'Ray image' presentation slideshows

Remote Sensing

Remote Sensing. 29. Remote sensing Content 29.1 Production and use of X-rays 29.2 Production and use of ultrasound 29.3 Use of magnetic resonance as an imaging technique Learning outcomes Candidates should be able to: (a) explain in simple terms the need for remote sensing (non-invasive

1.5k views • 85 slides

Discovering the Universe Ninth Edition

1.12k views • 68 slides

Universe Eighth Edition

687 views • 55 slides

RF Propagation Resources and Beacons

936 views • 46 slides

Medical Vocabulary by Diana Curtis

732 views • 46 slides

Clusters of Galaxies (and some Cosmology) Scientific and Data Analysis Issues

Clusters of Galaxies (and some Cosmology) Scientific and Data Analysis Issues. Keith Arnaud NASA Goddard University of Maryland. Structure in the Universe. Fluctuations in density are created early in the Universe.

457 views • 45 slides

Calculate the net force acting on a particle

Mass transfer in a binary system. Calculate the net force acting on a particle . Gravitational potential in the corotating frame. Mass Transfer in Binary Stars. In a binary system, each star controls a finite region of space, bounded by the Roche Lobes (or Roche surfaces ).

571 views • 43 slides

SEISMOLOGY OF STELLAR ATMOSPHERES

SEISMOLOGY OF STELLAR ATMOSPHERES. Zdzislaw Musielak Physics Department University of Texas at Arlington (UTA). OUTLINE. Stellar Activity in the H-R Diagram Stellar Activity and Exoplanets Atmospheric Oscillations Models and Theoretical Predictions Atmospheric Seismology.

583 views • 42 slides

Guiding Questions

602 views • 40 slides

Optimizing Patient Radiation Dose

Optimizing Patient Radiation Dose. John Aldrich PhD FCCPM Department of Radiology Vancouver Coastal Health University of British Columbia. Outline. Changes in Medical Imaging Dose, Effective Dose and Risk Medical Imaging Utilization Status of Patient Dose in BC Skin Doses Summary.

741 views • 39 slides

Radiation

Radiation. Electromagnetic Radiation. X-rays. William Roentgen German Physicist - 1895. Was working with cathode ray tubes when he noticed that a phosphorescent material in his lab was glowing several meters away.

640 views • 37 slides

Module 8: High Energy Astrophysics

703 views • 36 slides

ICA FOUNDATION International Contraceptive Access

ICA FOUNDATION International Contraceptive Access. Provider Training Presentation May 2012. LEVONORGESTREL INTRAUTERINE SYSTEM. The LNG IUS contraceptive was developed in the 1970s by Population Council and Bayer Schering Pharma Oy, combining the features of oral contraceptives and IUD .

482 views • 34 slides

An introduction to COSMIC RAYS

Catch a Cosmic Ray Program. An introduction to COSMIC RAYS. COSMIC RAYS:. Messages from exploding stars and even more powerful objects. What are cosmic rays? How do we detect them? What can we learn from them? Where do they come from?. History of Cosmic Rays: 1785-1902.

1.04k views • 31 slides

Neutron Stars and Black Holes

0. Neutron Stars and Black Holes. Chapter 11:. 0. Neutron Stars. A supernova explosion of an M > 8 M sun star blows away its outer layers. . P ressure becomes so high that electrons and protons combine to form stable neutrons throughout the object.

492 views • 30 slides

Similarity and Difference in sequences of solar flares, earthquakes, and starquakes

Similarity and Difference in sequences of solar flares, earthquakes, and starquakes. V. Kossobokov International Institute of Earthquake Prediction Theory and Mathematcal Geophysics, Russian Federation Institut de Physique du Globe de Paris, France F. Lepreti, V. Carbone

376 views • 25 slides

The Milky Way Galaxy

695 views • 18 slides

RADIATION PROTECTION IN DIAGNOSTIC AND INTERVENTIONAL RADIOLOGY

IAEA Training Material on Radiation Protection in Diagnostic and Interventional Radiology. RADIATION PROTECTION IN DIAGNOSTIC AND INTERVENTIONAL RADIOLOGY. Part 15.7: Optimization of protection in radiography Practical exercise - processor. Overview / Objectives.

497 views • 15 slides

Neutron Stars

Neutron Stars. Will the PowerPoint presentations ever end? No. . Post-Supernova Explosion. Does the entire star destroy itself during SN? NO. Everything past the core is expelled outward at high velocities.

362 views • 12 slides

Place the following images in a sequence to represent the life cycle of a mid-sized star: 5, 7, 10, 11, 13, 20, 23

222 views • 3 slides