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The ISR roadmapThe ISR roadmapin the COOPEUS projectin the COOPEUS project
Anders Tjulin, EISCAT Scientific [email protected]
EISCAT User Meeting 2015 ISR Roadmap 2
What is COOPEUS?
● A programme connecting research infrastructures– Supported by the EU (FP7) in cooperation with NSF– September 2012 – August 2015
● Five areas of research– Space weather– Carbon observations– Biodiversity– Ocean observations– Solid earth dynamics
● Partner institutes in USA and Europe
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COOPEUS structure
● Analytical phase– Commonalities and gaps connected to data and information
collection and sharing within the communities in Europe and across the Atlantic are identified
● Intermediate synthesis phase– Collect the results– Identify case studies
● Domain specific user scenarios● Event specific user scenarios
● Study phase– Case studies carried out
● Final synthesis phase– Define roadmap for future cooperation
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COOPEUS Task 2.5
● Task 2.5: Construction of joint atmospheric radar roadmap– In this task, we will develop a common approach to facility scheduling
and operating procedures, which will optimize the co-ordination of EU and US facilities at an observational level, in order to ensure best value return from the entire observing network.
– We will also develop a common understanding of the priorities for future facility developments and upgrades.
– The output will be a joint roadmap for ISR observations including recommendations for how a common scheduling and operational philosophy can be implemented and a list of prioritized future tasks to improve the co-ordination of existing facilities and the interoperability of their data.
– In this way, we will map out a co-ordinated approach for the international community, extending beyond the lifetime of the project.
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The roadmap
● The finished roadmap is available for download– www.coopeus.eu/progress/
● Based on discussions with COOPEUS project partners and e-infrastructure operators
● Recommendations for incoherent scatter radar operations
EISCAT User Meeting 2015 ISR Roadmap 6
Why do we need ISR observations?
● ISR technique is one of the most powerful methods for detailed measurements of the ionosphere– Electron density– Electron and ion temperatures– Bulk flow
● Observing connection between Sun and Earth– Solar-terrestrial physics– Space weather
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Trends in ISR research
● Generally increasing interest in environmental sciences– International collaborations– Global coverage
● Space weather prediction– Improved dependence on modelling of effects
from space weather events● Continuous observations
– Moving from campaigns towards observatories● Larger data volumes and quicker data access
requirements
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The global context
● The ionosphere ignores political borders
● Observations should ideally also ignore political borders
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ISR systems in the world
● There are more than fifteen facilities in the world capable of ISR observations
● COOPEUS involves EISCAT and US systems
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ISR facilities in the COOPEUS project
EISCAT UHF
EISCAT VHF
EISCAT UHFEISCAT Svalbard Radar
EISCAT_3D
Millstone Hill
Jicamarca
Arecibo
JicamarcaSondrestrom
PFISR
RISR
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ISR facilities in the COOPEUS project
Operator Owner Funder First operation
EISCAT UHF EISCAT EISCAT SA, STEL, NIPR, CRIRP, NFR, NERC, VR 1981
EISCAT VHF EISCAT EISCAT SA, STEL, NIPR, CRIRP, NFR, NERC, VR 1985
EISCAT Svalbard Radar EISCAT EISCAT SA, STEL, NIPR, CRIRP, NFR, NERC, VR 1996
EISCAT_3D EISCAT EISCAT TBC TBC
Millstone Hill MIT MIT NSF 1960
Jicamarca Radio Observatory Cornell University Instituto Geofisico del Perú NSF 1961
Arecibo Observatory SRI International NSF NSF 1963
Sondrestrom SRI International NSF NSF 1983
PFISR SRI International NSF NSF 2007
RISR SRI International NSF (University of Calgary) NSF (University of Calgary) 2009 (2011)
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The need for a roadmap
● Large variations in equipment and organisation– Harmonisation needed for efficient collaboration
● Increasingly more data intensive– Common strategy for data formats and access– Must be in line with capabilities and standards set by e-infrastructure providers
● EISCAT_3D to be constructed “soon”– Defining system for the future– Ready for future standards
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Areas for collaborative efforts
● Identified areas where collaborative efforts suitable and of great value– Definition of data levels– Data format– Access– Standard operations– Non-standard operations– Training and education– Outreach
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Data levels● Data levels used in ISRs were identified earlier in the COOPEUS project
– Presented at EISCAT_3D Users Meeting 2014● Level 1: Lowest accessible level of digital sampled and filtered data
– System-specific– Not normally stored
● Level 2: Correlated data products– Data exchange– Used for long-term storage
● Level 3: Physical parameters– Most requested from users
● (Level 4: Graphical visualisations and published articles)● Sufficient metadata needed for all levels
Receiver
RF signal voltageV(t)
Correlated productsV(t)V*(t+T)
Plasma parametersn, Te, Ti, ...
Correlator Fitter
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Data format
● Level 1– Traditionally no standards have been needed– Storing these data requires standards– HDF5 used at AMISR and Millstone Hill a starting point
● Level 2– Largest harmonisation effort needed here– HDF5 is a starting point
● Level 3– Standard data container used by the Madrigal database– Should be upgraded/changed to handle EISCAT_3D data
Common Features of Correlated ISR Data Formats
System metadata
Antenna – specified for TX and RX systems separately:
Site reference coordinates
Number of beams
For each beam:
Beam shape
Beam pointing
Beam pointing coordinate system
For each feed polarisation:
Feed bandpass shape
Feed amplitude and phase calibration
Transmitter:
TX frequency time history
Modulation envelope time history:
Amplitude
Phase
Peak power
Average power
Receiver:
Number of channels
For each channel:
Association of that channel with antenna beam / feed / polarisation, or with sampled TX channel
Receiver centre RF frequency
Receiver final frequency (=0 for baseband data)
Receiver effective impulse response / bandpass shape (amplitude and phase)
Receiver timing:
RF blank interval, if present
Attenuation time history
Noise calibration diode injection system parameters (if present):
Timing of noise calibration pulse injection
Absolute noise calibration pulse power
Receiver amplitude and phase calibration
Receiver noise temperature
Correlated product data
Number of lag profiles
For each lag profile:
Associated receiver channels (different if cross-correlation, same if auto-correlation)
Associated transmitted modulation
Radar ambiguity function: delay × lag × range
Time average interval
Start offset from leading edge of TX pulse
Range sampling vector
Lag sampling vector
Lag product matrix (range × lag)
Lag product variance matrix (range × lag)
DC offset as a function of range
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Access
● Access to data– Madrigal exists now for level 3 data
● Other data portals could also be offered
– Data available through requests– Technical solutions under discussion in several projects
● Access to facilities– Technical aspects– Access rights
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Standard operations
● All facilities have a set of standard modes● Increased value if these could be combined for global view of
ionosphere● Continuous, or near continuous, operation of great value to study
trends through long data series– Such operations only possible from a limited number of ISR facilities– Financing the high costs for continuous operations is a big issue
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Non-standard operations
● The incoherent scatter radar world days are coordinated observations by the ISRs of the world– About 20 per year– Scheduled well in advance– Coordinated through the Incoherent Scatter Working Group of URSI– Data available as soon as possible
● Protocols for unplanned coordinated observations are needed– For example following large space weather events
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Training and education
● ISR operator community is very small● Training of engineers should be coordinated
– Not automatic – projects for this have to be defined● Education of users should be coordinated
– International ISR courses are organised regularly
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Outreach
● The ISR operator community should have a common voice– Limited to commonalities
● Protection of radio frequencies● Stressing the importance of continuous observations
● Projects to streamline this coordination should be identified
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Communication channels
● The COOPEUS project has shown us:– where coordination can be made– how difficult coordination is in practice
● Identify channels to discuss the needed harmonisation actions– URSI ISWG meetings (every three years) a possible starting point
● An arena for coordination needs to be organised, and funded, in a sustainable fashion
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Recommendations on organisational level (part 1)
● Identify a sustainable arena that is suitable for discussions on international coordination.
● Follow the COOPEUS joint data policy.● Work towards the introduction of persistent data identifiers.● Agree on a level 2 data standard and make sure that it is suitable for long term storage.● Make sure that the level 3 data produced are fit to be used in common data portals by
connecting sufficient amount of meta-data.● Prepare protocols for migration of data, both to new formats and new depositories.● Open for possibilities to implement a common scheduling and operational philosophy.
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Recommendations on organisational level (part 2)
● Continue the incoherent scatter world days planning as it is done now.● Make sure that protocols exist for event-driven observations, where one
facility/organisation can suggest operation of other facilities/organisations.● Make efforts to expand the ISR community through high visibility and good
connection to academic institutions.● Identify projects for training and exchange of radar operation engineers.● Continue the incoherent scatter radar summer schools.● Identify projects for coordinating outreach efforts.
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Recommendations on facility level
● Aim for using harmonised level 1 data format for the internal data processing.
● Ensure that data migration activities follow strategy protocols.● Use the ENVRI reference model as a guideline for the data framework.● Ensure that standard operating modes are defined for producing long-
term continuous data sets that can be used to observe ionospheric changes over time.
● Open for activities involving exchange of engineers for training purposes.