Ingrid Mann EISCAT Scientific Association Background Project Status Opportunities
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1 The EISCAT 3D Project Ingrid Mann EISCAT Scientific Association Background Project Status Opportunities Ingrid Mann, 29 February 2012
2 What is EISCAT 3D: New generation atmospheric radar: multi-static phased array radars advanced digital processing EISCAT community heritage: radar instrumentation radar codes inversion techniques Image: EISCAT
3 Why EISCAT 3D: Need to replace existing system change observation frequency expand research theme stay competitive Image: EISCAT
4 When EISCAT 3D: discussions within EISCAT user community FP6 design study FP7 preparatory phase Need investments Image: EISCAT Need to start construction
5 ( ) Results of the Design Study Performance Specification Site surveys Frequency allocations Science Case Antennas Front End Beam- forming Imaging system Transmitter Data system E I S C A T_3D The next generation European Incoherent Scatter radar system FINAL DESIGN STUDY REPORT DELIVERABLE EISCAT Scientific Association D11.1 Universitetet i Tromsø University of Tromsø i June 2009 DesignStudy_Results
6 EISCAT 3D 2008 ESFRI: European Strategy Forum on Research Infrastructures to develop the scientific integration of Europe to strengthen its international outreach *EISCAT 3D for the environment
7 ( ) EISCAT 3D preparatory phase October 2010 September 2014 FP7 call: Construction of new infrastructures Aim: ensure that the EISCAT_3D project will reach a sufficient level of maturity with respect to so that the construction of the EISCAT_3D radar system can begin immediately after the conclusion of the phase.
8 ( )
9 EISCAT 3D Preparatory Phase Project Structure Projects partners: EISCAT Scientific Association Tromsø University Luleå University Swedish Institut for Space Physics Oulu University Swedish Research Council National Instruments Rutherford Appleton Laboratory
10 EISCAT 3D Preparatory Phase Project Structure General Assembly one member from each partner two members from coordinator Meets twice per year and makes major decisions
11 EISCAT 3D Preparatory Phase Project Structure Executive Board Members Esa Turunen Henrik Andersson Thomas Ulich Jonny Johansson Ian McCrea EISCAT (coordinator) EISCAT Oulun Yliopisto (UOULU) Luleå Tekniska Universitet (LTU) Science and Technology Facilities Council (STFC) Weekly telecon, Physical Meeting 4 x per year
12 EISCAT 3D Preparatory Phase Project Structure TAC members: Frank Lind, MIT Haystack (technical coordinator) Werner Singer, IAP Kuehlungsborn Tom Grydeland, Norut Tromsø Jan Geralt Bij de Vaate, Astron, Dwingeloo First meeting 15. September 2011 Plans two physical meetings per year
13 Project & Users EISCAT 3D user meetings 2010, 2011, 2012 Science group meetings twice per year Project All Hands meeting (once per year) National meetings Discussions during other EISCAT meetings
14 Project Status FP7 progress in different workpackages need more coordination of technical efforts first periodic report in March 2012 Swedish 2 year Planning Grant
15 Timeline* EISCAT 3D Decisions first commitments Consolidation Work on new agreement Site works commence Installation Manufacturing and/or Prototype build *reported to ESFRI September 2011 Preparatory Phase
16 Basic EISCAT 3 D cost of order 120 M plan modular construction adjust to funding scheme start at available sites initial site for prototype proof of concept & first science
17 Basic EISCAT 3 D Core: mono static transmitter/receiver array plus outlier receiver array 4 Remote sites: receive-only arrays
18 Basic EISCAT 3 D Core: mono static transmitter/receiver array plus outlier receiver array 4 Remote sites: receive-only arrays Supporting Instruments: heating facility CCD cameras with filters imaging spectrometer digital ionosondes platform for further instrumentation
19 EISCAT 3 D basic site configuration
20 Wishlist what core site location should permit: studying atmospheric phenomena at low altitude that appear east of the Scandinavian mountain range observing together with supporting optical instruments which requires clear skies measuring along the geomagnetic field lines that are followed by the downleg path of sounding rockets à optimum core site 69 N 20.5 E
21 EISCAT 3D Frequency need to keep 40 km distance from DAB transmitters
22 EISCAT 3D will be advanced laboratory to study plasma phenomena on small spatial scale ( 100 m) Opportunities flexible observatory for space weather and atmospheric studies (seconds to years) key facility in multi-instrument and global campaigns data provider for Earth system modelling ( TB/s, store 1000 TB/yr)
23 Opportunities Expanding Community Data handling & processing Atmospheric Modelling Education Collaborations in Nordic Region Image: EISCAT
24 Opportunity: EISCAT Finland Norway Sweden China Japan United Kingdom (contributions from France, Russia, Ukrania)..expand membership
25
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