 210 GHz for the measurement of the amounts of various minor constituents of the stratosphere involved in ozone chemistry. In order to be able to measure even very faint spectral lines a superconducting tunnel junction has been chosen as mixer element. Additionally, special care has been taken in developing the calibration unit of the system. Besides the classical hot-cold calibration three different balancing methods can be employed: a beam-switch technique with an atmospheric reference signal, a beam switch technique with a reference signal from a variable reference load or a frequency switch technique. The system has been integrated and is currently under testing. It will be installed at the International Scientific Station Jungfraujoch in he Swiss Alps and operated within the framework of the European Alpine stations of the Network for the Detection of Stratospheric Change.
The small amount of water vapor in the upper troposphere plays an important role in the Earth's climate system, e.g. by determining the occurrence and distribution of cirrus clouds. However, only little is known about the vertical distribution of upper tropospheric humidity (UTH). In this paper we propose a method for the retrieval of UTH from measurements taken by the Millimeter wave Atmospheric Sounder (MAS) onboard the space shuttle. MAS is a microwave limb sounder that was originally built to measure trace gases in the stratosphere and mesosphere. One of its channels around 204 Hz is sensitive to the amount of water vapor near the tangent point down to altitudes of about 7 km. Retrievals performed with simulated data have shown promising results. First comparisons with measured data show large discrepancies between actual measurements and the predictions of the widely used Liebe model. Preliminary results suggest that the Liebe model strongly underestimates the dry air continuum in this frequency range for the limb-sounding geometry.
Microwave radiometry is an extremely powerful tool for atmospheric research. It is specially suited for the investigation of the dynamical and chemical processes that are important in the depletion of the ozone layer and related phenomena of the middle atmosphere. The theoretical and technical concepts of microwave remote sensing of the atmosphere are briefly reviewed. A special weight is given to the approaches as used at the Institute of Applied Physics (lAP) of the University of Bern for ground-based instruments and sensors on aircraft and on the space shuttle. Examples of results from the different instruments in the frequency range of 20 to 200 GHz illustrate the huge potential of this technique for atmospheric research.
Measurements of the 142 GHz rotational line of O3 are performed with a cooled total power radiometer. The spectral data obtained with this instrument are inverted with the Chahine algorithm in order to obtain an altitude profile of O3 in the range of 20 km to 70 km. Such profiles are compared with ozone measurements from other techniques available in the alpine region, such as Umkehr and balloon sonde data. For the correction of tropospheric effects mainly originating from water vapor, data from a dual channel radiometer at 21 GHz/31 GHz are used.
Millimeter-wave radiometers are being used in remote sensing of stratospheric trace gases. For constituents with relatively strong spectral lines (several K), for example, ozone and water vapor, a total power radiometer with a simple load-switch calibration technique may be sufficient. If the spectral lines are weaker, and the signal to noise ratio is smaller than 10-4, a balanced calibration technique should be applied. Unfortunately, this can not easily be realized in the millimeter-wave region. Therefore, a quasi-balanced noise source in the atmosphere itself is planned.
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