20th EVGA Meeting and 12th Analysis Workshop 2011

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    in Bonn, Germany, on invitation of the Max Planck Institute for Radio Astronomy

    Dates: March 29 - 31, EVGA Meeting
    March 31, Analysis Workshop

    LOC:  Walter Alef
    Axel Nothnagel
    Simone Bernhart
    Beate Naunheim
    Hermann Sturm

     

    Abstracts:

     

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    Oleg Titov (Geoscience Australia), Sebastien Lambert (Paris Observatory)

    Authors Title Abstract Talk/Poster
    Martin Ettl, Alexander Neidhardt, Matthias Mühlbauer, Christian Plötz, Hayo Hase, Sergio Sobarzo, Cristian Herrera, Eric Oñate, Pedro Zaror, Felipe Pedreros, Octavio Zapato Experiences with regular remote attendance towards new observation strategies Current VLBI observations are controlled and attended locally at the radio telescopes on the basis of pre-scheduled session files. Operations have to deal with system specific station commands and individual setup procedures. Either the scheduler nor the correlator or analyst get real-time feedback about system parameter during a session. Changes in schedules after the start of a session by remote are impossible or at least quite difficult. For future scientific approaches a more flexible mechanism would optimize the usage of resources at the sites. Therefore shared-observation control between world-wide telescopes, remote attendance/control as well as completely unattended-observations could be useful, besides the classic way to run VLBI observations. To reach these goals the Geodetic Observatory Wettzell in cooperation with the Max-Planck-Institute for Radio Astronomy (Bonn) develop a software extension to the existing NASA Field System for remote control. Meanwhile remote control possibilities are regularly used and established at Wettzell. Based on this technology the completely remote attended and controlled geodetic VLBI session between Wettzell, Germany and Concepción, Chile were successfully performed over 24 hours. Also the intensives on weekends are regularly operated by remote. These first tests are extraordinary valuable to gather information about the differences between VLBI systems and to measure the performance of internet connections and automatic connection re-establishments. In addition, future developments for an authentication and user role management will be realized within the upcoming NEXPRES project. P

    Martin Ettl, Alexander Neidhardt, Matthias Mühlbauer, Wlater Alef, Ed Himwich, Christopher Beaudoin, Christian Plötz, Arpad Szomoru

    Concepts for continuous quality monitoring and station remote control In the Work Package 5 of the third task in the newly funded “Novel EXploration Pushing Robust e-VLBI Services”–project (NEXPReS) the Technische Universitaet Muenchen realize concepts for continuous quality monitoring and station remote control in cooperation with the Max-Planck-Institute for Radioastronomy, Bonn. NEXPReS is a three-year project aimed at further developing e-VLBI services of the European VLBI Network (EVN), with the goal of incorporating e-VLBI into every astronomical observation conducted by the EVN. This project focus on developments of an operational e-control system with authentication and authorization. It includes an appropriate role management with different remote access states for future observation strategies. To allow a flexible control of different systems in parallel sophisticated graphical user interfaces are designed and realized. It requires also a session oriented data management. Because of the higher degree of automation additional system parameters and information is collected with a new system monitoring. The whole system for monitoring and control is fully compatible to the NASA field system as extension. The concept will be proofed with regular tests between Wettzell and Effelsberg. The project is scheduled for the coming three years.  T
    Alexander Neidhardt,
    Martin Ettl, Helge Rottmann, Christian Plötz, Matthias Mühlbauer, Hayo Hase, Walter Alef, Sergio Sobarzo, Cristian Herrera, Ed Himwich
    New observation strategies with e-control With new remote control technologies it is not necessary anymore that the operator is on location. He can control the system from remote (remote observation). This technology can also be used to control more than one telescope by one operator. The control can be shared between operators (shared observation). At Wettzell also completely unattended observations have been done especially for the weekend sessions  for over 2 years now. The goal is to simplify operational workflows in combination with general control structures. These new observation strategies are not only designed for VLBI. They also offer other space techniques new possibilities for technical realization of a Global Geodetic Observing System (GGOS). To realize continuous and reliable observations it is necessary to ease inconvenient night and weekend sifts. Remote and autonomous observations are necessary steps to reach this goal. Therefore the developed software for control and monitoring is offered to the community in releases for download. Several new and comfortable features are already implemented to support the daily work of an operator.  T
    G. Kronschnabl, Hayo Hase, T. Klügel, A. Neidhardt, K. Pausch, W. Göldi VLBI2010 – The TWIN radio telescope project at Wettzell, Germany The Twin Telescope Wettzell Project is funded to be executed during the period of 2008−2011. The design of the TTW was based on the VLBI2010 vision of the corresponding IVS Working Group. In the first two project years the design passed the simulations with respect to its specifications and was approved for production. At the Geodetic Observatory Wettzell a thorough soil analysis was made in order to define the sites for the towers of the new radio telescopes. Meanwhile the construction work has begun and acceptance tests of several telescope parts, e.g. azimuth bearings, took place. The new radio telescopes are almost completely assembled and the progress is quite on time. In parallel to the construction work at the Wettzell site, the design work and ordering of the different feed options are under progress. P
    Christopher Jacobs

    X/Ka Celestial Frame

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    Arthur Niell

    Observations with a VLBI2010 System

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    Alessandra Bertarini

    Polarization Leakage: Final Results

    The precision of geodetic and astrometric measurements is degraded by instrumental errors of which polarization leakage is one of the larger.Its effect can be corrected in the data provided one knows the leakage characteristics of the stations. I describe resulting polarization leakage measurements and the algorithm that was implemented to correct for their effect on the geodetic delay measurables. From the measured leakage terms, one would expect polarization leakage to affect the group delay measurements by 0.5~ps to 7~ps, depending on the stations involved in the baseline. This proved to be below the statistical noise in a single VLBI experiment and so the improvement from the correction could not be detected. Polarization leakage was found, unespectedly, not the dominant source of non-closing errors.

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    Walter Alef

    Bonn correlator status report

    We will present the status of the Bonn MPIfR/BKG VLBI correlator center including a field report on how the MK IV hardware correlator was replaced by the DiFX software correlator.

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    T. Hobiger(1), M. Sekido(1), T. Otsubo(2,1) , T. Gotoh(1), T. Kubooka(1), H. Takiguchi(1) and H. Takeuchi(3) (1) National Institute of Information and Communications Technology (NICT), Japan (2) Hitotsubashi University, Japan (3) Japan Aerospace Exploration Agency(JAXA), Japan

    VLBI analysis with c5++ - status quo and outlook

    Otsubo et al. (2002) have developed an analysis software package based on Java named CONCERTO4 which enabled the user to consistently process SLR, GPS and other satellite tracking data. Driven by the need to update the software and replace the existing Java code, VLBI was added as an additional module to this analysis package and renamed c5++. The software provides state-of-the-art modules for a variety of geodetic, mathematical and geophysical tasks that can be combined to a stand-alone VLBI application. Although many of these modules can be used for any of the space geodetic techniques, a couple of technique specific solutions (like relativity, antenna deformation, etc.) had to be coded exclusively for VLBI. We are going to discuss details of the software and its development and we are going to summarize how the automated analysis procedure of the real-time UT1 experiments has been realized with c5++. Other fields of applications for this software will be shown as well. We conclude our presentation with an outlook on future applications (including time and frequency transfer and space-craft navigation) as well as discuss the next steps towards a software package which allows combination of space geodetic techniques on the observation level.

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    Bill Petrachenko <style type="text/css"/>

    VLBI2010: Status and Prospects

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    The current status and future prospects of VLBI2010 will be discussed from a technique point of view.

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