Schult, Carsten; Stober, Gunter; Brown, Peter; Pokorný, Petr; Campbell-Brown, Margaret (2020). Characteristics of very faint (+16) meteors detected with the Middle Atmosphere ALOMAR Radar System (MAARSY). Icarus, 340, p. 113444. Elsevier 10.1016/j.icarus.2019.113444
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In September/October 2016 a dedicated specular meteor trail experiment with the high-power, large-aperture MAARSY radar was conducted, combining the high-power density of the radar with the large scattering target of trail echoes with the goal of probing the population of very small, slow-moving meteoroids. In contrast to meteor head echo observations, we find our raw velocity distribution peaks around 19 km/s for meteoroids with a limiting radar magnitude of +16. The correction for different observing biases to an equivalent limiting mass leads to a peak in the meteoroid influx at 13 km/s. Our calculated meteoroid masses range from 10⁻¹¹ to 10⁻⁷ kg. Using an ablation model we show that our detections are near the micrometeorite ablation limit at low speeds. A tentative comparison with a Jupiter Family Comets (JFC) dynamical meteoroid model shows an apparent excess of large, slow meteoroids not predicted by the model.
Item Type: |
Journal Article (Original Article) |
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Division/Institute: |
08 Faculty of Science > Institute of Applied Physics 10 Strategic Research Centers > Oeschger Centre for Climate Change Research (OCCR) 08 Faculty of Science > Institute of Applied Physics > Microwaves |
UniBE Contributor: |
Stober, Gunter |
Subjects: |
600 Technology > 620 Engineering 500 Science 500 Science > 530 Physics |
ISSN: |
0019-1035 |
Publisher: |
Elsevier |
Language: |
English |
Submitter: |
Simone Corry |
Date Deposited: |
08 Apr 2020 10:24 |
Last Modified: |
05 Dec 2022 15:37 |
Publisher DOI: |
10.1016/j.icarus.2019.113444 |
BORIS DOI: |
10.7892/boris.142557 |
URI: |
https://boris.unibe.ch/id/eprint/142557 |