Meetings
Sixth IVS General Meeting
February 7-13, 2010
Hobart, TAS, Australia
Overview
Poster
Location
Schedule
mini-TOW
Related Meeting
Accommodation
Registration
Program
Submit an Abstract
Travel Information
Invitations
Program Committee
Local Committee
The IVS holds a technical meeting, called the General Meeting, every two years.
The purpose of the meeting is to assemble representatives from all IVS components
to share information, hear reports, and plan future activities. The meeting also
provides a forum for interaction with other members of the VLBI and Earth science
communities.
The keynote of the sixth GM is the new perspectives of the next generation
VLBI system under the theme "VLBI2010: From Vision to Reality". The vision
of the VLBI2010 system is gradually being realized. The unprecedented new
capabilities of 1-mm positional accuracy and station velocities of 0.1 mm/yr,
continuous observational time series for station positions and Earth
orientation parameters, and fast turnaround time from observation to geodetic
and astrometric result will foster new science and applications.
The content of the meeting will be of interest to the broad spectrum of IVS members
as well as to the wider VLBI and Earth science community. All IVS Associate Members
and individuals who have interests in the various applications and research fields of
VLBI such as geodesy, astrometry, Earth sciences, and related fields are encouraged
to attend the meeting and to make an oral or poster presentation. Non-IVS members are
cordially invited to attend the meeting and to make a presentation.
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The official poster of the General Meeting is available in various
resolutions:
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The meeting will be held in Hobart, Tasmania, Australia and will be hosted by the
University of Tasmania, School of Mathematics and Physics. The venue will be the
Physics Building (No. 13) of the Sandy
Bay Campus. The student accommodation is building no. 47. A
map of Sandy Bay is, for instance, available through Google maps
or Google earth by searching for "Sandy Bay, Tasmania, Australia". An icebreaker
reception (Sunday, 16:00-18:00) is planned as a cocktail party at Zero Penthouse of
Zero
Davey. Zero Davey is located in
Sullivans Cove on Hobart's waterfront.
The overall schedule of the week includes the General Meeting sessions
plus related meetings.
| Day |
Date |
Meeting |
Location |
| Sun |
Feb 7 |
Registration (2-6 pm) |
Zero Penthouse at Zero Davey |
| Icebreaker Reception (4-6 pm) |
Zero Penthouse at Zero Davey |
| Mon |
Feb 8 |
General Meeting sessions (morning) |
University of Tasmania |
| General Meeting sessions (afternoon) |
University of Tasmania |
| Tue |
Feb 9 |
General Meeting sessions (morning) |
University of Tasmania |
| Visit of Hobart Station (afternoon) |
Mt. Pleasant Observatory |
| Wed |
Feb 10 |
General Meeting sessions (morning) |
University of Tasmania |
| General Meeting sessions (afternoon) |
University of Tasmania |
| Conference Dinner (evening) |
Barilla Bay Restaurant |
| Thu |
Feb 11 |
VLBI2010 Developers and Analysis meeting (all day) (*) |
University of Tasmania |
| Fri |
Feb 12 |
Directing Board meeting (all day) |
University of Tasmania |
| Sat |
Feb 13 |
mini-TOW (full day) |
Mt. Pleasant Observatory |
(*) The VLBI2010 Developers and Analysis meeting is a joint meeting of the
Analysis groups (Analysis Workshop), Working Group 4, and the VLBI2010
Committee and VLBI2010 developers.
A day-long Technical Operations Workshop (mini-TOW) is being organized by
This workshop is intended to provide an opportunity for station personnel
attending the General Meeting to discuss issues and problems. It will provide
hands-on training and problem resolution in VLBI operations. Topics covered will
include, among other things, VLBI basics, experiment pre-checks and operations,
RFI, phase calibration, and FS remote control.
There is only limited space available; hence only limited attendance is possible.
The current list of mini-TOW participants
(teachers and students) encompasses 20 people. Please contact the organizers about
the option to be included.
Following the General Meeting week, a VLBI-related full-day workshop will be held in
Auckland, New Zealand. Prior to the
SKANZ2010 Conference,
a workshop "VLBI and GNSS: New Zealand and Australian Perspectives"
will be organized on Monday February 15, 2010. This workshop is logistically tagged on the
SKANZ2010 Conference
and includes the option to participate in the site visit of the new VLBI station
at Warkworth on Tuesday February 16. Please check the SKANZ2010 Web site for more
information and make your travel plans accordingly.
General.
The local organizing committee has blocked a number of rooms in the on-campus
housing facilities and in a selected hotel. These two options should be requested
together with the registration. Please use the registration and accommodation
form for this action. The form is available in PDF
and in Word format. Please fill in the
appropriate parts and send it to the local organizing committee. The deadline
for arranging accommodation through the local organizing committee is
January 7, 2010. If you prefer to seek other lodging
options, please feel free to make use of the recommended accommodation for the
Sandy Bay area given below.
On-campus option.
Accommodation for the conference is available at the new
University Apartments, completed in August 2004. The University
Apartments boast spectacular views over the city of Hobart and the Derwent River and
is only a short walk from the campus (5 min). Single rooms with shared facilities are
available for $40.00 AUD per night. Each room is in an apartment of six reserved for
conference delegates, the apartments each have two bathrooms, a shared kitchen and
lounge/dinning room. Bookings can be requested as part of your registration. Please
let the local organizing committee know if you would like to share your apartment
with any particular people.
Hotel option.
A limited number of rooms have also been reserved at
Wrest Point Hotel & Casino
and can also be requested as part of your registration. Wrest Point is 7 minutes walk to
the University. 4.5 star hotel accommodation with city and harbour views. Rooms
range in price from $156 AUD to $184 AUD per night. Note: As of
January 6 the Standard Room for $156 AUD is sold out.
Further options.
For participants not wishing to stay at the provided accommodation we recommend
several other hotels and lodging
options in Sandy Bay which are all within walking distance of the University.
If you are having trouble booking accommodation for the meeting, please contact
the local organizing committee.
The registration fee includes conference materials, conference dinner, coffee
breaks, and catered lunch breaks. There is an early bird rate of $280 AUD and
a regular rate of $380 AUD. The early bird rate is payable via credit card by
the early bird deadline. The regular rate is payable by credit card by the
regular registration deadline or in cash at the meeting.
The deadline for registering for the early bird rate was
November 30, 2009. Deadline for the regular
rate was January 7, 2010. Please use the
registration and accommodation form to register for the meeting. The form
is available in PDF and in
Word format. Please fill in the
appropriate parts and send it to the local organizing committee.
Note: Pre-meeting registration is now closed. Potential participants who
want to register late should get in contact with
.
Once your registration has been processed, your name will be added to the
registration list.
The draft program of the meeting is available for download in PDF format.
Please send a note to
if you discover any mistake. The book of abstracts is currently being worked
on and will be available in the third week of January.
- Draft program (A4, 15 pages),
- Book of abstracts: not available yet
Hard copies of the final program and book of abstracts will be provided to
particpants at the meeting.
The Program Committee and session conveners prepared the following session descriptions.
| Session |
Title |
Conveners |
Description |
| 1 |
Realization and New Perspectives of VLBI2010 |
,
|
The outstanding VLBI results available today are valuable for various fields
of science and research and are needed for many practical applications. Due
to its unique features VLBI plays a key role in the maintenance of precise
global reference frames, TRF and CRF, and in the provision of all Earth
Orientation Parameters. The unprecedented new capabilities of the next
generation VLBI system of 1-mm positional accuracy and station velocities of
0.1 mm/yr, continuous observational
time series for station positions and Earth orientation parameters, and fast
turnaround time from observation to geodetic result will foster new science
and applications. |
| 2 |
Network Stations, Operation Centers, Correlators |
,
|
This session focuses on the recent activities and future plans at VLBI networks,
stations and correlators. Presentations about issues that relate to improving
VLBI data quality in general and more particularly with regard to "VLBI2010"
are solicited. Also welcome are submissions concerning the GGOS Project's
contributions to local surveys to determine the spacial vectors from the
radio telescopes to co-located geodetic instruments. Network station status
reports should be submitted to this session. |
| 3 |
VLBI Data Structure, Analysis Strategies and Software |
,
|
IVS data are collected at the IVS Data Centers and analyzed by the IVS Analysis
Centers. In this session, we call for contributions related to the IVS Data and
Analysis Centers' activities and plans for the future. We solicit contributions
from the IVS Data Centers concerning data flow, services for users, reliability
and timeliness of data exchange between the primary Data Centers. IVS Analysis
Centers are invited to contribute papers related to their current activities,
development and comparison of models and software used for the data analysis, and
assessment of the errors and accuracy of the VLBI results. We expect VLBI data to
increase dramatically—by at least a factor of 10, and maybe a factor of
100—in the near future because of VLBI2010. Because of this, we are
especially interested in Data Centers and Analysis plans related to automation
of data collection, processing and analysis. Presentations related to the
comparison and development of analysis strategies are welcome, as our changes
that need to be made because of VLBI2010. |
| 4 |
Interpretation of VLBI Results in Geodesy, Astrometry and Geophysics |
,
|
The analysis of VLBI observations produces time series, long-term average
positions and rates, and values of physical parameters. Suggested topics include
the use of such VLBI results in modeling geophysical fluids from the atmosphere
to the core, nutation/precession, high frequency Earth orientation changes,
refinement of the terrestrial and celestial reference frames, interpretation of
the motions of specific sites and radio sources, astrophysical investigations,
tests of relativity, and other scientific uses of geodetic and astrometric VLBI
data. Also included are investigations of the troposphere and the ionosphere by
VLBI. Another area is the comparison, validation and combination of VLBI with
other space geodetic techniques, and the integration of the techniques within
the framework of IAG's Global Geodetic Observing System (GGOS). |
| 5 |
Progress in Technology Development |
,
|
This session will concentrate on new technology developments in VLBI that have
occurred recently or are currently in development. Included (but not limited
to) are such topics as 1) development of digital processing technologies in the
VLBI signal chain that are expected to soon replace traditional analog BBC’s,
2) continuing development and deployment of advanced high-data-rate disk-based
recording systems, 3) transmission of raw VLBI data via high speed networks,
dubbed ‘e-VLBI’, 4) new correlator technologies and techniques, 5) RFI excision
techniques, 6) advanced calibration techniques and 7) automation of station
operations. Contributors to the session are encouraged to report their progress
and ideas on new technologies and methods, and to show how these new developments
will improve the overall VLBI program. |
The extended abstract submission deadline was December 2, 2009. Abstract submission
is now closed. If you want to submit a late abstract, please contact
Dirk
Behrend.
The Program Committee and conveners has reviewed all contributed paper submissions.
All contributed papers have be accepted. Due to the large amount of submitted oral
presentations about ten contributions have been changed from an oral to a poster
presentation after consulting the authors. A draft program is available in the
Program section.
Visa. In order to enter Australia you will need a visa, an
Electronic
Travel Authority (ETA), or an eVisitor—depending on your nationality. Either of these
must be obtained before travelling to Australia. The ETA and eVisitor are applied
for electronically. eVisitor is available to passport holders from the European Union
and a number of other European countries; there is no fee for the online application of
eligible passport holders. An ETA can be applied for through a
travel agent, airline, specialist service provider or an Australian visa office
outside Australia. Eligible passport holders have to pay a fee (currently $20 AUD).
If your country is not listed in the ETA or eVisitor eligibility lists, please check
with the Australian Embasssy/Consulate in your country on the required visa procedure.
Tourism. Tasmania is a favorite vacation spot boasting 18 National
Parks which protect the largest area of temperate rainforest remaining on earth, a
World Heritage Area. The local organizers have assembled a Web page with suggested
tours and destinations from short trips to longer journeys. Please visit the GM2010
Tourist
Information page to get inspired.
Time. Tasmania observes daylight saving time during the (southern)
summer months and is then 11 hours ahead of Univsersal Time: Australian Eastern
Daylight Time (AEDT) = UTC + 11 hrs.
Money. Australia's currency is the Australian dollar, made up
of 100 cents. There are 5c, 10c, 20c, 50c, $1, and $2 coins, and $5, $10, $20, $50,
and $100 notes. Although the smallest coin in circulation is 5c, prices are often
still marked in single cents. and then rounded up to the nearest 5c when you come
to pay.
Electricity. Plugs have three flat pins; the electricity supply is
220-240 V AV at 50 Hz.
IVS will send a letter of invitation to attend the meeting as a means of support.
If this would be of assistance for your travel plans, please contact the
IVS Coordinating Center
to request a letter. If you need a letter from the Australian meeting host,
please contact .
The members of the Program Committee were named by the Directing Board. Members are:
Members of the local organizing committee are:
Please feel free to contact any of the committee members with any questions.
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