1 / 21

Meteors

Meteors. Members: Ahn Soo Young Jee Myeong Keun Diego Širola Slaven Mišak Team leader: Nikola Strah. Scientific advisors: Goran Zgrablić Izidor Pelajić Nikola Biliškov. Goals. Background. Meteors: -small particles of dust -up to 50m in diameter

zoie
Download Presentation

Meteors

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Meteors Members: Ahn Soo Young Jee Myeong Keun Diego Širola Slaven Mišak Team leader: Nikola Strah Scientific advisors: Goran Zgrablić Izidor Pelajić Nikola Biliškov

  2. Goals

  3. Background Meteors: -small particles of dust -up to 50m in diameter -circle the Sun – meteor streams

  4. Radio observation Goal: -detect a signal from a station far far away (more than 800 km) (forward scattering) -record the signal through the night -analyze the recorded data Ionization trail TV station Prague Meteor Group Lab

  5. Equipment - Yagi antenna - iCom IC-PCR1000 receiver - Computer and Humanware

  6. Details • iCom IC-PCR1000 receiver • Frequency 49.7396 MHz TV station in Prague, output power 150 kW, distance 544 km, video and audio signal recorded • PC computer Pentium 3 • Data recording, reduction and analysis performed with CoolEdit & Audacity software, sampling rate 11087 Hz Digging the hole for the antenna Yagi antenna in the dark

  7. Results • 13h of raw data to be processed • 10 minutes of actual meteor recordings

  8. Visual observation Plan: -gather few hours of observations -send report to IMO -calculate ZHR

  9. Results - Few hours of observation - Reports sent to IMO - ZHR calculated for all observations - Observed showers: - Perseides - Southern δ Aquarides - κ Cygnides ZHR:-κ Cygnides- 1.day 3 2.day 40 3.day 41

  10. ELF • Goals: • Record a meteor signal in ELF band (0- 300 Hz)

  11. Equipment • ELF orb • 50 Hz filter • DC filter • NI DAQmx SCB-68 and appropriate software

  12. Schematics NI DAQmx SCB-68 PC with acquisition software made in LabView 7.1 50 Hz cutoff 150 Hz cutoff Low pass DC Filter Electrometer

  13. Results • equipment testing Signal from the electrometer Signal from the electrometer when electrometer was grounded

  14. - We used Slaven for grounding purposes With the grounding Without the grounding

  15. Signal recorded

  16. FFT calculated using LabView programmed software and CoolEdit Frequency Analysis

  17. Video • Goal: • Simultaniousley record the sky with video camera combined with radio & visual observation for analisys.

  18. Equipment • Watec WAT-902H CCD camera • DC power supply- founded and thoroughly tested • Video capture card • MetRec and Meteoder software

  19. Results - Video capture card (Meteor II) doesn’t work - Camera works - DC power supply is operating “First light” from camera- tested on video monitor from the control room of the observatory

  20. THE END Thank you for your attention!Any questions?

More Related