VIAGGIO IN POLONIA. Podróż do Polski. INNO NAZIONALE POLACCO. VIAGGIO IN POLONIA. CRACOVIA ZAKOPANE MINIERE DI SALE AUSCHWITZ SOSNOWIEC ACQUA PARK LAVORO DI…. Fiume Vistola. Cattedrale. Piazza. Cracovia.
By ayalaWhitewater Canoe Trip Batiscan River, Quebec. 1 st Merrickville Venturer Scouts July 1-8, 2010. Adults Venturers Stew Hamill Ben Catton Allan Yates Calvin Gale Jennifer Gale Gregory Jackman Alex McKay Adam Szalai Max Taylor. www.1stmerrickville.ca. v1. River Location. Itinerary
By xerxesMAXDOAS horizontal (averaging) effects MPI for Chemistry (MPIC), Mainz, Germany T. Wagner, J. Remmers, S. Beirle. 4-azimuth MAX -DOAS measurements in Mainz Characterisation of the information content using 3D RTM. Master Thesis, Julia Remmers. Comparison of the Telescopes (5°)
By weldonAdjoint modeling of the coupled ocean/sea-ice state P. Heimbach 1 , D. Menemenlis 2 , M. Losch 3 , I. Fenty 1 , J.M. Campin 1 , C. Hill 1 , A. Nguyen 2 (1) MIT/EAPS, Cambridge, MA, USA (2) JPL/CalTech, CA, USA (3) AWI, Bremerhaven, Germany. http://www.ecco-group.org http://mitgcm.org.
By nevinThe OPERA Anomaly - a Quick Summary with Comments. Physics 841, Fall 2011 Prof. Brian Meadows. OPERA Experiment (Gran Sasso, Italy). Purpose: Look for “appearance” of ¿ leptons from a º ¹ “beam” from CERN (SPS) 730 km away. At CERN ¼ ( K ) mesons decay ¼ § ( K § ) ¹ § º ¹
By leviThis lecture will help you understand:. Motion Is ______________ Speed : __________and ____________ Velocity ______________ Free Fall. Motion Is Relative. Motion of objects is always described as ______ to something else. For example:.
By debbieMOTION An object is in motion if its position changes. The mathematical description of motion is called kinematics. The simplest kind of motion an object can experience is uniform motion in a straight line. The object experiences translational motion if it is moving without rotating.
By dorisDevelopment of Telescopes for Extremely Energetic Neutrinos. ~1 km. Steven W. Barwick, UC-Irvine. Neutrino Telescopes: Agenda. 10 years of progress with optical Cherenkov Detectors Extremely Energetic Neutrinos - New Technologies Radio Cherenkov: ARIANNA. Teraton -Petaton.
By bowieExamining Buoyancy Waves in the Martian Atmosphere with Mars Climate Sounder Robert M. Edmonds, J.R. Murphy, D.A. Teal New Mexico State University, Department of Astronomy. Introduction. Analysis Cont. MCS Results.
By faithObjective Evaluation of the Meso-NH Simulations during Hibiscus-Troccinox-Troccibras. Forecasts for the TROCCINOX campaign Three case studies: 13 Feb, 24 Feb, 3 March. J.-P Chaboureau, J.-P. Cammas, J. Duron, F. Gheusi, C. Mari, P. J. Mascart, J.-P. Pinty
By jovan,, XIX century was the age of empires , XX century – the age of states , XXI century becomes the age of cities” Wellington E. Webb, Mayor of Denver. 1. VILNIUS : FACTS & FIGURES. ≈30 km. ≈50 km. 16 m illion inhabitants in a 300 km radius Vilnius population 5 27 930
By randiLocal and regional distance earthquakes (0° - 15°). 1. Introduction 2. Data examples 3. Exercises. Snells‘ Law for refracted waves: Sin i 1 /v p1 = sin i 2 /v p2 Critical angle (for P n waves): i 2 = 90° sin i crit = v 1 /v 2 i crit = 48° for v 1 = 6 km/s and v 2 = 8 km/s
By shelAirborne Measurements of the Columbia River Plume Andy Jessup and Bill Plant APL-UW. Determine Plume Location/Characteristics SST Water Type/Sediment Load Waves (dir. spectra), roughness features Identify features of interest (fronts, IW). Airborne Sensors. Infrared Surface Temperature
By gilonMagmatic fluxes. 508_2k13_lec17. Fluxes. Rates of magmatism (vol/time or similar) to be compared to rates of other tectonics processes; Can be applied to rates of everything geologic. Isotope -time relationships, but how relevant are the samples outlined in red?. Techniques.
By terylApplications National Institute for Computational Sciences (NICS): NSF and ORNL 2011 Model Problems. Ricky A. Kendall Scientific Computing and Workflows National Institute for Computational Sciences. Enabling Transformational Science. WRF Climate.
By gashaThe structure and kinematic of gas in the center of recent star-formation burst in the Irr Galaxy IC10. Egorov O.V. 1 , Lozinskaya T.A. 1 , Moiseev A.V. 2 1 Sternberg Astronomical Institute, Moscow, Russia
By deronContribution to: 8th Annual CMAS Conference Friday Center, UNC-Chapel Hill OCTOBER, 19-21, 2009, Friday Center for Continuing Education, 100 Friday Center Dr Chapel Hill, NC 27517, United States. Simulations with MM5-CMAQ and WRF/CHEM models of a
By chavezEarthquake Information. Summary:. Credit EMSC. Page created by W. G. Huang. Earthquake Information. Summary:. Credit EMSC. Page created by W. G. Huang. Earthquake Information. 201103090245 UTC Mw=7.2 D=9 km. 201103110546 UTC Mw=8.8 D=30 km. 2500 km. Taiwan.
By kuengLinking land cover change to pressures on biodiversity. http://www.creaf.uab.es/biopress/. Question: How have past changes in land cover affected Biodiversity ? Why: Legislative imperative to protect the environment. EEA is our key stakeholder How: Measuring land cover change by
By mindaECE 1100: Introduction to Electrical and Computer Engineering. Spring 2011. Wanda Wosik Associate Professor, ECE Dept. Notes 10. Antennas Transmission and Reception of waves. Slides developed by Dr. Jackson. Antenna. An antenna is used to transmit or receive an electromagnetic signal.
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