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    In the MAss LOst in wind fluX (MALOX) project the automatic weather station AWS Virginia purpose is to contribute to the monitoring of global climate change monitoring standard meteorological parameters. The AWS is located at Inexpressible Island (74°56’S 163°41’E) at --- m a.s.l., and has been installed on the ---. It acquired, every minute, all year round, the meteorological vaiables of wind velocity, wind direction, temperature, pressure and relative humidity.

  • The datataset includes sound pressure levels acquired in the Ross Sea during project AMORS

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    The project is focused on the acquisition of data using interference filter radiometer DC_FRAD2011-04. Radiometer has been located in February 2012 at Concordia station, on the physics shelter in Dome C (75°06.1620' S, 123°19.1342' E). Is active all year round and measures the global solar irradiance (watt/m2nm) at the values ​​of 13 different wavelengths (about one spectrum per minute), where the filters are centered, and from these it can obtain the spectral irradiance with a resolution of 0.5 nm. The data is transferred to Italy on a daily basis via an Ethernet link. Data are acquired from January 2012 to May 2013.

  • TNB1 and TNB2 continuous GNSS stations There are currently two continuous GNSS stations, TNB1 and TNB2, nearby the Italian base MZS (Mario Zucchelli Station). Collected data, in RINEX format, are sent daily in Italy and are available for download at the Database page of this website. TNB1 continuous GPS station was monumented during the 1997-1998 campaign on a granite outcrop. It was originally equipped with an Ashtech Z-12 GPS receiver and an Ashtech 700936D Dorne Margolin antenna with chokering. Installed on a concrete pillar, TNB1 continuously collected data of the GPS constellation for about 17 years. In November 2015, the instrumentation was completely renewed. Currently, the station is equipped with a Leica GS25 GNSS receiver and a Leica AT504 Dorne Margolin antenna with chokering. TNB1 collect data of GPS and GLONASS constellations.

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    Installation of two radiometers with interference filters (F_RAD) operating in the spectral region from 296 nm to 400 nm. The purpose is to measure the global solar irradiance at the values ​​of the wavelengths where the filters are centered and from these derive the spectral irradiance with a resolution of 0.5 nm. The radiometers are currently positioned in the Antarctic stations of Mario Zucchelli and DomeC Concordia and operate permanently throughout the year. Measurements of absorbance of polysulphone dosimeters before and after exposure to UV solar radiation by laboratory spectrophotometer, data analysis, determination of the UV dose response curve vs absorbance variation and comparison of the results detected in the two sites. It can be used for the measurement of solar UV irradiance for research on the climate and the physics of the atmosphere.

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    The aim of the MAss LOst in wind fluX (MALOX) project is to better understand the phenomenon of snow transport over a coastal area characterized by strong winds. The automatic weather station AWS Lucia purpose is to contribute to the monitoring of global climate change monitoring standard meteorological parameters. The AWS is located at Larsen Glacier, (74° 57′ 2″ S - 161° 46′ 19″ E) at 1350 m a.s.l., and has been installed the 25 january 2007. It acquires, every minute, all year round, the meteorological variables by two sensors for wind velocity and wind direction, two sensors for temperature (at 1 and 3 meters) and for relative humidity, and finally one for atmospheric pressure. Moreover, the AWS acquires further data using radiation sensor (longwave and shortwave), driftometer for the snow transport and height snow sensor.

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    An automatic geomagnetic station for monitoring the Earth’s magnetic field variations has been installed in December 2020 at Talos Dome, a remote site on the Antarctic Plateau, about 300 km away from the permanent geomagnetic observatory at Mario Zucchelli Station (MZS). Designed and assembled at the laboratory of electronics of the Istituto Nazionale di Geofisica e Vulcanologia (INGV) in Rome, this autonomous station is formed by a vector magnetometer specifically manufactured by Lviv Institute (Ukraine) for very low temperatures and a low-power system supplied by batteries charged by wind generator and solar panel. Data, sampled at 1 Hz, are locally stored and can be downloaded once a year during the Antarctic summer expeditions. The goal was to integrate observatory data for better monitoring the geomagnetic field from an uncovered Antarctic area. In fact, it is well known that the distribution of geomagnetic observatories strongly favors the northern hemisphere and each new instrumental installation in Antarctica should be considered as a useful attempt to balance the geomagnetic monitoring in the two hemispheres. The achieved goal was to obtain a long data series, keeping the station working even during the austral winter when the temperature can reach −60°C; we recorded 4 years of data.

  • ISMAR_AN95 (?) ORA di BAIA TERRA NOVA ctd dicembre 1994 - CTD casts in the Ross Sea Station AN94043 - AN94045 - AN94046 - AN94047 - AN94048 - AN94049 - AN94050 - AN94051 - AN94052 - AN94053 - AN94054 - AN94055 - AN94056 - AN94057 - AN94058 - AN94059 - AN94060 - AN94061 - AN94062 - AN94063 - AN94064 - AN94065 - AN94066 - AN94067 - AN94068 - AN94069 - AN94070 - AN94071 - AN94072 - AN94073 - AN94074 - AN94075 - AN94076

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    The project is focused on the acquisition of data using the MZS_FRAD2008-02 interference filter radiometer, installed in November 2009 at Mario Zucchelli station, on the roof of the building OASI (74°41.6059' S 164°05.9423' E). The radiometer is active all year round and measures the global solar irradiance (watt / m2nm) at the values ​​of 9 different wavelengths (about one spectrum per minute), where the filters are centered, and obtained from these the measure of the spectral irradiance with a resolution of 0.5 nm. The data is transferred to Italy on a daily basis via an Ethernet link. Data are acquired in the summer station of MZS from November 2009 to May 2013.

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    Objective of the project is to develop and test acoustic methodologies for the long-term monitoring of environmental variability in the Antarctic regions, through underwater acoustic oceanography experiments. Using passive and active acoustic systems is possible obtain the remote observation of air-sea-ice interaction processes in polynya areas in the Terra Nova Bay (74 ° 40′59.99 "S 164 ° 04′00.01" E). Acoustic measurements are carryed out by launching an oceanographic mooring supporting a 300 kHz broadband ADCP and CTD probes (temperature, conductivity and pressure sensors), left in the area until the following year's campaign.