International VLBI Service
for Geodesy and Astrometry
TERMS OF REFERENCE
October 20, 1998
SUMMARY
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Objectives
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Data Products
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Research
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Components
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Coordination
COMPONENTS
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Network Stations
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Operation Centers
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Correlators
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Analysis Centers
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Data Centers
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Technology Development Centers
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Coordinating Center
COORDINATORS
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Technology Coordinator
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Network Coordinator
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Analysis Coordinator
DIRECTING BOARD
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IVS Associate Members
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Correspondents
1. SUMMARY
1.1 Objectives
The International VLBI Service for Geodesy and
Astrometry (IVS) is an international collaboration of
organizations which operate or support Very Long Baseline Interferometry
(VLBI) components.
The primary objective of IVS is to foster VLBI programs as a joint
service to support geodetic,
geophysical, astrometric, and other research and operational activities.
This is accomplished
through close coordination to provide high-quality VLBI data and products.
The second objective of IVS is to promote research and development
activities in all aspects of
the geodetic and astrometric VLBI technique. This objective also supports
the integration of
new components into IVS. The further education and training of
VLBI participants is supported
through workshops, reports, electronic network connections, and other means.
The third objective of IVS is to interact with the community of users of VLBI products and to
integrate VLBI into a global Earth observing system. IVS interacts closely with the
International Earth Rotation Service (IERS) which is tasked by the IAU and IUGG with
maintaining the international celestial and terrestrial reference frames and with monitoring Earth
rotation.
To meet these objectives, IVS coordinates VLBI observing programs, sets performance
standards for VLBI stations, establishes conventions for VLBI data formats and data products,
issues recommendations for VLBI data analysis software, sets standards for VLBI analysis
documentation, and institutes appropriate VLBI product delivery methods to ensure suitable
product quality and timeliness. IVS closely coordinates its activities with the astronomical
community because of the dual use of many VLBI facilities and technologies for both astronomy
and astrometry/geodesy.
IVS accepts observing proposals for research and operational programs that conform to the IVS
objectives.
1.2 Data Products
VLBI data products contribute uniquely to these important determinations:
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definition and maintenance of the celestial reference frame
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monitoring universal time (UT1) and length of day (LOD)
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monitoring the coordinates of the celestial pole (nutation and precession)
These results are the foundation of many scientific and practical applications requiring the use of
an accurate inertial reference frame, such as high-precision navigation and positioning.
IVS provides, through the collaborative efforts of its components, a variety of significant VLBI
data products with differing applications, timeliness, detail, and temporal resolution, such as:
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all components of Earth orientation parameters at regular intervals
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terrestrial reference frame
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VLBI data in appropriate formats
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VLBI results in appropriate formats
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local site ties to reference points
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high-accuracy station timing data
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surface meteorology, tropospheric and ionospheric measurements
All VLBI data products are archived in IVS Data Centers and are publicly available.
1.3 Research
The VLBI data products are used for research in many related areas of geodesy,
geophysics, and astrometry, such as:
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UT1 and polar motion excitation (over periods of hours to decades)
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solid Earth interior research (mantle rheology, anelasticity, libration, core modes,
nutation/precession)
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characterization of celestial reference frame sources and improvements to the frame
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tidal variations (solid Earth, oceanic, and atmospheric)
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improvements in the terrestrial reference frame, especially in the vertical (scale) component
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climate studies
To support these activities, there are ongoing research efforts whose purpose is to improve and
extend the VLBI technique in such areas as:
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improvements in data acquisition and correlation
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refined data analysis techniques
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spacecraft tracking (Earth-orbiting and interplanetary)
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combination of VLBI data and results with other techniques
Components
IVS acquires VLBI data, correlates the data,
analyzes the data to produce geodetic, astrometric, and other results,
and archives and publicizes data products.
IVS accomplishes its goals through the component described in the next
section.
IVS will accept proposals at any time for any of its components.
Such proposals will be reviewed by the Directing Board. The IVS
components are the following:
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Network Stations
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Operation Centers
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Correlators
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Analysis Centers
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Data Centers
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Technology Development Centers
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Coordinating Center
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Directing Board
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Associate Members
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Corresponding Members
Coordination
Specific activities for technology, network data quality, and data products are
accomplished through the functions performed by three coordinators:
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Technology Coordinator
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Network Coordinator
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Analysis Coordinator
2. COMPONENTS
IVS acquires VLBI data, correlates the data, analyzes the data to produce geodetic and
astrometric results, and archives and publicizes data products. IVS accomplishes its goals
through the components described below.
2.1 Network Stations
The IVS observing network consists of high performance VLBI stations.
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Stations can be dedicated to geodesy or have multiple uses (including astronomical
observations or satellite tracking applications).
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Stations comply with performance standards for data quality and operational reliability set
up by the Directing Board.
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VLBI data acquisition sessions are conducted by groups of Network Stations
that are distributed either globally or over a geographical region.
2.2 Operation Centers
The IVS Operation Centers coordinate the routine operations of one or
more networks. Operation Center activities include:
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planning network observing programs,
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establishing operating plans and procedures for the stations in the network,
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supporting the network stations in improving their performance,
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making correlator time available at an IVS Correlator,
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generating the detailed observing schedules for use in data acquisition sessions by IVS
Network Stations,
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posting the observing schedule to an IVS Data Center for distribution and to the
Coordinating Center for archiving.
IVS Operation Centers follow guidelines from the Coordinating Center for timeliness and
schedule file formats. Operation Centers cooperate with the
Coordinating Center in order to define:
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the annual master observing schedule,
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the use of antenna time,
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tape availability and shipping,
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the use of other community resources.
2.3Correlators
The IVS Correlators process raw VLBI data and station log files following a data
acquisition session. Their other tasks are to:
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provide immediate feedback to the Network Stations about problems that
are apparent in the data,
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jointly maintain the geodetic/astrometric community's tape pool,
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make processed data available to the Analysis Centers,
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regularly compare processing techniques, models, and outputs to
ensure that data from different Correlators are identical.
2.4 Analysis Centers
The IVS coordinates VLBI data analysis to produce high-quality results
for its users. These activities are performed by Analysis Centers,
which contribute to the IVS core products, and by Associate Analysis
Centers, which contribute other specialized products. Two types of
Associate Analysis Centers are recognized: Global and Special.
The Analysis Centers receive and process VLBI data from one or more IVS
Data Centers and are committed to produce the core products, without
interruption, and at a specified time lag to meet IVS requirements. The
IVS core products, at a minimum, consist of Earth orientation parameters,
station coordinates, and source coordinates. The Analysis Centers place
their final results in IVS Data Centers for dissemination to researchers
and other users. They adhere to IVS recommendations for the creation of
high-quality products and their timely archiving and distribution. Any
deviations that an Analysis Center makes from IVS recommendations are
properly documented. Analysis Centers provide timely feedback about
station performance.
The Global Associate Analysis Centers process all the observed VLBI
data. Some process data directly from Correlators and then make
available as products the final VLBI database files and SINEX files.
Others start with these database to perform their analyses, but will
process all the databases.
The Special Associate Analysis Centers analyze selected databases for
one (or more) specific interests, such as regional data processing,
terrestrial reference frame maintenance, or Earth orientation results.
In addition, all types of IVS analysis centers satisfy the following
standards:
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Analysis is performed using VLBI software packages that adhere to IVS
recommendations.
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Centers perform software development and produce documentation. They
periodically compare their products.
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Centers adhere to IERS Conventions. Any exceptions are documented.
2.5 Data Centers
The IVS Data Centers are repositories for VLBI observing schedules,
station log files, and data products. Data Centers may mirror other
Data Centers to make the distribution and maintenance
of data more efficient and reliable.
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Data Centers are the primary means of distributing VLBI products to users.
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Data Centers work closely with the Coordinating Center and with the
Analysis Centers to ensure that all the information and data required
by IVS components are quickly and reliably available.
Data Centers provide the following functions:
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receive and archive schedule files from Operation Centers,
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receive and archive log files and ancillary data files from the Network Stations,
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receive and archive data products from the Analysis Centers,
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provide access and public availability to IVS data products for all users.
2.6 Technology Development Centers
The IVS Technology Development Centers contribute to the development of new VLBI
technology. They may be engaged in hardware and/or software technology development, or
evolve new approaches that will improve the VLBI technique and enhance compatibility with
different data acquisition terminals. They will:
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design new hardware,
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investigate new equipment,
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develop new software for operations, processing or analysis,
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generate new information systems,
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develop, test, and document prototypes of new equipment or software,
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assist with deployment, installation, and training for any new approved technology.
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After dissemination of the new hardware or software, the centers may continue to provide
maintenance and updating functions.
2.7 Coordinating Center
The IVS Coordinating Center is responsible for coordination of both
the day-to-day and the long-term activities of IVS, consistent with the
directives and policies established by the Directing Board. Specifically,
the Coordinating Center monitors, coordinates, and supports the
activities of the Network Stations, Operation Centers, Correlators,
Data Centers, Analysis Centers, and Technology Development Centers.
The Coordinating Center works closely with the
Technology Coordinator, the Network Coordinator, and the Analysis Coordinator
to coordinate all IVS activities.
The primary functions of the Coordinating Center are to:
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coordinate observing programs approved by the Directing Board,
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maintain the master schedule of observing sessions,
coordinating the schedule with astronomical observing programs
and with IVS networks,
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foster communications among all components of the IVS,
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define the best use of community resources,
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develop standards for IVS components,
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provide training in VLBI techniques,
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organize workshops and meetings, including an annual IVS technical meeting,
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produce and publish reports of activities of IVS components,
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maintain the IVS information system and archive all documents,
standards, specifications, manuals, reports, and publications,
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provide liaison with the IERS, IAG, IAU, and other organizations,
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provide the Secretariat of the Directing Board.
Through a reciprocity agreement between IVS and IERS the Coordinating Center serves as the
VLBI Coordinating Center for IERS, and as such its designated representative, subject to the
Directing Board approval, is a member of the IERS Directing Board. Such a representative is a
non-voting member of the IVS Directing Board. In turn, the IERS Directing Board designates a
representative to the IVS Directing Board. This arrangement is to assure full cooperation
between the two services.
3. COORDINATORS
3.1 Technology Coordinator
The IVS Technology Coordinator is selected by the Directing Board
from responses to an open solicitation to the IVS Technology Development Centers.
The Technology Coordinator is responsible for coordinating the new
technology activities of IVS and for stimulating advancement of the VLBI technique. The
Technology Coordinator performs the following functions:
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maintains cognizance of all current VLBI technologies and ongoing development
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coordinates development of new technology among various IVS components
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helps promulgate new technologies to the geodetic/astrometric community
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strives to ensure the highest degree of global compatibility of VLBI data acquisition systems
The Technology Coordinator works closely with the astronomical community because of the
many parallels between the technology development required for both groups.
3.2 Network Coordinator
The IVS Network Coordinator is selected by the Directing Board
from responses to an open solicitation to all IVS components.
The Network Coordinator represents the IVS Networks on the Directing
Board and works closely with the Coordinating Center. The Network Coordinator is responsible
for stimulating the maintenance of a high quality level in the station operation and data delivery.
The Network Coordinator performs the following functions:
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monitors adherence to standards in the network operation,
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participates in the quality control of the data acquisition performance of the network stations,
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tracks data quality and data flow problems and suggests actions to
improve the level of performance,
The Network Coordinator works closely with the geodetic and astronomical communities who
are using the same network stations for observations. The Coordinator takes a leading role in
ensuring the visibility and representation of the Networks.
3.3 Analysis Coordinator
The IVS Analysis Coordinator is selected by the Directing Board
from responses to an open solicitation to the IVS Analysis Centers.
The Analysis Coordinator is responsible for coordinating the analysis
activities of IVS and for stimulating VLBI product development and delivery. The Analysis
Coordinator performs the following functions:
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fosters comparisons of results from different VLBI analysis software packages and different
analysis strategies,
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encourages analysis software documentation,
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participates in comparisons of results from different space geodetic techniques,
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monitors Analysis Centers' products for high quality results and for adherence to IVS
standards and IERS Conventions,
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ensures that analysis products from all Analysis Centers are archived and available for the
scientific community, and
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forms the official products of IVS, as decided by the IVS Directing Board, using a suitable
combination of the analysis results submitted by the Analysis Centers.
The Analysis Coordinator works closely with the geodetic and astronomical communities who
are using some of the same analysis methods and software. The Analysis
Coordinator plays a leadership role in the development of methods for distribution of VLBI
products so that the products reach the widest possible base of users in a timely manner. The
coordinator promotes the use of VLBI products to the broader scientific community and interacts
with the IVS Coordinating Center and with the IERS.
4. Directing Board
The Directing Board determines policies, adopts standards, and approves the scientific and
operational goals for IVS. The Directing Board exercises general oversight of the activities of
IVS including modifications to the organization that are deemed appropriate and necessary to
maintain efficiency and reliability.
A specific function of the Board is to set scientific goals for the
IVS observing program. The Board will establish procedures for external
research programs and will review any proposals thus received.
The Board may determine appropriate actions to ensure the quality of the
IVS products and that the IVS components maintain the adopted standards.
The Directing Board consists of appointed members who serve ex officio,
members elected by the Directing Board, and members elected by the IVS
components. The members are:
Appointed members ex officio:
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IAG representative
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IAU representative
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IERS representative
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Coordinating Center Director
Selected by Directing Board upon review of proposals from the
relevant IVS component (see below):
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Technology, Network, and Analysis Coordinators (3 total)
Elected by Directing Board upon recommendation from the
Coordinating Center (see below):
Elected by IVS Components (see below):
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Correlators and Operation Centers representative (1)
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Analysis and Data Centers representative (1)
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Networks representatives (2)
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Technology Development Centers representative (1)
Total number: 14
The four appointed members are considered ex officio and are not subject to institutional
restrictions. The other 10 persons must be members of different IVS components. At-large
members are intended to ensure representation on the Directing Board of each of the components
of IVS and to balance representation from as many countries and
institutions as possible. All
elected members serve staggered four-year terms once renewable.
Election of Board members by the IVS components shall be conducted by a
committee of three
Directing Board members, the chair of which is appointed by the chair
of the Directing Board.
The committee solicits nominations for each representative from the
relevant IVS components.
Networks representatives can be nominated by well-defined, operating
networks accepted as such by the Directing Board.
For each position, the candidate who receives the largest number
of votes from the Associate Members will be elected. In case of
a tie the Directing Board will make the decision.
The chair is one of the Directing Board members and is elected by the Board for a term of four
years with the possibility of reelection for one additional term. The chair is the official
representative of IVS to external organizations.
Most decisions by the Board are made by consensus or by simple majority vote of the members
present. In case of a tie, the chair shall vote but otherwise does not vote. If a two-thirds quorum is
not present, the vote shall be held later by electronic mail.
A two-thirds vote of all Board members is
required to modify the Terms of Reference, to change the chair, or to
change any of the members elected by the Directing Board
before the normal term expires.
The Board meets at least annually, or more frequently if meetings are
called by the chair or at the request of at least three Board members.
The Board will conduct periodic reviews of the IVS organization and its
mandate, functions, and components. The reviews should be done every
four years.
The Secretariat of the Directing Board is provided by the Coordinating Center.
4.1 IVS Associate Members
Individuals affiliated with organizations that participate in any of the
IVS components may become IVS Associate Members.
Associate Members are generally invited to attend non-executive sessions
of the Directing Board meetings with voice but without vote.
Associate Members take part in the
election of the incoming members of the Directing Board representing
the IVS components.
4.2 IVS Correspondents
IVS Correspondents are individuals on a mailing list maintained by the Coordinating Center.
They do not actively participate in IVS but express interest in receiving IVS publications, wish
to participate in workshops or scientific meetings organized by IVS, or generally are interested
in IVS activities. Ex officio correspondents are the following:
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IAG General Secretary
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President of IAG Section II -- Advanced Space Technology
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President of IAG Section V -- Geodynamics
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President of IAU Division I -- Fundamental Astronomy
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President of IAU Commission 19 -- Rotation of the Earth
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President of IAU Commission 8 -- Positional Astronomy
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President of IAU Commission 31 -- Time
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President of IAU Commission 40 -- Radio Astronomy
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President of URSI Commission J -- Radio Astronomy
Version date: 20 October, 1998