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 . Robert . Louisell. , St. Ambrose University. Francis . Kazemek. , St. Cloud State University. Jennifer Wilhelm, University of Kentucky. What is a shadow?. For example, we ask “What is a shadow?”, seeking a . 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?”. CSE . 274 [. Fall. . 2015]. , Lecture . 3. Shadow and Environment Mapping . http://. www.cs.ucsd.edu. /~. ravir. To Do. By . next Thu. , . e-mail me . brief project description (can be done in groups of 2). Time to discuss next week. the. C . omposition. of. E . nceladus. via. Alex Gonring, Capri Pearson, . Sam Robinson, Jake Rohrig, . & Tyler Van Fossen. University of Wisconsin - Madison. P . rimary. L . ander. and. U . nderwater. 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. Heliosphere= . the . region of space, encompassing the solar system, in which the solar wind has a significant influence.. .  . corona. = is . an aura of plasma that surrounds the sun and other celestial bodies. Typical cold sea surface temperatures, in conjunction with the subsidence associated with the subtropical high, are responsible for the formation of a shallow cool moist marine boundary layer capped by a strong inversion. Marine stratus clouds form in this marine boundary layer. . 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. Mars, also known as the red planet, is the 4. th. planet from the sun. It has the largest volcano in the solar system and has some very large impact craters.. Appearance. The planet mars is made from rock. The ground there is red because of the iron oxide in the rocks and dust. The planets atmosphere is very thin and contains heaps of carbon dioxide (also known as co2). Did you know, mars’ first ever name was Ares, named after the Ancient . of. E . nceladus. via. Alex Gonring, Capri Pearson, . Sam Robinson, Jake Rohrig, . & Tyler Van Fossen. University of Wisconsin - Madison. P . rimary. L . ander. and. U . nderwater. M . icroorganism. Brent Sherwood. brent.sherwood@jpl.nasa.gov. . GLEX, May 2012. The Space Show, July 24, 2012. FISO, August 1, 2012. HSF ≠ Exploration. GLEX – May 2012. Mars: On the Path or In the Way?. Sherwood . ESA and NASA are discussing the potential benefits of contributions by NASA to ESA's Solar Orbiter mission, planned for launch in 2015. Although negotiations between the Agencies continue at this tim cool surface features. Lets look at some!. (all images credit: Mike . Sussman. ). The famous “Face on Mars”. Now don’t get all excited…. How Come We Missed These?. Look harder!. The Panda!. George Washington Screaming!.