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2016 | 6 | 1 | 78-89

Article title

Visual Observations as Exercises in Physics

Title variants

Languages of publication

EN

Abstracts

EN
Visual meteor observations are a fun and interesting approach to astronomy and to scientific research in general. It can be used for laboratory or practical exercises in physics at high schools and universities. The students can personally collect and analyze the acquired data. The output consists of Zenithal Hourly Rate (ZHR) values, spatial density and population index. In this paper, the so called counting method is described as it is the most suitable method for beginners. As a practical example, the ZHR curve of the Lyrid meteor shower was evaluated and the maximum and the duration of the shower were calculated.

Publisher

Year

Volume

6

Issue

1

Pages

78-89

Physical description

Dates

published
2016-06-01
online
2016-05-28

Contributors

author
  • Alexander Dubček University of Trenčín, Trenčín, Slovakia
author
  • Faculty of Mathematics, Physics and Informatics, Comenius University in Bratislava, Bratislava, Slovakia
author
  • Observatory and Planetarium in Hlohovec, Hlohovec, Slovakia
  • Faculty of Education, University of Prešov, Prešov, Slovakia
  • High School of Piarists, Trenčín, Slovakia

References

  • Drga, J., & Bulko, M. (2014). Determination of average maximum of Orionids meteor shower from visual observations. University review, 8(3-4), 104-107.
  • Drga, J., & Janek, M. (2014). Determination of the maximum of the Geminid meteor shower from visual observations. WGN Journal of the International Meteor Organization, 42(3), 125-126.
  • IMO. (2013a). Determination of the limiting magnitude. Retrieved from
  • IMO. (2013b). Electronic visual report form. Retrieved from
  • Koschack, R., & Rendtel, J. (1988). Number density in meteor streams. WGN - Journal of the IMO, 16(5), 149-157.
  • Koschack, R., & Rendtel, J. (1990a). Determination of spatial number density and mass index from visual meteor observations (I). WGN - Journal of the IMO, 18(2), 44-58.
  • Koschack, R., & Rendtel, J. (1990b). Determination of spatial number density and mass index from visual meteor observations (II). WGN - Journal of the IMO, 18(4), 119-140.
  • McBeth, A. (2014). IMO meteor shower calendar 2014.
  • Meteor showers: IAU 3-letter codes (2014). Retrieved from
  • Molina, A., & Moreno, F. (2013). Lyrids and perseids meteoroids: reconciliation and discrepancy between cometary outgassing theory and electrophonic sound data. The astronomical journal, 145(4), 4.
  • Porubcan, V., Hajduk, A., Cevolani, G., & Trivellone, G. (1996). Lyrid meteor shower observed by a forward scatter meteor radar, Contributions of the astronomical observatory Skalnate Pleso, 26, 5-9.
  • Porubcan, V., & Simek, M. (1988). Distribution of Lyrid meteoroids in a large range of echo durations. Bulletin of Astronomical institutes of Czechoslovakia, 39, 165-168.
  • Van Wassenhove, J. (1987). Belgian and Danish radio observations in April 1987. WGN Journal of the International Meteor Organization, 16(4), 123-126.

Document Type

Publication order reference

Identifiers

YADDA identifier

bwmeta1.element.doi-10_1515_atd-2016-0002
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