Meteoroid orbital element distributions at 1 AU deduced from the Harvard Radio Meteor Project observations

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概要

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• The orbital element distributions of meteoroids detected during the Harvard Radio Meteor Project, 1968-69 Synoptic Year Program, have been reanalysed to remove selection effects associated with the radar observations. Corrections are made for the observing schedule, antenna beam patterns, the radio diffusion ceiling, speed dependence of ionization production, the flux enhancement due to the Earth's gravity and the probability of encounter with the Earth. These render the eccentricity, aphelion distance, and inclination distributions for meteoroids larger than 10<SUP>-4</SUP>g (radius -200 μm), with orbits that cross the ecliptic near 1 AU.

• 公益社団法人 日本地震学会、地球電磁気・地球惑星圏学会 、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会の論文

著者

• Taylor A.

  Durham School Durham

• Elford W.

  Department Of Physics And Mathematical Physics University Of Adelaide

関連論文

• Meteoroid orbital element distributions at 1 AU deduced from the Harvard Radio Meteor Project observations
• Meteoroid orbital element distributions at 1 AU deduced from the Harvard Radio Meteor Project observations

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