PPT-Optical depth from shadows in orbiter images of Mars

Nick Hoekzema Oliver Stenzel Lena Petrova Wojtek Markiewicz Maya GarciaComas Nick Thomas Klaus Gwinner Ai Inada Optical depth from shadows in orbiter images of Mars the optical depth . For real-time rendering. Crysis. 3 screenshot - . http://www.gamingcentrum.com/wpcontent/uploads/2012/04/crysis42412-2.jpg. Sean Lilley. Hard shadows. Basic ray traced shadows:. Shoot ray from eye. Ray hits a surface . NASA launched a multipurpose spacecraft named Mars Re - connaissance Orbiter on Aug. 12, 2005 to advance our under - standing of Mars through detailed observation, to examine po - its trajectory. The Exploring the Sun-. heliosphere. connection. Science questions. Mission overview. Status update. The Sun creates the heliosphere. Why study the Sun-space connection?. Addresses ESA’s Cosmic Vision question “How does the solar system work?”. PRESENTED BY,. RAMYA.K . M.TECH COS 1. st. yr. Contents . Mission objectives. Pre-launch updates. Spacecraft navigation. Payloads. Launch vehicle PSLV- C25. Facts on mars. Latest updates. Mission objectives. By: Kaleb Robertson. 8. . successfully landed . M. ars Rovers/Landers. May 1971:. . Mars . 3 successfully lands on mars but has a malfunction and loses connection seconds later.. Aug.–Sept. 1975: . February 24, 2015. Charles . Whetsel. , . Rich . Zurek. , . Rob Lock. Emerging Capabilities for the Next Mars Orbiter. Pre-Decisional: For planning and discussion purposes only. . Next Orbiter Can Support Many Potential Next Steps. Longwave. High. Clouds. Shortwave. High. Clouds. Shortwave. Low. Clouds. . . Δ. Optical Depth: -4 %. Δ Total Cloud Frac.: -0.50 %. . . Δ CTP: -8.30 hPa. . . Δ. Optical Depth: 2.0 % K. -1. and. . Curiosity. Rover. Metka Batič. Mars. Red planet – . iron. . oxide. Thin. . atmosphere. Large temperature . changes. No magnet . field. . – . radiation. 2 . Moons. : . Phobos. , . Deimos. CURRENT PLANS. Group 4 - Acacia Davis, Gregory Kim, Emily Mares, Jimmy Song. There are currently 8 missions operating on Mars with 3 officially planned for the future. . Groups involved include:. NASA. , Time & Cosmos. L. ecture 2. Solar . System . - . The . T. errestrial. (Inner) Planets. Prof. Ken Tsang. The Plane of the Ecliptic . is illustrated in this Clementine . star tracker . camera image which reveals (from right to left) the Moon lit by . Shading. [Figure from Prados & Faugeras 2006]. Focus/defocus. [figs from H. Jin and P. Favaro, 2002]. Images from same point of view, different camera parameters. 3d shape / depth estimates. Texture. Raytrace. shadows. Smooth Shading. Flat shading. Smooth Shading (. Gouraud. ). Vertex . normals. Soft edges. References. “How to show shadows in the Maya viewport”. . 2008. . http. ://www.wonderhowto.com/how-to/video/how-to-show-shadows-in-the-maya-viewport-197116. from the 1783-1784 Laki Eruption Luke Oman2,3 4,54,5 Department of Environmental Sciences, Rutgers University, New Brunswick, New Jersey 2Department of Geology and Geophysics, University of Hawaii, Stereo. Stereo. Multi-view analysis. Stereopsis. Finding correspondce. Depth. Reading: Chapter 12 and 11. Taken at the same time or sequential in time. stereo vision. structure from motion. optical flow.