Program Overview and Sessions Timetable
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Program Overview and Sessions Timetable
A poster session will take place on Tuesday 28th at Leonardo Building.
Poster size and Layout: the available whiteboards size is 122 cm wide (48.03") x 125 cm high (49.2"). E.g. A0 format can fit perfectly vertical or landscape.
]]>As evidence of its splendor during the Roman era, Aquileia boasts a vast archaeological site, where it is possible to admire many artifacts, including the ruins of the forum, the burial ground, the river port and a few habitations.
Aquileia also played an important religious role at the beginning of the Christian era; it is thus possible to admire the remains of an early Christian Basilica, unique exemplar of religious architecture dating back to the 5th-6th Centuries. The beautiful mosaics that decorated the structure are now visible in the Early Christian Museum in Aquileia.
View of Archeological Area of Aquileia
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€350 per person
€150 Students/ Pensioners (*)
€100 Accompanying persons(**)
The conference registration fees include:
A limited number of grants are available to support the travel and living expenses of selected participants, with priority given to participants working in a developing country and who are at the early stages of their career. The payment of the registration fee for selected applicants from developing countries will be waived.
]]>Chairs: Keith Groves, Eurico de Paula
The occurrence of amplitude and phase scintillations on transionospheric radio wave signals due to scattering by ionospheric irregularities is an important aspect of space weather that affects space-based communications and navigation systems in different ways. Advances and research in irregularities and scintillation measurements and effects are discussed in this section. Relevant topics include the characterization of irregularities focused on their climatology and morphology, spatial and temporal correlations and occurrence patterns, and their associated scintillation effects on radio wave propagation including the relationship between different scintillation indexes, effects of amplitude and phase scintillation on new GPS signals (L2C and L5) and spatial/temporal/spectral characteristics and correlations. This section also targets the influence of irregularities and scintillation on GNSS positioning and the potential for threat reduction relative to GPS-only applications. Studies of irregularities effects on GNSS users are solicited, especially for space- and ground-based augmentation and aviation users, and discussion of important results, outstanding problems and challenges related to GNSS systems is welcome. New measurement techniques and comparisons of scintillation observations with other sensor data are of particular interest.
Chairs: Yannick Beniguel, Chuck Rino
Radio propagation disturbances regularly observed on low earth-orbiting and GNSS satellites are attributed to intermediate-scale structure (hundreds of kilometers to hundreds of meters). This scintillation phenomenon is of practical concern because it can degrade satellite communication, navigation, and surveillance operations. The global monitoring capability of the GNSS has stimulated significant advances in our understanding of large-scale ionospheric structure. However, commensurate progress in reconciling scintillation observations with hypothesized and/or measured power-law structure characteristics has been limited. This session seeks multi-frequency scintillation data analyses that attempt to reconcile observations with theoretical predictions based on definitive power-law structure and/or in-situ structure measurements.
Chairs: Bruno Nava, Matthew Angling
Many models have been developed to capture different aspects of the ionosphere: median empirical models capture the ionospheric climatology, whilst first principle models can represent many of the physical processes in the ionosphere. However, in order to represent ionospheric weather (i.e. processes and structures occurring over periods of hours and over medium spatial scales) it is necessary to move towards data assimilation (DA). DA can exploit diverse data types such as ground and space-based GNSS derived TEC, in situ electron density measurements, and ionosonde derived plasma frequency. Furthermore, a wide variety of DA methods have been applied to the ionosphere in recent years. These include Kalman Filters, 3 or 4-dimensional variational methods and tomographic techniques. Papers on the assimilation of ionospheric data into empirical or first-principle models are solicited for this session. Of particular interest are papers describing new assimilation methods, methods that exploit multi-sensor observations, and methods that exploit more than one model such as multi-model ensembles.
Chairs: Tim Fuller-Rowell, Dieter Bilitza
Advances in observations have revealed anomalies and structure in the ionosphere previously unmodeled. For instance, ground-based GNSS networks and radio occultation have revealed three or four peaks in the F-region plasma density latitude structure, rather than the typical two peaks associated with the traditional equatorial ionization anomalies (EIAs). In addition, during strong geomagnetic activity, storm-enhanced densities at mid-latitudes can dominate the global structure and create steep gradients in plasma density. Furthermore, new ionosonde and digisonde observations, as well as the GNSS observations, have enabled visualization of the complex high-resolution ionospheric wave structure seen as TIDs and MSTIDs, driven by waves from the lower atmosphere and from the auroral sources propagating through the thermosphere. This session targets new modeling capabilities, including thermosphere-ionosphere, whole atmosphere-ionosphere, and magnetosphere-ionosphere-thermosphere models, that are able to capture these anomalies, structure, and features. This session also targets the challenge of developing appropriate metrics to validate the existing and new modeling capabilities. Note that this session does not specifically target new data assimilation techniques, or ionospheric structure associated with equatorial irregularities, which are covered by other sessions.
Chairs: Sandro Radicella, Andrzej Krankowski, Babatunde Rabiu, Francisco Azpilicueta
Critical to ionospheric modeling efforts and data assimilative processes are ground and space based TEC measurements availability and quality. A number of recent initiatives have led to deployment of ground networks capable of measuring TEC in regions hitherto dearth of TEC data. The increasing amount of available GNSS constellations, ground networks of receiving stations and altimetry missions able to increase the number of accessible measurements is an important contribution to the data availability. Space based TEC data are being used more and more to characterize the ionosphere under different solar-geomagnetic conditions mainly through radio-occultation techniques. Differences in performance of different TEC calibration techniques remain a problem particularly when data are used for model validation or assimilation. The session conveners aim to get an updated vision of the availability of ground and space based high quality TEC data and their use to advanced characterization of ionospheric conditions. Authors are encouraged to present their results obtained using TEC ground and space measurements with special attention to multi-station or regional coverage and estimate of data retrieval accuracy.
Chairs: Endawoke Yizengaw, Jann-Yenq Liu, Angela Aragon-Angel
Since the mid-1960s, the GNSS based radio occultation technique has been used to study the structure and properties of the atmospheres of not only Earth but also other planets, such as Venus, Mars, some other outer planets, and many of their moons. By measuring the phase delay of radio waves from GNSS satellites as they are occulted by the Earth’s atmosphere, the vertical density profiles of the bending angles of radio wave trajectories can be estimated using measurements onboard LEO satellites. The success of the GPS/MET mission in 1995 inspired a number of follow‐on missions that include radio occultation experiment, including the CHAMP, GRACE, SAC-C, COSMIC, Metop-A/B, C/NOFS, and upcoming COSMIC-2 satellites. The combined profiles from these different LEO satellites provide excellent opportunities to explore the dynamics and structure of the ionosphere, especially in the regions that have been devoid of ground-based instruments, allowing for investigation of the longitudinal variability of the ionospheric density structure. This session seeks contributions that advance the application of RO technique for space weather studies. In addition, we welcome presentations exploring innovative methodologies that address the current problem on RO inversion technique at the equatorial region where ionospheric irregularity, such as sporadic E and spread F, present and degrade the linear combination technique that affect the quality of density profile extracted in the region.
Chairs: Cathryn Mitchell, Giorgiana De Franceschi
This session solicits contributions on GNSS-based research and applications at high latitudes. Studies dealing with ionospheric irregularities, scintillation and total electron content (TEC) gradients are of interest. Papers dealing with GNSS data collection, data sets, model and processing developments and infrastructure available to support investigations are also welcome, as are those where GNSS is one part of a multi-instrument approach in particular in conjunction with incoherent scatter radars. Finally, papers highlighting and contrasting the differences and similarities at high and low latitudes and bi-polar comparisons are of interest. Impacts of research results on different applications such as positioning, space weather, solid Earth, cryosphere research and remote sensing are also highly encouraged.
Chairs: Norbert Jakowski, Anthea Coster
"Space weather events become noticeable in the geospace system either by the direct action of solar flares onto the atmosphere or through the coupling of the solar wind into the magnetosphere and ionosphere via the geomagnetic field. The resulting effects can impact positioning, navigation, and communications. The best way to prepare for near- and long-term space-weather impacts on modern society is to improve our ability to understand and forecast these events and to fully realize what the impacts are on our technological infrastructure. The goal of this session is to provide a forum for discussing ionosphere-space weather relationships in the context of applications utilizing space based radio systems.
The following questions should be addressed:
How can ionospheric monitoring and modelling be utilized to further our understanding of space weather in its complexity?
How is ionospheric weather impacted by energy inputs, either directly from the sun or indirectly via coupling processes with other geospheres such as the thermosphere and magnetosphere?
How can ionospheric weather be described, benchmarked and forecasted effectively to correct and mitigate the ionospheric impact on applications utilizing trans-ionospheric radio signals?
How can this information be provided to customers in an appropriate form according to their needs, e.g. considering latency, temporal and spatial resolution, and reliability, taking into account international perspectives on observations, modeling and forecasting?
Patricia Doherty, Bertram Arbesser-Rastburg
This session will address ionospheric effects on Satellite Navigation Systems and their users including aviation, maritime and land users. These systems may include regional augmentation systems such as Satellite-Based Augmentation Systems (SBAS), Ground-Based Augmentation Systems (GBAS), and the Global satellite systems including GPS, Glonass, Galileo and Compass. The FAA’s WAAS system was the first SBAS system deemed operational in July 2003. Since that time, the greatest impacts to WAAS availability have been extreme solar storm events. Other systems like EGNOS, started operations during solar minimum and they have experienced impacts on performance from the ionosphere during the current Solar Cycle 24. Navigation users in the polar regions will be challenged by solar storms with degraded accuracy and availability. Augmentation and aircraft systems planned to operate in the low latitude regions will be seriously challenged by the extreme ionospheric dynamics of the equatorial ionosphere. There challenges have already been observed by air, land and maritime users in those areas. Solar Cycle 24 is now is its declining phase and it will go down in history as one of the lowest solar cycles in over 100 years. However, satellite navigation systems have continued to develop with new services, applications and new frequencies. This session invites abstracts related to system performance assessments due to ionospheric effects, mitigation techniques, effects on users and program status for all navigation systems.
Attila Komjathy, Sergey Pulinets
Natural hazards, including earthquakes, volcanic eruptions, and tsunamis have been significant threats to humans throughout recorded history. The Global Navigation Satellite System (GNSS) satellites including GPS, GLONASS, Galileo, BeiDou and others have become primary sensors to measure signatures associated with such natural hazards. These signatures typically include GNSS-derived seismic deformation measurements, co-seismic vertical displacements, and real-time GNSS-measured ocean buoy positioning estimates. Another way to use GNSS observables is to compute the ionospheric total electron content (TEC) monitor post-seismic and pre-seismic ionospheric disturbances caused by earthquakes, volcanic eruptions, and tsunamis. These measurements provide new scientific insight into the geophysical source phenomenology, wave propagation physics, and electromagnetic coupling processes. We solicit observational, theoretical and modeling contributions that specifically address the societal benefits that can be realized through the routine monitoring of atmospheric and ionospheric disturbances. Innovative concepts for the monitoring of seismic and tsunami hazards that make use of Earth to ionosphere coupling via acoustic gravity waves are particularly welcome. Precursory signals and perturbations consecutive to recent earthquakes are also pertinent. With improved knowledge of the various geophysical processes involved, these means have the potential to enhance natural hazards warning systems in order to save human life and mitigate economic damage.
Chairs: Katy Alazo-Cuartas, Gopi Seemala, Yenca Migoya-Orue
]]>Trieste, home to ICTP, is located in the northeast corner of Italy, close to the Slovenian border. It is easily reachable by plane, train and car. Arriving by plane, one can choose to land at Ronchi dei Legionari airport, Venice Marco Polo Airport, or Treviso Airport. Trains operated by Trenitalia travel frequently between Trieste and major Italian cities, and there is a train stop located conveniently close to ICTP. Buses are available for local and regional transport.
Rates: Single Room (from 90 EUR to 140 EUR); Double Room (from 110 EUR to 180 EUR)
A number of rooms (10) have been blocked for the Beacon Symposium participants. Reservations deadline: 30/05/2016.
Tel: +39 040 224551
Tel: +39 040 2247085
Grand Hotel Duchi D'AostaTel: +39 040 7600011
Hotel VictoriaTel: +39 040 362415
Urban Hotel DesignTel: +39 040 302065
Hotel ContinentaleTel: +39 040 631717
Rates: Single Room (from 55 EUR to 70 EUR); Double Room (from 74 EUR to 95 EUR)
Tel: +39 040 365208
Hotel James JoyceTel: +39 040 302065
Residence del MareTel: +39 040 307346
Residence le TerrazzeTel: +39 040 369822
]]>Sandro Radicella
Bruno Nava
Yenca Migoya Orue
Stanka Tanaskovic
Pandora Malchose
Patricia Doherty, Chair, Beacon Satellite Studies Group of URSI Commission
G, USA
Bruno Nava, Co-Chair, Beacon Satellite Studies Group, Italy
Andrzej Krankowski, Co-Chair, Beacon Satellite Studies Group, Poland
Sandro Radicella, Italy
Matthew Angling, United Kingdom
Francisco Azpilicueta, Argentina
Anthea Coster, USA
Giorgiana De Franceschi, Italy
Keith Groves, USA
Norbert Jakowski, Germany
Cathryn Mitchell, United Kingdom
Babatunde Rabiu, Nigeria
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