Custodian 发表于 2025-3-27 00:05:35
http://reply.papertrans.cn/15/1490/148907/148907_31.pngExpertise 发表于 2025-3-27 04:13:51
http://reply.papertrans.cn/15/1490/148907/148907_32.png群居动物 发表于 2025-3-27 06:19:41
http://reply.papertrans.cn/15/1490/148907/148907_33.pngTAP 发表于 2025-3-27 12:36:31
http://reply.papertrans.cn/15/1490/148907/148907_34.pngAtmosphere 发表于 2025-3-27 17:27:50
Fengzhou Liang,Fang Liu,Tongqing Zhouon: the orbital energy. The new function proved to be useful in the classification amongst the IAU2003 meteoroids which we searched for streams by .. function and also using .. and ..-function given by Valsecchi et al. For major streams, the results agree very well. For minor, and near-ecliptical streams the results sometimes differ markedly.镶嵌细工 发表于 2025-3-27 19:02:24
Hongyu Huang,Guijun Fan,Yantao Li,Nankun Muthe directional dependence of the activity and the velocity distribution of the sporadic meteoroid population on a two degree scale. These data can be used to investigate the origin of the sporadic meteoroid sources.Guileless 发表于 2025-3-28 01:14:15
http://reply.papertrans.cn/15/1490/148907/148907_37.pngCUB 发表于 2025-3-28 03:17:56
http://reply.papertrans.cn/15/1490/148907/148907_38.pngevanescent 发表于 2025-3-28 06:50:27
http://reply.papertrans.cn/15/1490/148907/148907_39.pngcrescendo 发表于 2025-3-28 12:45:47
Teng Huang,Huiqun Yu,Guisheng Fan We identified at least one of these clumps as particles trapped in the 7:1 mean motion resonance with Jupiter, potentially capable of producing meteor ourbursts of ZHR~ 1000 roughly once per century.