期刊文献+

基于Shape-from-Shading的月球表面三维形状恢复算法研究 被引量:2

Research on 3-D Reconstruction Algorithm of the Moon Surface Based on Shape-from-shading Method
下载PDF
导出
摘要 提出了一种基于Shape-from-Shading的月球表面三维形状恢复算法。首先分析了在太阳光照射下月球表面成像模型,建立了使用Lommel-Seeliger反射模型描述的反射图方程。然后用有限差分近似微分运算,将反射图方程所示的一阶变系数线性偏微分方程进行离散化处理,得到关于表面高度函数的代数方程。进而采用超松弛迭代法进行求解,获得月球表面三维高度函数值。最后使用合成图像和实际月球图像进行三维形状恢复仿真实验。实验结果表明提出的算法可以有效地恢复月球表面三维形状。 An algorithm of 3-D shape reconstruction of the Moon surface based on shape-from-shading method was proposed. Imaging model of the Moon surface under the illumination of the sun was discussed firstly. And Lommel-Seeliger reflectance model was used to establish reflectance map equation. When the finite difference approximated differential operator, the reflectance map equation described by the first order yawing-coefficient linear partial differential equation turned into a group of algebraic equations about the unknown surface height functions. Then SOR iterative method was used to solve the equations and heights of 3-D surface were achiered. At last, 3-D shape reconstruction experiments on synthetic image and real image of the Moon were performed to il- luminate the efficiency of the proposed method.
出处 《宇航学报》 EI CAS CSCD 北大核心 2008年第6期1995-2000,共6页 Journal of Astronautics
基金 国家自然科学基金(60502021) 教育部高等学校博士点专项科研基金(20050698025)
关键词 月球表面 三维形状恢复 Shape-from—Shading Lommel—Seeliger反射模型 有限差分 The Moon surface 3- D reconstruction Shape-from- Shading Lommel- seeliger reflectance model Finite difference
  • 相关文献

参考文献15

  • 1欧阳自远.我国月球探测的总体科学目标与发展战略[J].地球科学进展,2004,19(3):351-358. 被引量:177
  • 2Williams D R, Grayzeck E J. The lunar data project-restoration of apollo data for future lunar exploration[J]. Lunar and Planetary Science, 2006, 37: 1187- 1224.
  • 3Oberst J, Wahlisch M, Zhang W. New data on lunar topography derived from galileo and Clementine stereo images[J]. Lunar and Planetary Science, 1996,27 : 973 - 974.
  • 4Gordon C, Scott B, Marc F, et al. Lunar reconnaissance orbiter overview: the instrument suite and mission[ J]. Space Science Review, 2007, 129(4) : 391 - 419.
  • 5Diggeten V J. A photometric investigation of the slopes and heights of the ranges of hills in the Maria of the Moon[J]. Bull. Astron. Inst. Netherlands, 1951,11(423) : 283 - 289.
  • 6Link F. Photometry of the lunar surface[J]. The Moon, 1972, 5: 265 - 285.
  • 7Horn B K P. Height and gradient from shading [ J]. International Journal of Computer Vision, 1990, 5( 1 ) : 37 - 75.
  • 8Wohler C. Shape from shading under coplanar light sources[ C ]//Rasmussen C E, Bulthoff H H, Giese M A, Scholkopf B (Eds.). Proceedings of the 26th DAGM Symposium. Tubingen. Springer, 2004 : 278 - 285.
  • 9Christian W, Raffaello L, Paolo L, et al. A combined speetrophotometric and morphometric study of the lunar mare dome fields near Cauehy, Arago, Hortensius, and Milichius[J]. Icarus, 2006, 183 (2) : 237 - 264.
  • 10Volker L, Christian H, Randolph L K. Derivation of planetary topography using multi-image shape-from-shading[J]. Planetary and Space Science, 2006, 54(7): 661- 674.

二级参考文献26

  • 1Grant Heiken, David Vaniman, Bevan M French.Lunar Sourcebook-A User's Guide to the Moon[M].Cambrdage: Cambridge University Press, 1991.121-474.
  • 2Lawrence D J, Feldman W C, Barraclough B L, et al. Global elemental maps of the Moon: The lunar prospector gamma-ray spectormater[J]. Science, 1998, 281(4): 1 984-1 988.
  • 3Paul G Lucey, Blewett D T. Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images[J]. Journal of Geophysical Research, 2000, 105(8): 20 297-20 305.
  • 4Paul G Lucey, Blewett D T, Hawke B R. Mapping the FeO and TiO2 content of the lunar surface with multispectral imagery[J]. Journal of Geophysical Research, 1998, 103:3 679-3 699.
  • 5Elphic R C, Lawrence D J, Feldman W C, et al. Lunar Fe and Ti abundance: Comparison of Lunar Prospector data[J]. Science, 1998,281(4): 1 993-1 996.
  • 6Lawrence D J, Feldman W C, Barraclough B L, et al. Thorium abundances on the lunar surface[J]. Journal of Geophysical Research, 2000, 105(8): 20 307-20 331.
  • 7Larry A. Haskin Gillis Seffrey J, Korotev Randy L, et al. The materials of the Lunar Procellaru-KREEP Terrane: A synthesis of data from geomorphological mapping, remote sensing, and sample analyses[J]. Journal of Geophysical Research, 2000,105(8): 20 403-
  • 8Mark A Wieczorek, Roger J Phillips. The ''Procellarum KREEP Terrane'': Implications for mare volcanism and lunar evolution[C]. Journal of Geophysical Research, 2000,105(8): 20 417- 20 430.
  • 9Head J W, Wilson L. Lunar mare volcanism: Stratigraphy, ruption conditions, and the evolution of secondary crusts[J]. Geochimia et Cosmochimica Acta, 1992,56:2 155-2 175.
  • 10中国科学院地球化学研究所编.月质学研究进展[M].北京: 科学出版社,1977.41-203.

共引文献181

同被引文献16

  • 1介鸣,尹航,黄显林.月球探测器自主软着陆中的三维重构技术研究[J].宇航学报,2007,28(4):966-971. 被引量:7
  • 2Horn B K P. Height and gradient from shading [ J]. International Journal of Computer Vision, 1990, 5(1) : 37 - 75.
  • 3Wohler C. Shape from shading under coplanar light sources [ C ] Rasmussen C E, Bulthoff H H, Giese M A, Scholkopf B (Eds.) Proceedings of the 26th DAGM symposium. Tubingen. Springer 2004 : 278 - 285.
  • 4Volker L, Christian H, Randolph L K. Derivation of planetary topography using multi-image shape-from shading[J]. Planetary and Space Science, 2006, 54(7): 661- 674.
  • 5Christian W, Raffaello L, Paolo L, et al. A combined spectrophotometric and morphometric study of the lunar mare dome fields near Canchy, Arago, Hortensius, and Milichius[J]. Icarus, 2006, 183 (2) : 237 - 264.
  • 6McEwen A S. A precise lunar photometric function[J]. Lunar and Planetary Science, 1996, 27: 841- 842.
  • 7Kreslavsky M A, Shkuratov Yu G, Velikodsky Yu I, et al. Photometric properties of the lunar surface derived from Clementine observations[J]. Journal of Geophysical Research, 2000, 105(E8): 20281 - 20295.
  • 8Zhang R, Tsai P S, Cryer J E, et al. Shape from shading: a survey [J]. IEEE Transactions on Pattern Analysis and Machine Intelligence, 1999, 21(8): 690-706.
  • 9Kao C Y, Osher S, Qian J. Lax-Friedrichs sweeping scheme for static Hamilton-Jacobi equations[J]. Journal of Computational Physics, 2004, 196: 367-391.
  • 10Prados E, Faugeras O. Shape from shading: a well-posed problem? [C]. Proceedings of the IEEE Conference on Computer Vision and Pattern Recognition. San Diego, CA, USA: IEEE Computer Society, 2005 : 870 - 877.

引证文献2

二级引证文献6

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部