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
Information for Authors
Presentations
Proceedings
Travel Information
Invitations
Program Committee
Local Committee
Pictures
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. From the University of Tasmania you can
follow a walk (40-45 min) suggested by Google maps or hire a cab (about 10 min drive).
View Walking Directions in New Tab
Please see an overview of all conference related locations on Google map at
http://tinyurl.com/ivsgmmap
courtesy of Jim Lovell.
If you are a user of Google Earth, please feel free to download the
meeting .kmz file (zipped kml, Keyhole Markup Language).
The file will start Google Earth and "fly" you to specified locations. It provides a
general view of the AuScope sites and indicates the conference venue, some of the
accommodation, good local restaurants and the like. Thanks to Jim Lovell for putting
this together.
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. The program
of the joint meeting is available in PDF format.
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.
We have reached the capacity limit and have started a waiting list. If a signed
up student cannot attend, the highest entry from the waiting list will fill the
vacant spot. We apologize for the inconvenience. You can check the current
list of mini-TOW participants (teachers
and students) and the waiting list. 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 program and booklet (incl. abstracts) of the meeting are available for download
in PDF format. Please send a note to
if you discover any mistake.
- Program (A4, 14 pages, 620 KB),
- GM booklet: program plus abstracts (A4, 58 pages, 2,164 KB)
Hard copies of the program and GM booklet (book of abstracts) will be provided to
participants 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 |
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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 |
,
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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 |
,
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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 |
,
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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 |
,
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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.
Both oral and poster papers will be published in the meeting proceedings. Please see the
proceedings section of this page for instructions on preparing
manuscripts.
Information for oral papers:
- All oral papers are 15 minutes, including discussion. Invited papers are 20 resp.
25 minutes, including discussion.
- Presentation equipment will include a PC projector (plus laptop), one overhead
projector, a wireless microphone for the speaker, and a laser pointer.
Oral contributions are to be uploaded prior to the session. This should be
done before the session is held (preferably a day earlier). You can perform the
upload at the registration desk at Zero Davey on Sunday, February 7, or in
the auditorium Monday through Wednesday, February 8-10. The auditorium and
poster area are on the campus of the University of Tasmania at Hobart in the
Physics building.
Information for poster papers:
- The space available for posters will be 180 cm tall by 100 cm wide.
- Materials for mounting posters will be provided.
- Posters can be put up in the poster area Monday morning.
- Posters will be left up for the duration of the meeting till Thursday 18:00.
All oral presentations and some poster presentations given at the meeting are
available for downloading. You can either directly
browse all presentation files or you can visit the
presentations page that will provide you
with individual links to the presentations.
Papers presented at the General Meeting will be published in a volume of Proceedings.
The proceedings will be published as a NASA Conference Publication. The reference
should be cited as follows: IVS 2010 General Meeting Proceedings, edited
by D. Behrend and K. D. Baver, NASA/CP-2010-xxxxxx (Note: NASA's publication office
will provide the running number 'xxxxxx', once the proceedings volume is finalized.)
Authors must follow the instructions for manuscript
submission. The deadline for submission of files for publication is
April 15, 2010.
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.
Arriving in Hobart. Most flights to Hobart go via the major hubs
of Sydney or Melbourne. At Hobart airport there are no money changing facilities.
If you intend to change money to get Australian dollars, you are advised to do that
at the Sydney or Melbourne airports. However, there is an ATM at Hobart airport where
you can draw money, provided your bank card (and PIN) are set up to work overseas.
Airport transportation. Taxis and airport bus services are available for
transport to Hobart and the University of Tasmania. A taxi form the airport is $50-60 AUD
and takes about 30-35 minutes. There are two bus services. (1) The Redline Airporter bus meets all incoming flights at Hobart airport. You
do not need to book a ticket if you are traveling form the airport to Hobart city (just
jump on the bus at the airport), but you do need to book in advance if your are traveling
to the airport. The cost is $15 AUD one-way, and $25 AUD return. If you are going to
the University Apartments, the bus driver will drop you off at bus stop 14. From bus
stop 14 it is still a 10-min walk up a steep hill to the University Apartments. All
major hotels are serviced directly. (2) The Southern Airport Pick-up Service will drop you
off and collect you at a range of locations in Hobart, including (unlike the Redline
Airporter bus) directly at the University's Accommodation Services office. For the
Southern Airport mini-bus advance bookings are essential, a 2 or 3 days' notice is
advisable. For bookings call +61-(0)3-6231-5080 or e-mail
letsseeTasmania@tastel.net.au or
cruisecompanytas@bigpond.com.
The cost is $25 AUD one-way from the airport to city locations, including the
University.
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.
You can find pictures taken during the meeting week in the links given below. If you
want to make your pictures available, please send a note to
Thumbnail listing of pictures:
You can also browse and download picture files on the ftp server.
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