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    81. http://star.arm.ac.uk/preprints/384.pdf
    ... Seen in projection, the disc is concentrated within a rather narrow range of ecliptic latitude (halfwidth 1/2 3 ­5 ), but closer analysis of the inclination distribution provides evidence for a surprisingly high level of dynamical excitation ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/384.pdf -- 2025.0 Кб -- 07.01.2003
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    82. Research Reports
    ... In favourable conditions this cloud can be seen from the Earth as the zodiacal light, lying along the ecliptic plane. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2000/node19.html -- 67.6 Кб -- 30.07.2001
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    83. http://star.arm.ac.uk/preprints/411.ps
    ... The appropriate weights can be derived as follows. TNO surveys target the ecliptic. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/411.ps -- 769.3 Кб -- 15.01.2004
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    84. http://star.arm.ac.uk/nibulletin/2011/Oct03.html
    ... Pedro has givenѓЉexcellent lectures to the IAA]ѓЉThe discovery that the spinning object is tilted at nearly 90 degrees to the ecliptic plane is surprising, and suggests that this type of object could be very common in the Kuiper Belt. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2011/Oct03.html -- 21.0 Кб -- 03.10.2011
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    85. http://star.arm.ac.uk/~ambn/iris.ps
    ... determination is by Magnusson (1986), who finds an ellipsoidal shape with a=b = 1:18 and b=c = 1:41 and a pole direction with ecliptic longitude and latitude (–; fi) of either (15 \Sigma 5 ffi ; +25 \Sigma 15 ffi ) or (195 \Sigma 5 ffi ; +15 \Sigma 15 ffi ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/iris.ps -- 128.8 Кб -- 04.11.1996
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    86. http://star.arm.ac.uk/~ambn/268csj.ps
    ... The solution may also explain the Faint Young Sun paradox and the inclina­ tion of the solar equator relative to the ecliptic. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/268csj.ps -- 88.3 Кб -- 15.04.1997
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    87. http://star.arm.ac.uk/~ambn/pcuvflare.dvi-ps
    ... Its low orbit means that, for objects at low ecliptic latitude, the Earth occults many targets for up to half the observing time. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/pcuvflare.dvi-ps -- 318.1 Кб -- 31.05.1996
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    88. http://star.arm.ac.uk/nibulletin/2013/Dec03.html
    ... Venus isТљstill nearТљmaximum elongation from the Sun, but it'sТљonly now becoming fairlyТљeasy to see from our latitudes, becauseТљthe ecliptic lies at a very shallow angle to the W horizon in autumn evenings.Тљ It's slowly getting higher in the evening ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2013/Dec03.html -- 34.0 Кб -- 03.12.2013
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    89. http://star.arm.ac.uk/~meb/bailey_etal_1999_leonids_MNRAS.pdf
    ... with the Earth in 1998 during their descending nodal passage at heliocentric distance rD , it is necessary that they (i) cross the ecliptic at the same heliocentric distance as the Earth; (ii) have orbits such that the longitude Q of their ascending node ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~meb/bailey_etal_1999_leonids_MNRAS.pdf -- 202.2 Кб -- 06.10.2011
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    90. http://star.arm.ac.uk/~meb/ras_leaflets2012/Moon.2012.pdf
    ... However, it is then difficult to explain why the orbit of the Moon is inclined at 5° to that of the Earth (ecliptic). ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~meb/ras_leaflets2012/Moon.2012.pdf -- 389.0 Кб -- 05.03.2012
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