The Effect of Major Meteor Streams on the Total Ozone in the Earth’s Atmosphere

Gorbanev, Yu. M.; Stogneeva, I. A.; Shestopalov, V. A.; Knyazkova, E. F.; Kimakovskaya, I. I.; Kimakovsky, S. R.; Golubaev, A. V.

doi:10.18524/1810-4215.2017.30.114643

Cited by 2 publications

(2 citation statements)

References 22 publications

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“…The main parameter of single station meteor trajectory is the position of meteor's path big circle pole (Gorbanev & Golubaev, 2009). This parameter is used for further calculating of radiant point coordinates and heights (Astapovich, 1958).…”

Section: Single Station Observationmentioning

confidence: 99%

“…Meteor observation using video techniques was started at Research Institute «Mykolaiv astronomical observatory» (RI MAO) in 2011. This is the third big meteor research campaign in Ukraine after Odessa (Gorbanev, et al, 2006;Gorbanev, 2009) and Kiev (Hajdukova, et al, 1995;Kozak, 2001). The research is based on a system of fixed telescopes equipped with TV CCD cameras for both single and double station observation.…”

Section: Introductionmentioning

confidence: 99%

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Results of Positional and Photometric Measure- Ments of Meteor Trajectories Observed in Mykolaiv 2017-2018

Kulichenko

Shulga

Gorbanev

2019

OAP

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Regular meteor observation using TV CCD unintensified techniques was started in 2011 in RI «Mykolaiv astronomical observatory» (RI MAO). The method of meteor registration is based on using "trackand-stack" technique for obtaining frames with reference stars and online meteor detection software developed at RI NAO. The main accent of the research is made on precise astrometry and meteoroid orbits calculation. New observational campaign with baselines 11.7 and 100 km was started in 2017-2018 in collaboration with Astronomical Observatory of the I.I. Mechnikov Odessa National University. Eight telescopes with narrow field lens (f=50 mm, f/1.2) were installed in Mykolaiv and Odessa. More than 3000 single station meteors and 221 double station meteors were detected during 2017-2018. Uncertainties of meteor trajectory and orbital parameters are calculated using Monte Carlo method. Catalog of meteor trajectory positions and photometric parameters has created. Standard deviation of approximation of a meteoric trajectory in a large circle is (15-20)". Kinematic parameters of atmospheric meteoric trajectories and elements of heliocentric orbits for 3 meteors were calculated based on the results of television observations with cameras with a field of view <10° at a baseline distance 100 km. The average uncertainty of visible radiant estimation is in (0.3-0.7)º with baseline 100 km. The geocentric velocity estimation uncertainty is 0.5 km/s, elevation uncertainty is 50-150 m.

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Section: Single Station Observationmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

Results of Positional and Photometric Measure- Ments of Meteor Trajectories Observed in Mykolaiv 2017-2018

Kulichenko

Shulga

Gorbanev

2019

OAP

Self Cite

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Development of meteor astronomy at the Odessa University during the period of Ukraine's independence

Hrushytska

2019

Hist. sci. technol.

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The article using the methods of bibliographic and source study analysis and systems approach highlights the state and main trends in the development of meteor astronomy in Odessa during the time of independent Ukraine. At the beginning of the 21st century, continuous meteor patrol was restored at the Odessa Astronomical Observatory, which was intensively conducted at the Observatory during Soviet times. It was based on the use of the television and telescopic method, which was used in the CIS for the first time. The advantages of using the television telescopic method in comparison with the photographic and radar methods for solving the fundamental problems of meteor astronomy are noted. The text gives valuable information on the features of continuous meteor patrols at the observation station Kryzhanovka and the work of the expeditionary automatic meteor patrol on Snake Island (Odessa region, Ukraine). The methods of conducting telescopic television observations and processing observational material developed by Odessa researchers are considered. The main directions of meteoric studies conducted in the Odessa Astronomical Observatory using television meteor patrol materials were determined. Studying the physics of meteoric phenomena, obtaining exact coordinates of individual meteor radiant, spectral observations of meteors, studying double and multiple meteors, studying the structure and density of meteoric dust particles, solving interaction problems meteor showers with the Earth's atmosphere, statistics of meteor phenomena in the Earth's atmosphere are the main directions of meteoric studies of Odessa Astronomical Observatory. The scientific potential of Yu. M. Gorbanev in the field of meteor astronomy of, the leader of the meteoric group, O. V. Holubaieva, the head of the meteor's television patrol at the

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The Effect of Major Meteor Streams on the Total Ozone in the Earth’s Atmosphere

Cited by 2 publications

References 22 publications

Results of Positional and Photometric Measure- Ments of Meteor Trajectories Observed in Mykolaiv 2017-2018

Results of Positional and Photometric Measure- Ments of Meteor Trajectories Observed in Mykolaiv 2017-2018

Development of meteor astronomy at the Odessa University during the period of Ukraine's independence

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