1. Meteor Science Why and how? 1. Meteor Science Why and how? 3. Virtual Observatories State-of-the-art databases in astronomy 3. Virtual Observatories State-of-the-art databases in astronomy 4. Virtual Meteor Observatory State-of-the-art database in meteor science 4. Virtual Meteor Observatory State-of-the-art database in meteor science Context Problem Inspiration Solution 2. Meteor data mining Meteors as a statistical science 2. Meteor data mining Meteors as a statistical science Part of my YGT project at ESA
Meteoroid – a solid object moving in interplanetary space, of a size considerably smaller than an asteroid and considerably larger than an atom or molecule. (IAU, 1961) (Better definition: object in space between 100 μm and 10 m.) Interesting because… • they teach us about asteroids and comets (poorman’s Rosetta); • they are potentially harmful to spacecraft; • they look cool when they hit us!
see and what we want to know (Vaubaillon, 2005) (Top: Arlt, 2001. Bottom: Asher, 1999.) Meteor rate in Earth’s atmosphere 55P Dust trails near Earth orbit Simulated dust trails of 67P Churyumov-Gerasimenko
beyond Earth’s orbit (Vaubaillon, Christou, 2006) 45P near Venus In situ (Stardust, 2006) But… only observations of meteors in the atmosphere of the Earth currently provide us with a statistically significant set of data.
• Meteor counts in intervals per shower • Magnitude distributions per shower • Observing conditions: ◦ Limiting magnitude ◦ Field of view obstruction ◦ Number of cows Since 1982: • 2.2 million meteors • 5500 observers • 80 countries • Uniform observing method! Still outperforms video cameras for determining flux profiles.
Algorithm 1. Group data intervals into adaptive bins. Parameters: ◦ Optimum number of meteors (200) ◦ Minimum bin width (5 minutes) ◦ Maximum bin width (5 hours) 2. Estimate ZHR for each bin using weighted averaging:
relevance (Bruenjes, 2004) (Ryabova, 2006) Principal method for obtaining accurate photometry, astrometry and orbits. Coverage not good enough for fluxes (yet). Radiant structure (model)
aim point 100 km height Upper aim point 160 km height PC PC PC PC WinXP control machine DOS machine with MetRec DOS machine with MetRec DOS machine with MetRec Trigger for grabbing Internet, ESTEC ca. 140 km IAC network grating (Koschny, April)
The Canary Island Long-Baseline meteor Observatory (CILBO) is currently being implemented • First light before the end of 2008? • Expect >1000 meteoroid orbits per year, plus spectra for several 100s of meteors.
1. Meteor Science Why and how? 1. Meteor Science Why and how? 3. Virtual Observatories State-of-the-art databases in astronomy 3. Virtual Observatories State-of-the-art databases in astronomy 4. Virtual Meteor Observatory New advance in meteor science 4. Virtual Meteor Observatory New advance in meteor science Context Problem Inspiration Solution 2. Meteor data mining Meteors as a statistical science 2. Meteor data mining Meteors as a statistical science
problem • Great potential in cross-correlating radar-visual-camera observations and comparing results and models, but not practical ◦ Different data formats and units ◦ Codes in different languages ◦ Data quality not clear ◦ Limited online availability Text CSV XML FITS Excel dBase Access Binary … (Barentsen, 2008) Meteor Scientist C/C++ Fortran IDL Perl … We need a proper (active) data archive
& C Virtual Meteor Observatory System Components VMOTools Java VO Application s VO Application s Users Users Conversion & validation of existing archives Data archiving & analysis Web interfaces & services Drupal framework Apache HTTP Server PostgreSQL Database HTML VOTable VMOWeb PHP pgVMOMath pgVMOAstro pgVMOOrbit MetRecConverter MetRecValidator Component: Libraries: Task: SQL Call
Observatory VMO Virtual Meteor Observatory SQL Database Visual … VOTable Global Virtual Observatory Global Virtual Observatory Converter Tool XML MetRec Web Interface Internal Libraries Other Astronomers VOTable Other VO’s Quality check User Existing archives
Observatory: abstract example Archive A Archive A Processing A Processing A Archive B Archive B Archive C Archive C Data Retrieval Procedure A Data Retrieval Procedure B Processing B Processing B Science Science Shocks (X-ray) Dust (IR) e- (Radio) Example: Cassiopeia A Data Retrieval Procedure C Processing C Processing C Archive A Archive A Archive B Archive B Archive C Archive C Self-defining data standard Generic Processing Generic Processing Science Science Virtual Observatory = set of standards to query, retrieve and process data in a generic way. Standard Web-service Check units! e.g. http://esa.int/voquery?OBJECT=CasA
• International Virtual Observatory Alliance ◦ Standard data models and formats ◦ Standard data query and access protocols • SIA: Simple Image Access • SSP: Simple Spectral Access • Designed for astronomy, not planetary science ◦ Example: data access protocols take RA and DEC as input. ◦ Planetary science community needs to adapt standards • Planetary VO is part of EuroPlanet FP7 proposal. • VO for meteors is part of proposal. • Workshop will be held at ISSI (Bern) in November devoted to meteor science in the VO.
Virtual Meteor Observatory (VMO) makes meteor science data more easily accessible. • Basic functionality implemented, extensions and improvements to follow in later versions. • VMO 1.0 will be released on 20 september 2008 (International Meteor Conference). • Definition of Planetary VO ongoing, we aim to participate.