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The Surrender Software
Scientific image rendering for space scenes with the SurRender software Scientific image rendering for space scenes with the SurRender software R. Brochard, J. Lebreton*, C. Robin, K. Kanani, G. Jonniaux, A. Masson, N. Despré, A. Berjaoui Airbus Defence and Space, 31 rue des Cosmonautes, 31402 Toulouse Cedex, France [email protected] *Corresponding Author Abstract The autonomy of spacecrafts can advantageously be enhanced by vision-based navigation (VBN) techniques. Applications range from manoeuvers around Solar System objects and landing on planetary surfaces, to in -orbit servicing or space debris removal, and even ground imaging. The development and validation of VBN algorithms for space exploration missions relies on the availability of physically accurate relevant images. Yet archival data from past missions can rarely serve this purpose and acquiring new data is often costly. Airbus has developed the image rendering software SurRender, which addresses the specific challenges of realistic image simulation with high level of representativeness for space scenes. In this paper we introduce the software SurRender and how its unique capabilities have proved successful for a variety of applications. Images are rendered by raytracing, which implements the physical principles of geometrical light propagation. Images are rendered in physical units using a macroscopic instrument model and scene objects reflectance functions. It is specially optimized for space scenes, with huge distances between objects and scenes up to Solar System size. Raytracing conveniently tackles some important effects for VBN algorithms: image quality, eclipses, secondary illumination, subpixel limb imaging, etc. From a user standpoint, a simulation is easily setup using the available interfaces (MATLAB/Simulink, Python, and more) by specifying the position of the bodies (Sun, planets, satellites, …) over time, complex 3D shapes and material surface properties, before positioning the camera. -
Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
The Reference Mission of the NASA Mars Exploration Study Team
NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor Science Applications International Corporation Houston, Texas David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 This publication is available from the NASA Center for AeroSpace Information, 800 Elkridge Landing Road, Linthicum Heights, MD 21090-2934 (301) 621-0390. Foreword Mars has long beckoned to humankind interest in this fellow traveler of the solar from its travels high in the night sky. The system, adding impetus for exploration. ancients assumed this rust-red wanderer was Over the past several years studies the god of war and christened it with the have been conducted on various approaches name we still use today. to exploring Earth’s sister planet Mars. Much Early explorers armed with newly has been learned, and each study brings us invented telescopes discovered that this closer to realizing the goal of sending humans planet exhibited seasonal changes in color, to conduct science on the Red Planet and was subjected to dust storms that encircled explore its mysteries. The approach described the globe, and may have even had channels in this publication represents a culmination of that crisscrossed its surface. these efforts but should not be considered the final solution. It is our intent that this Recent explorers, using robotic document serve as a reference from which we surrogates to extend their reach, have can continuously compare and contrast other discovered that Mars is even more complex new innovative approaches to achieve our and fascinating—a planet peppered with long-term goal. -
Lighting Efficiency CLIMATE TECHBOOK
Lighting Efficiency CLIMATE TECHBOOK Quick Facts Lighting accounts for about 11 percent of energy use in residential buildings and 18 percent in commercial buildings. Both conserving lighting use and adopting more efficient technologies can yield substantial energy savings. Some of these technologies and practices have no up-front cost at all, and others pay for themselves over time in the form of lower utility bills. In addition to helping reduce energy use, and therefore greenhouse gas emissions, other benefits may include better reading and working conditions and reduced light pollution. New lighting technologies are many times more efficient than traditional technologies such as incandescent bulbs, and switching to newer technologies can result in substantial net energy use reduction, and associated reductions in greenhouse gas emissions. A 2008 study for the U.S. Department of Energy (DOE) revealed that using light emitting diodes (LEDs) for niche purposes in which it is currently feasible would save enough electricity to equal the output of 27 coal power plants. Background Nearly all of the greenhouse gas (GHG) emissions from the residential and commercial sectors can be attributed to energy use in buildings (see CLIMATE TECHBOOK: Residential and Commercial Sectors Overview). Embodied energy – which goes into the materials, transportation, and labor used to construct the building – makes up the next largest portion. Even so, existing technology and practices can be used to make both new and existing buildings significantly more efficient in their energy use, and can even be used in the design of net zero energy buildings—buildings that use design and efficiency measures to reduce energy needs dramatically and rely on renewable energy sources to meet remaining demand. -
A Physically-Based Night Sky Model Henrik Wann Jensen1 Fredo´ Durand2 Michael M
To appear in the SIGGRAPH conference proceedings A Physically-Based Night Sky Model Henrik Wann Jensen1 Fredo´ Durand2 Michael M. Stark3 Simon Premozeˇ 3 Julie Dorsey2 Peter Shirley3 1Stanford University 2Massachusetts Institute of Technology 3University of Utah Abstract 1 Introduction This paper presents a physically-based model of the night sky for In this paper, we present a physically-based model of the night sky realistic image synthesis. We model both the direct appearance for image synthesis, and demonstrate it in the context of a Monte of the night sky and the illumination coming from the Moon, the Carlo ray tracer. Our model includes the appearance and illumi- stars, the zodiacal light, and the atmosphere. To accurately predict nation of all significant sources of natural light in the night sky, the appearance of night scenes we use physically-based astronomi- except for rare or unpredictable phenomena such as aurora, comets, cal data, both for position and radiometry. The Moon is simulated and novas. as a geometric model illuminated by the Sun, using recently mea- The ability to render accurately the appearance of and illumi- sured elevation and albedo maps, as well as a specialized BRDF. nation from the night sky has a wide range of existing and poten- For visible stars, we include the position, magnitude, and temper- tial applications, including film, planetarium shows, drive and flight ature of the star, while for the Milky Way and other nebulae we simulators, and games. In addition, the night sky as a natural phe- use a processed photograph. Zodiacal light due to scattering in the nomenon of substantial visual interest is worthy of study simply for dust covering the solar system, galactic light, and airglow due to its intrinsic beauty. -
Lighting Journey
Your journey to a Lighting Career DESIGNED BY HURLBUT ACADEMY Creating Depth, Mood and Emotion with Lighting DIY Home Depot Lights Parts 1 & 2 Lighting Large Day Interiors, DIY Lighting, Essential Tools Lighting For Specific Camera Blocking LOCATION LIGHTING SET LIGHTING S C I S A B E Day Exteriors: Shaping and Day Interiors: How to Light an H Wide-shots and Controlling Interview with 4 T The Scout Walk-talks Light Leko Lights N R Day Exteriors: A Day Interiors: Shaping Light E Shaping Natural Night Interiors: L The Build Part 1 Light w/ Negative and Shadow The Build Fill Shaping light & Day Interiors: Day Exteriors: Shadow: Nailing Night Interiors: The Build Part 2 Shaping high sun for the Close-Up The Finesse close ups Lighting From Above: The Night Interiors: Day Interiors: Day Exteriors: Softbox The Shoot The Shoot Part 1 Lighting w/ available light Mounting The Softbox Day Interiors: The Shoot Part 2 Wall Spreader Etiquette Lighting techniques - Building the perfect key light Lighting for 3 cameras: Why & How TV Gag: Kino Flo Lights The Police Light Gag LOCATION LIGHTING SET LIGHTING Day Exteriors: On Set: Fathers How to Light Day Interiors: Changing the and Daughters - Green Screen The Scout direction of the sun Blocking and Series: Lighting for close-ups Lighting for Small your subject R Interiors E H Day Interiors: On-set: Into the How to Light T The Build Part 1 On Set: Fathers R Badlands Green Screen and Daughters - U Character Series: Lighting F Understanding Development with Just two Your Camera T through camera lights I Day -
Project Xpedition Is the Product of Purdue University‟S Aeronautical and Astronautical Engineering Department Senior Spacecraft Design Class in the Spring of 2009
92 Project Xpedition Purdue University AAE 450 Spacecraft Design Spring 2009 Contents 1 – FOREWORD ........................................................................................................................................... 5 2 – INTRODUCTION ................................................................................................................................... 7 2.1 – BACKGROUND .................................................................................................................................... 7 2.2 – WHAT‟S IN THIS REPORT? .................................................................................................................. 9 2.3 – ACKNOWLEDGEMENTS .....................................................................................................................10 2.4 – ACRONYM LIST .................................................................................................................................12 3 – PROJECT OVERVIEW ....................................................................................................................... 14 3.1 – DESIGN REQUIREMENTS ...................................................................................................................14 3.2 – INTERPRETATION OF DESIGN REQUIREMENTS ...................................................................................18 3.3 – DESIGN PROCESS ..............................................................................................................................19 3.4 – RISK -
The Moon and Eclipses
Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole. -
Introduction to Lighting - DIG Workshop 14 June 2019
Introduction to Lighting - DIG workshop 14 June 2019 Liana Bull & Robert King Turner Lighting is in many respects the most important aspect of photography, period. It’s essentially what our camera captures when we take a photograph, and it’s the manipulation of that light that ultimately determines what type of image is produced. There are infinite ways to use light in photography, each one creating a completely different result. Learning to understand and control how the light affects your images is arguably the single most important thing to improving your photography. Photography can be thought of as “painting with light.” The word photography is derived from Greek roots: “photos” meaning “light” and “graphe” meaning “drawing.” Without light, there would be no photography. Natural Light Photography, what does that even mean? Natural light photography is simply to record an image using the light that exists all around us. This can be direct sunlight, reflected sunlight or ambient sunlight Lighting is a key factor in creating a successful image. Lighting determines not only brightness and darkness, but also tone, mood and the atmosphere. Therefore it is necessary to control and manipulate light correctly in order to get the best texture, vibrancy of colour and luminosity on your subjects. Using Natural Light in Photography As a photographer, you get used to working with different kinds of lighting, including natural light, to produce high quality photos. Natural light can blend lightly within its environment to create a soft subtle light. Now, we aren’t always going to be so lucky and have ample light, the chance to pose a subject, or even have an option to be outdoors. -
Rgb Portrait Kit Usage Instructions ®®
RGB PORTRAIT KIT USAGE INSTRUCTIONS ®® LIGHT STANDS Unpack each light stand and loosen leg locks. Pull the upright section upwards while pushing the leg bracket down to extend the tripod legs. Tighten the knob on the leg bracket to secure the base. Loosen and extend each upright section to your desired height, then tighten to lock. Set the light on the top pin of the stand, and tighten the side knob of the light stand adapter to secure the light in place. AC POWER CORD Thread the included AC power cord into the AC receiver on the back of the light. Plug into nearby wall plug. Switch the “On/Off” button to the “On” position. The LED back z should illuminate. ATTACH AC POWER CORD OPEN LIGHT STANDS & MOUNT LIGHT HEAD SOFTBOX ATTACHMENT Unpack and open each softbox with care. Softboxes will open rapidly after tight packaging. OPEN & UNFOLD SOFTBOX Line up softbox opening with LED light head, and stretch and pull over the light head until it fits snugly over the light. STRETCH SOFTBOX OPENING OVER LIGHT HEAD Attach diffusion sheet to the front of the softbox by aligning the Velcro edges to the corners of the softbox, and press firmly to attach all edges. ATTACH FRONT DIFFUSER TO SOFTBOX VELCRO EDGES PROFESSIONAL PHOTOGRAPHY MADE SIMPLE 800.624.8891 SAVAGEUNIVERSAL.COM USAGE INSTRUCTIONS ®® RGB PORTRAIT KIT DISPLAY REAR PANEL CONTROL If the light is paired with the Savage Light Manager app, a blue light next to the Bluetooth BLUETOOTH INDICATOR RGB INDICATOR icon on the back panel will be illuminated. -
Applications of SAR Interferometry in Earth and Environmental Science Research
Sensors 2009, 9, 1876-1912; doi:10.3390/s90301876 OPEN ACCESS sensors ISSN 1424-8220 www.mdpi.com/journal/sensors Review Applications of SAR Interferometry in Earth and Environmental Science Research Xiaobing Zhou 1,*, Ni-Bin Chang 2 and Shusun Li 3 1 Department of Geophysical Engineering, Montana Tech of The University of Montana, Butte, MT 59701, USA; E-Mail: [email protected] (X.Z.) 2 Department of Civil, Environmental, and Construction Engineering, University of Central Florida, 4000 Central Florida Blvd.; Orlando, FL 32816, USA; E-Mail: [email protected] (N.B.C.) 3 Geophysical Institute, University of Alaska Fairbanks, 903 Koyukuk Drive, P.O. Box 757320, Fairbanks, AK 99775-7320, USA; E-Mail: [email protected] (S.L.) * Author to whom correspondence should be addressed; E-Mail: [email protected] (X.Z.); Tel.: +1-406-496-4350; Fax: +1-406-496-4704 Received: 23 September 2008; in revised version: 10 December 2008 / Accepted: 12 March 2009 / Published: 13 March 2009 Abstract: This paper provides a review of the progress in regard to the InSAR remote sensing technique and its applications in earth and environmental sciences, especially in the past decade. Basic principles, factors, limits, InSAR sensors, available software packages for the generation of InSAR interferograms were summarized to support future applications. Emphasis was placed on the applications of InSAR in seismology, volcanology, land subsidence/uplift, landslide, glaciology, hydrology, and forestry sciences. It ends with a discussion of future research directions. Keywords: InSAR, phase, interferogram, deformation, remote sensing. 1. InSAR Overview of InSAR 1.1. Introduction Interferometric synthetic aperture radar (InSAR) is a rapidly evolving remote sensing technology that directly measures the phase change between two phase measurements of the same ground pixel of Sensors 2009, 9 1877 the Earth’s surface. -
Digital Elevation Models of the Moon from Earth-Based Radar Interferometry Jean-Luc Margot, Donald B
1122 IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, VOL. 38, NO. 2, MARCH 2000 Digital Elevation Models of the Moon from Earth-Based Radar Interferometry Jean-Luc Margot, Donald B. Campbell, Raymond F. Jurgens, Member, IEEE, and Martin A. Slade Abstract—Three-dimensional (3-D) maps of the nearside and of stereoscopic coverage. More recently, the Clementine space- polar regions of the Moon can be obtained with an Earth-based craft [7] carried a light detection and ranging (lidar) instrument, radar interferometer. This paper describes the theoretical back- which was used as an altimeter [1]. The lidar returned valid ground, experimental setup, and processing techniques for a se- quence of observations performed with the Goldstone Solar System data for latitudes between 79 S and 81 N, with an along-track Radar in 1997. These data provide radar imagery and digital ele- spacing varying between a few km and a few tens of km. The vation models of the polar areas and other small regions at IHH across track spacing was roughly 2.7 in longitude or 80 km m spatial and SH m height resolutions. A geocoding procedure at the equator. Because the instrument was somewhat sensitive relying on the elevation measurements yields cartographically ac- to detector noise and to solar background radiation, multiple re- curate products that are free of geometric distortions such as fore- shortening. turns were recorded for each laser pulse. An iterative filtering procedure selected 72 548 altimetry points for which the radial Index Terms—Interferometry, moon, radar, topography. error is estimated at 130 m [1].