Croatian Meteor Network Group Data reduction and analysis Students: Filip Trojko Lovro Vukadinović...
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Croatian Meteor Network Group
Data reduction and analysis
Students: Filip Trojko
Lovro Vukadinović
Sandi Šegota
Leonardo Pierobon
Team leaders: Filip Novoselnik Denis Vida
Višnjan school of astronomy 2011
Goals
• automatization of the station • visual IMO method observing• February Eta Draconids• meteor stream analysis• time synchronisation software• learning the data reduction procedure• making video tutorial
Višnjan school of astronomy 2011
Croatian Meteor Network
• first tests – 2006.; active work since 2007.• 35 cameras at the moment• data analysis and processing (known stream
analysis, discovering new streams and potential meteorites...)
Višnjan school of astronomy 2011
CMN data reduction
• object detection (MTP)• filtering (MTPFilter)• astrometry• photometry• orbits (UFOOrbit)
Višnjan school of astronomy 2011
IMO visual method• 14 perseids, 2 sporadic • night of maximum (2 hours)
Višnjan school of astronomy 2011
IMO report
Automatization of the stations
• Python 2.7.2.• automatic data reduction pipeline:
- deleting unnecessary images
- MTP
- uploading to the server• completely automatic station
Višnjan school of astronomy 2011
February Eta Draconids
• new meteor stream – CAMS (NASA)• checking CMN data in the period of activity (3rd
– 4th February)• the parent body: unknown long-period comet
(potentially dangerous!)• detected 1 potential FED (waiting for the
confirmation)
Višnjan school of astronomy 2011
Hb /km He /km vg /km/s λ /° e i /° ω /° Ω /°
105.1 94.6 35.67 314.929 0.970 55.39 194.42 314.923
105.1 96.3 35.16 314.925 0.972 54.94 193.73 314.990
102.7 97.0 35.90 315.115 0.970 55.54 194.41 315.111
103.9 97.1 35.30 315.135 0.971 54.74 194.17 315.132
103.1 95.7 35.87 315.175 0.972 55.37 193.73 315.175
101.4 93.4 35.62 315.229 0.971 55.90 194.09 315.228
CMN: 100,78 97,23 35,2 314,77 0,98 53,79 187,9 314,77
CAMS:
Višnjan school of astronomy 2011
Ground map
Kappa Cygnids (KCG)
• radiant in Cygnus• ZHR: 3• active in the period from 3rd to 25th August• velocity: 25 km/s
Višnjan school of astronomy 2011
Alpha Capricornids (CAP)
• radiant in Capricornus• ZHR: 2-3• maximum activity 29th to 30th of July• velocity: 25 km/s; slow, but very bright
Višnjan school of astronomy 2011
Poynting – Robertson effect
• radiation pressure• energy ~ frequency• Doppler effect• deceleration of the small
particles• spiral falling of the small
particles on the Sun
Višnjan school of astronomy 2011
Time synchronisation
• Python 2.7.2.• extracting the station name from its code• copying the *.hmm files• calculating average time difference• time difference filtering• extrapolation
Višnjan school of astronomy 2011
The video tutorial
• Camtasia 7• data reduction procedure explained• for new members
Višnjan school of astronomy 2011
Future plans
• time synchronisation (2008 – 2009)• continuing the data analysis• education of new members
Višnjan school of astronomy 2011
Thank you for your attention!
Questions?
Filip Novoselnik: [email protected]
Denis Vida:[email protected]
Filip Trojko: [email protected] Vukadinović:[email protected] Šegota:[email protected] Pierobon:[email protected]
Višnjan school of astronomy 2011