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World Digital Magnetic Anomaly Map (WDMAM2005)
Task
Force meeting
Notes from Meeting
Number 3
by Juha V. Korhonen, Marta
Ghidella, Glenn Johnstone
Where: Potsdam
When: 2003 September
7, 2003
During: SCAR Geosciences SSG meeting at ISAES 2003
Present: Juha Korhonen (co-chair), Marta Ghidella, and members of the SSG and ADMAP project.
Summary
The relationship between
WDMAM and the Antarctic Digital Magnetic Anomaly Project (ADMAP) was discussed
during a meeting of the SCAR Geoscience Scientific Standing Group (GSSG).
The creation of an ADMAP
Action Group within GSSG was welcomed and agreed to by members at the
meeting. The formalisation of ADMAP as
an Expert Group will take place at XXVIII SCAR (Bremen) and will begin work
immediately – with Dr Marta Ghidella being nominated and appointed as the interim Chairperson for
the group.
Background
The International Symposium
on Antarctic Earth Sciences (ISAES) is held every four years at different
places in the world. The 9th meeting was held this year at the
University of Potsdam, Germany, between 8-12th September. There were
many ‘out of hours’ workshops and side meetings, and one of them was an
informal gathering of the GSSG on September 7th (GeoReach 2.4, the
GSSG newsletter, available at www.geoscience.scar.org/actiongroups/cog/)
Prior to the venue, the
GSSG Chief Officer, Phil O'Brien (Australia) had circulated a tentative agenda
between the GSSG members and asked for suggestions of other topics to be
included. M. Ghidella (who had recently become a member of WDMAM) proposed the
inclusion of the relationship between WDMAM and ADMAP in the agenda, and was
accepted. M. Ghidella then circulated an invitation to both ADMAP and WDMAM
members to attend.
The meeting was finally
held, chaired by Phil O'Brien (Australia) and Alessandro Capra (Italy). In
addition to the SSG members (not all) Juha Korhonen from WDMAM and four members
of ADMAP were present. Glenn Johnstone, Chairman of the Communication &
Outreach Group of the GSSG, was also present.
ADMAP as a group had been
quiet for the last few years, since the publication of a magnetic anomaly map
of Antarctica in 20010,
therefore there were two important issues to deal with:
1.
to revise the ADMAP status;
and
2. to define its relation with WDMAM.
Notes from meetings
ADMAP
The latest results of ADMAP
had been the publication a map (Golynsky et al., 2001see complete reference below) and the
production a special issue of Tectonophysics with related papers
(Magnetic Anomalies of the Antarctic, Vol. 347, 2002). The map, in digital
form, as well as the corresponding grid, are available from the Internet, but
are password protected. These can be
found at www.geology.ohio-state.edu/geophys/.
Further information about
ADMAP and its members can be found on the GSSG web site set up by Glenn
Johnstone in 2002: www.geoscience.scar.org/admap/
Several issues were
pending, first regarding if and how ADMAP was going to continue.
If it was not, there were some pending tasks, such as the production of a CD or
a DVD with the line data, as well as metadata. One case for continuation of the
project was that there were many new data sets that had to be incorporated to
the compilation - as the existing version only contains data up to the year
1997.
Concern was voiced that the
location of some of the datasets already used was unknown by the
attendees, as well as poor or non-existent metadata records for the line
data. To locate the line data,
and to re-organize the production of metadata records was
recognized as a necessary immediate task to address. This made it very
difficult to use any line data with reliability.
Alexander
Golynsky (Russia), the most hard working ADMAP member regarding compilation
work, gave a talk in which he explained the work he had done and also showed
further work he produced with data that are not in the compilation yet.
The importance of the
availability of line data was discussed.
They will be needed for further modification of the compilation with the
addition of new data, for planning new surveys and to address the task of examination
of the long wavelengths.
Alexander Golynsky (Russia), the most hard working
ADMAP member regarding compilation work, gave a talk in which he explained the
work he had done and also showed further work he produced with data that are
not in the compilation yet.
WDMAM
Juha Korhonen gave a
presentation on the current status of the project. In summary, he made the
ADMAP and GSSG people know the following (from GeoReach 2.4):
WDMAM is being undertaken
by the International
Association of Geophysics and Aeronomy (IAGA) Division 5.
The aim of the project is to source, collate and integrate magnetic anomaly
data from around the globe. Some work has already been done by ITC Delft in
compiling a global index of aeromagnetic data. There is, however, much more to
be done. Dr. Korhonen is interested in working with the ADMAP group to provide
the Antarctic component of the WDMAM.
J. Korhonen noted that
there are many issues surrounding access to data, data quality and data
storage. These are exactly the type of issues that have been identified by a
number of SCAR groups including GIANT, Geographic Information and JCADM.
Glenn Johnstone mentioned
there are a number of other international groups such as the Global Mapping
initiative (Japan) and the Permanent Committee on GIS Infrastructure for Asia
and the Pacific (PCGIAP) which have developed policies – particularly in
relation to the sharing or access to data. Glenn undertook to email Juha
Korhonen information about data sharing policies adopted by these groups.
Outcome: That ADMAP becomes an Expert Group of SCAR GSSG –
chaired, in the interim,d
by Dr Marta Ghidella (Argentina). This will be formalized at XXVIII SCAR and will get sstart worked immediately.
Outcome
In addition to the formal
outcome published in GeoReach, the result is that ADMAP acquired new life.
During the rest of the week, while ISAES was evolving, there were several
encounters between the ADMAP members, now including people that had not yet
arrived in Potsdam on Sunday 7th.
The news that ADMAP was in
action again was thus spread, and one on site result was the planning for the
production of a CD with the line data and metadata.
Follows the beginning of Carol
Finn
has provided a's of the summary of thea discussion of ADMAP people on September 10 in Potsdam:
To re-start progress
on compiling a master ASCII database, we revisited a variety of issues
discussed over the years. In accordance with the
original ADMAP protocols, we agreed that all ASCII point data for magnetic
surveys > 5 years old should be submitted to a master database in a
consistent format. We also agreed to include metadata.
Golynsky, A.,
M. Chiappini, D. Damaske, F. Ferraccioli, J. Ferris, C. Finn, M. Ghidella, T.
Isihara, A. Johnson, H.R. Kim, L. Kovacs, J. LaBrecque, V. Masolov, Y. Nogi, M.
Purucker, P. Taylor, and M. Torta, 2001: ADMAP - Magnetic Anomaly Map of the
Antarctic, 1:10 000 000 scale map, in Morris, P., and R. von Frese, eds.,
BAS (Misc.) 10, Cambridge, British Antarctic Survey.ADMAP - Magnetic Anomaly map of the Antarctic (2002). Sheet
No. BAS (Misc) 10. British Antarctic Survey. BAS miscellaneous Series.
Editors: P. Morris, R. Von Frese. Authors: A. Golynsky, M. Chiappini, D.
Damaske, F. Ferraccioli, J. Ferris, C. Finn, M. Ghidella, T. Isihara, A.
Johnson, S. Kovacs, V. Masolov, Y. Nogi, M. Purucker, P. Taylor, M. Torta.