VAMDC Virtual Atomic and Molecular Data Centre C. Mendoza (IVIC, - - PowerPoint PPT Presentation

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VAMDC Virtual Atomic and Molecular Data Centre C. Mendoza (IVIC, - - PowerPoint PPT Presentation

VAMDC Virtual Atomic and Molecular Data Centre C. Mendoza (IVIC, CeCalCULA) With the collaboration of: J.Gonzlez (UCV), L.A. Nez (CeCalCULA) M.C.Witthoeft, J. Garca, T.R. Kallman (NASA) F. Delahaye, C.J. Zeippen (Obs. Paris)


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SLIDE 1

VAMDC

Virtual Atomic and Molecular Data Centre

  • C. Mendoza (IVIC, CeCalCULA)

With the collaboration of:

J.González (UCV), L.A. Núñez (CeCalCULA) M.C.Witthoeft, J. García, T.R. Kallman (NASA)

  • F. Delahaye, C.J. Zeippen (Obs. Paris)

Uncertainties in atomic data and how they propagate in chemical abundances Instituto de Astrofísica de Canarias 27 October 2010

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SLIDE 2
  • VAMDC aims at building an interoperable e-infrastructure

for the exchange of atomic and molecular data. VAMDC involves 15 administrative partners representing 24 teams from 6 European Union member states, Serbia, the Russian Federation and Venezuela.

  • VAMDC is supported by EU in the framework of the FP7

"Research Infrastructures - INFRA-2008-1.2.2 - Scientific Data Infrastructures" initiative. It started on the 1rst of July for a duration of 42 months.

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SLIDE 3

VAMDC integrates several research groups mainly from the European Research Area

NIST IVIC CeCalCULA UCL U Cambridge Open U Queen’s U U Uppsala U Cologne CNRS INA Italia AO Belgrade U Vienna RAS RFNC

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SLIDE 4

Users will navigate seamlessly and retrieve data from 21 A&M databases

NIST HITRAN OPserver XSTAR TIPbase TOPbase W@DIS

SPECTRA

OZONE CDSD SpecW3

BELDATA

LASP PAH KIDA UMIST STSP

BASECOL

CDMS CHIANTI VALD VAMDC

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SLIDE 5

A&M data are used in a wide variety of research and industrial fields

Astrophysics

Fusion plasmas Atmospheric physics Lighting Lasers Nanotechnology Environment S e m i c

  • n

d u c t

  • r

s

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SLIDE 6

Outstanding problems in existing A&M databases are interoperability and data interfaces

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SLIDE 7

VAMDC intends to deploy an interoperable e-environment for distributed A&M databases

database1 database2 database3 database4

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SLIDE 8

E E-

  • science is collaborative data

science is collaborative data-

  • intensive science

intensive science

Original image from Hey, Tansley & Tolle (2009)

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SLIDE 9

Radiative Radiative decay decay of

  • f 3pnp

3pnp 1

1P

P states states in in Mg Mg-

  • like

like ions ions

State RLT (ns) 3p4p 1P 3.47E+00 3p5p 3.67E+00 3p5p 3.72E+00 3p6p 3.73E+00 3p7p 3.74E+00 3p8p 3.75E+00 3p9p 3.78E+00 3p10p 3.87E+00 3pnp 1P 3smp 1Po dominant channel: n = m

Butler et al (1990)

Mg I

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SLIDE 10

E-science is changing scientific research dynamics

  • Distributed computer environments
  • Virtual organizations
  • Grids
  • Clouds
  • Data-base centric computing
  • Warehousing (IVOA, VAMDC)
  • Data mining
  • Applications accessible as WSDL/SOAP web services
  • Service integrators
  • Scripts
  • Workflows
  • Social networks as end users
  • Data-curation environments
  • XML-based data exchange (XSAMS)
  • Metadata
  • Data preservation
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SLIDE 11

The OPserver is a good example of database-centric computing

OPserver at OSC

From Mendoza et al. (2007)

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SLIDE 12

Data exchange strategy

Source: Ralchenco et al., 2008, ICAMDATA-6, Beijing

VAMDC

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SLIDE 13

VAMDC will provide a registry of A&M web services

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SLIDE 14

The XSTAR spectral modeling code is being

  • ffered as a SOAP web service

XSTAR uaDB Command-based app

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SLIDE 15

Once XSTAR is available as a web service, it can be integrated in a web page

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SLIDE 16

Once XSTAR is available as a web service, it can be integrated in a workflow system

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SLIDE 17

Once XSTAR is available as a web service, it can be integrated in a workflow system

xspec

  • bserved spectrum

Workflow inputs

  • bserved + synthetic spectra

Workflow outputs XSTAR std_output

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SLIDE 18

The computation of astrophysical opacities would be a topical example for a workflow system

Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA Start RMO/RA End RMO/RA

Opacity Code

EOS

OPserver RMO/RA

ionization fractions level populations

Atomic DB Mono DB application application application

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SLIDE 19

Workflows maybe published in scientific social network systems

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SLIDE 20

Workflow may become the blueprints of reproducible & adaptable scientific methods

Source: myExperiment

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SLIDE 21

We should attempt to form A&M data producer/user communities

Source: myExperiment

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SLIDE 22

OP Fe RMO at Z OP Fe RMO at Z conditions conditions is is being being questioned questioned

From Bailey (2008) Z conditions: T ~ 156 eV, ne ~ 1022 cm-3

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SLIDE 23

Model of the curation process

Original image from Lord et al (2004)

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SLIDE 24

Conclusions

Scientific research is becoming increasingly collaborative and data-intensive (e-science) Atomic data production must be scaled up to the extreme requirements of virtual organizations Data repositories must be kept fit and integral for contemporary purpose, discovery and reuse (e- science curation) Data preservation is of vital importance