Title: SWWT Initiatives - Long term monitoring of Sun-Earth Interactions
1SWWT Initiatives - Long term monitoring of
Sun-Earth Interactions
- F. Lefeuvre
- contributions from 16 groups or individual SWWT
members
2CONTEXTE
- SW activities rely on long term ground-based and
space - based observations - Long term monitoring of the geospace (solar
corona, solar wind, magnetosphere, ionosphere,
atmosphere) is needed - - to understand physical mechanisms driving
Solar Earth interactions - - to identify time variations in the Earth
environment (space environment included) - - to provide SW services (forecast and
specifications) - Part of the observations are known to be
temporary (e.g. SOHO) - Other observations, continuously available
since many years e.g. magnetometers or
ionosondes) may be stopped due to changes in the
priorities of National Agencies -
3- The dual use of instruments (science and
operational activities), which should be an
advantage, may be viewed as a drawback - SWWT action in progress investigate the
possibility of creating a european coordination
structure (like ERANET) between all national and
international agencies involved (or to be
involved) in long term monitoring (long term
measurements, access to distributed data sets
with large data volume, model development ). - An ERA-NET (e.g. ASTRONET) does not provide new
funds but allows to agree on common strategies
and common support of programmes. - Three splinter meetings have been organized to
identify tasks for an ERANET-like structure. - - Paris meeting, elaboration of a
questionnaires sent to all SWWT members - - Toulouse and RAL meetings, discussion on
elements of the questionnaire. - The work is not completed.
42. OUTPUTS OF THE QUESTIONNAIRE- an example
the networks of g.b. magnetometers- synthesis
52.a The ground-based magnetometers
- What must be monitored
- The time and space variations of the Earth
magnetic field for time periods ranging from few
minutes to few decades in order to - - Earth magnetism,
- - dynamics of the auroral/polar regions,
- - determine the ionospheric current during SW
storms, - - produce geomagnetic indices and geomagnetic
field models, - - determine the ionospheric current during SW
storms, - - enable the calculation and estimation of the
induced geoelectric field and of the resulting
GICs in technological systems - Users are research institutes and industrial
companies
6- Present status, National and European funding
- - about 100 digital observatories (funded by
National Agencies) are gathered in the frame of
the INTERMAGNET network - - it is completed by more or less temporary
magnetometers (funded by National Agencies) run
by other networks like IMAGE - - the worlwide coordination of magnetic
observatories is made in the frame of an ad-hoc
IAGA working group - INTERMAGNET, consortium led by an executive
board (4 scientists), the technical issues and
standards are under the responsabilty of an
operating committee (14 scientists) - IMAGE, informal coalition between 10 European
research institutes who maintain magnetometers in
northern Europe
7- What are the gaps in the measurements and the
lack of coordination - - no gap in stations for Europe (planetary scale
, regional scale ?) - - coordination via IAGA ( an internal
coordination system for INTERMAGNET) -
- Benefit of a cooperation between National and
European organisms - - Cooperation allows reduction of costs and high
level technological infrastructure
82.b Synthesis
9Quantities to monitor Equipments Present driver Funding agencies Interest of a coordination
time and space Earth B field variations (Earth magnetism,dynam. Aur./polar regions) space and g.b. magnetom. Science (ind. users) National - maintain ( upgrade) technical performances
Cosmic ray fluxes and int. (effects on the Earth environt) g.b. neutron and muon monitors Science (ind. users) National Internat. - have data in line and archived
The structure of the ionosphere ionosondes Application (sci. users) National EU - secure the funding - maintain ( upgrade) technical performances
TEC variations Space and g.b. GNSS receivers Application (Sci. developt) National ESA - Secure the funding
Creation of an United Nation International
Committee for Global Navigation System (see
UNOOSA ICG)
10Quantities to monitor Equipments Present driver Funding agencies Interest of a coordination
High latitude ionosphere convection, conduction, (modelling) Super DARN EISCAT Science Intern. associations define a medium and long term strategy for long term monitoring
Scintillations (modelling) receivers Science? Applic. ? National Internat. data exchange
Solar activity g.b. (space ?) Magnetographs Coronographs H- a imagers Science (Ind. Users) National Internat. define a medium and long term strategy for g.b. and space measurements
Solar energy flux (understanding irradiance variations, therm ionosph. Res.) Space EUV/UV detectors g.b. F10.7 cm measurements (for proxy) Science (Ind. Users) TIGER SCOSTEP programme? National Internat. - secure the continuity of F 10.7 cm measurements - define a strategy (ISS?)
11Quantities to monitor Equipments Present driver Funding agencies Interest of a coordination
Coronal hole obs. (for CME prediction and detection) EUV soft x-ray images Science National Internat. define a medium and long term strategy for long term monitoring
Solar radio flux, signature of CMEs, shocks, SEP, .. Multi frequency radiotelescopes Science (Ind. Users?) National Internat. define a medium and long term strategy for long term monitoring
IMF and solar wind parameters at L1 Plasma and wave measurements on-board satellites Use by science as well as by application Internat. Define a European strategy
12General situation for Space based
measurementsLong term measurements(a) solar
corona and solar wind(b) radiationsPresent
situation - (a) supposed to be taken into
account by ESA/Sci.- (b) is the mission of the
ESA project of Tech network of CentersProblems
- (b) needs (a)- (b) has a scientific part
(ILWS)
133. INTEREST OF AN INTER-AGENCIES COORDINATION
STRUCTURE
- Ground-based measurements
- - secure the funding
- - optimize the space, time and frequency coverage
- maintain and improve the technical performances
- define strategies for long term monitoring
measurement (e.g. support of proposals for new
networks) - International equipments
- - define European medium and long terms
strategies - Space based measurements
- - facilitate dual use of satellites and ISS
(Science, Earth Observation and technical
satellite, etc.) or even dual satellites
14Access to distributed data sets with large data
volume ? get EU supports for data exchanges,
archiving, Virtual Observatories (in
particular via upstream actions) Model
development ? prioritize models to be developed
(and so supported) ? examine the possibility of
developing European global models
154. CONCLUSION
- long term monitoring is essential for scientific
as well as operational SW activities. Approaches
may-be different for ground-based measurements
and for space based measurements. Access to data
and model developments are complementary
problems. - Ground based measurements
- - National scientific agencies, which dont like
long time long term commitments, must be
convinced about the scientific objectives to fund
equipments - - Recommendations from Scientific Unions and/or
Interdisciplinary Bodies may help to convince
Scientific Unions - - IHY may give an opportunity to start new long
term monitoring (as an example The monitoring
of solar radio flux, signature of CMEs, shocks,
SEP, ... from a network of multi-frequency radio
telescopes) - - question what about the user needs?
16- Space based measurements
- - adapted strategies must be defined for long
term monitoring from space - - coordination is needed
- between ESA departments
- between ESA and National Space agencies
- with other European Space entities (EUMETSAT)
17- In all cases, a coordination between all partners
would be very useful - An ERA-NET could be a solution. This proposal has
first to be tested with ASTRONET