... of the Interplanetary Dust Distribution on the Ecliptic Plane and b) Study of the ... the uniformity of the interplanetary dust distribution on the ecliptic plane ... expected from modeling if the dust distribution is uniform along the ecliptic plane ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/JanchestagT2315tp.pdf -- 51.2 Кб -- 09.02.2007 Похожие документы
... of the Interplanetary Dust Distribution on the Ecliptic Plane and b) Study of the ... the uniformity of the interplanetary dust distribution on the ecliptic plane ... expected from modeling if the dust distribution is uniform along the ecliptic plane ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/JanchestagT2315tp.ps -- 93.6 Кб -- 09.02.2007 Похожие документы
... Construction contract signed. Telescope has limited steerability and thus needs to be close to equator to see ecliptic. Spherical reflector optics. ...
... An on-going micrometeor observing proposal (T1565) using the dual-beam capabilities have shown a qualitative di erence in the micrometeor radial topocentric velocity distribution when looking in three di erent ecliptic latitudes. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/JanchestagT1748tp.ps -- 97.9 Кб -- 19.04.2004 Похожие документы
... From the radar echo bandwidths, we determine the mean radius to be 64 ТБ 4 meters with a retrograde pole at ecliptic longitude and latitude (173, -81) with an uncertainty in latitude of ТБ 8 degrees and an obliquity of 169 degrees. ...
... Finally, close proximity to the plane of the ecliptic (dashed) allows Pleiads to be studied via lunar occultation, but unfortunately also complicates observation of the cluster in mid-infrared bands by maximizing background emission from solar zodiacal ...
... we: 1. rotate from mean equatorial system of date to ecliptic system about x axis (mean equinox). 2. rotate about eclipitic ... When going back from true ecliptic to true equatorial, use eps (avg obliquity) + deleps (obliquity due to nutation). ...
... While many particles with a/e combinations along the drag lines are seen farthest (north) from the ecliptic plane, eccentricities approach the parabolic limit of unity for those closest to the ecliptic plane. ...