Waves of Destruction: Launch of SDO Adam Jacobs Mentor: Dr. Dean Pesnell NASA Goddard Space Flight Center Code 671 Summer Internship 2010.

Slides:



Advertisements
Similar presentations
Chapter 3 – Radio Phenomena
Advertisements

Electromagnetic Waves
Section 2: The Nature of Light
How do scientific models describe light?
Chapter 15 Section 2 The Nature of Light Objectives
Waves Chapter 8 Waves.
Waves.
RAY OPTICS. 1. Mechanisms Particle/Molecule-light interactions responsible for creating optical effects. These interactions include: reflection, scattering,
Meteorology Moisture in the Atmosphere. Humidity Water Holding Capacity Air Temperature  Humidity - amount of moisture in the air  When an object (including.
Part 7. Special Topics and Appendices Chapter 17 Atmospheric Optics.
Chapter 15: Light, Color and Atmospheric Optics
Detailed vertical structure of orographic precipitation development in cold clouds An illustration of high-resolution airborne mm-wave radar observations.
Rocket Aerodynamics and Stability
Electromagnetic Waves
1 Diagnostics of Solar Wind Processes Using the Total Perpendicular Pressure Lan Jian, C. T. Russell, and J. T. Gosling How does the magnetic structure.
Introduction to Hypersonic Propulsion Systems
Physics of fusion power Lecture 11: Diagnostics / heating.
Classical vs Quantum Mechanics Rutherford’s model of the atom: electrons orbiting around a dense, massive positive nucleus Expected to be able to use classical.
Destructive Effects of Nuclear Weapons
Color in the day and night skies Optical phenomena in the atmosphere is varied and can be awe inspiring. Can range from auroras to halos, sun pillars to.
1 Recognize that all waves transfer energy. R e l a t e f r e q u e n c y & w a v e l e n g t h t o t h e e n e r g y o f d i f f e r e n t t y p e s.
P6 – The Wave Model of Radiation
Wave Basics – Day 1. Fill in the blank: Waves transmit ________. energy.
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Journey to the Center of the Earth
Chapter 15: Light, color and atmospheric optics White and colors White and colors White clouds and scattered light White clouds and scattered light Blue.
Sound and LightSection 2 Section 2: The Nature of Light STANDARDS: SC.912.P Explore the theory of electromagnetism by comparing and contrasting.
Compressible Flow Introduction
Aero Engineering 315 Lesson 20 Supersonic Flow Part II.
Atmospheric Optics Bend, Bounce, and Scatter. Why is the sky blue? First, remember that visible light is made up of a spectrum of colors.
WAVE Basics Chapters 15.
Lecture 21 Nature of Light Reflection and Refraction
 1) Determine the wave speed of a wave that has a period of 3 minutes and a wavelength of 0.05 m.  2) How are electromagnetic and mechanical waves different?
The Sun.
1 Chapter 6 WAVES Dr. Babar Ali. 2 CHAPTER OUTLINE  Wave Concept Wave Concept  Wave Properties Wave Properties  Wave Speed Wave Speed  Wave Types.
Wave property of light Waves can carry energy Wavelength ( ) : distance between successive crests (or troughs) Frequency (f): # of waves passing a point.
Atmospheric Optics - II. RECAP Human perception of color, white objects, black objects. Light scattering: light is sent in all directions –forward, sideways.
Sound 14-5 The Doppler Effect
WAVES. COS 9.0, 9.1,9.2 WHAT YOU’LL LEARN Recognize that waves transfer energy. Distinguish between mechanical waves and electromagnetic waves. Explain.
Chapter Twenty-Three: Waves 23.1 Harmonic Motion 23.2 Properties of Waves 23.3 Wave Motion 1.
Wave Properties Students will be able to Explain wave structure Contrast transverse and longitudinal waves Describe properties of a wave.
Electromagnetic Waves and Their Propagation Through the Atmosphere
Chapter 4 Atmospheric Optics.
Naturally Occurring Optical Phenomena
MAE 4262: ROCKETS AND MISSION ANALYSIS
Transformation of Energy Activity/Investigation Review.
255. Airplane model in free flight at M=1
Question 1 1) wavelength 2) frequency 3) period 4) amplitude 5) energy
Table of Contents The Air Around You Air Pressure Layers of the Atmosphere Energy in Earth’s Atmosphere Heat Transfer Winds The Atmosphere.
Chapter 3 Radiation. Units of Chapter Information from the Skies 3.2 Waves in What? The Wave Nature of Radiation 3.3 The Electromagnetic Spectrum.
What is light? Light can act either like a wave or like a particle Particles of light are called photons.
Waves and Properties of Light
WAVE INTERACTIONS Longitudinal Wave (Compression Wave) wave particles vibrate back and forth along the path that the wave travels.
Chapter 15: Atmospheric Optics Fig. 15-CO, p. 414
Chapter 24 Sec. 1 Light Sec. 2: Tools of Astronomy
Waves We talked about the motion of bodies, such as planets and baseballs. At the most fundamental level, one has elementary particles (electrons, quarks).
Wave Properties. S8P4. Students will explore the wave nature of sound and electromagnetic radiation. d. Describe how the behavior of waves is affected.
Introducing Sound Waves David William D. Ecoben III-Archimedes.
Structure of Earth as imaged by seismic waves
Topic 11.2 Extended A – Mach speeds M ACH S PEEDS  If the sound source moves faster than the speed of sound, the source passes up the wave front, producing.
High-Resolution Polarimetric Radar Observation of Snow- Generating Cells Karly Reimel May 10, 2016.
1 Recognize that all waves transfer energy. R e l a t e f r e q u e n c y & w a v e l e n g t h t o t h e e n e r g y o f d i f f e r e n t t y p e s.
Sound and LightSection 2 Waves and Particles 〉 How do scientific models describe light? 〉 The two most common models describe light either as a wave or.
Waves Unit 1: Lessons 1-2. What are waves? A wave is a disturbance that transfers energy from one place to another A medium is the material through which.
Sound barrier Giorgi Matsaberidze.
If astronauts on Mars wanted to send a message back to Earth
1 WAVES.
Chapter 20 The Energy of Waves.
1 WAVES.
Chapter 20 The Energy of Waves.
Presentation transcript:

Waves of Destruction: Launch of SDO Adam Jacobs Mentor: Dr. Dean Pesnell NASA Goddard Space Flight Center Code 671 Summer Internship 2010

Project Description Atlas 5 Rocket (With SDO Payload) Generating Waves What I Did Described and explained several atmospheric related phenomena Have a meteorologist’s perspective Asked Dr. Pesnell many questions everyday. (See YouTube video)

Launch Topics Trajectory of Atlas 5 Rocket Crepuscular Ray Prandtl-Glauert Collar

Launch Topics Sundog Rocket Generated Waves Interaction of Waves and Sundog

Atlas 5 Rocket Trajectory The Atlas 5 carrying SDO, went Mach 1 somewhere between 8.5 and 9km Plotted sound speed using temperature profile.

Crepuscular Ray How Ray Is Created Light is scattered by particles in the atmosphere. Rays are visible when there is an obstruction. What the Ray Told Us The cloud layer height and depth Corresponds with possible cloud layer in sounding

Prandtl-Glauert Collar How the Prandtl-Glauert Collar Forms Not rare or unheard of for rockets (See Ares rocket at right). Effect of Compressibility. Mark of Subsonic to Transonic Mach range 0.8 – 1.2 Forms due to a sudden pressure drop along surface of body at shock front. Homogenous Nucleation Occurs What Collar Told Us Transonic to Supersonic Transition

Sundog How it’s Created Need a layer of falling ice crystals. In our case, the crystals most likely were hexagonal plates. Falling crystals become nearly horizontal and refract light by 22 degrees

Waves How they formed Rocket created a pulse. Generated by the shock front or thermal expansion of plume. Short pulses create wide ranges of wavelengths. Dispersive wave packet generated. Group velocity observed is about 100 m/s. Wave Type Most likely compression waves. Particle Densities Plate Orientations

Inadvertent Sundog-Waves Interaction Problem of Visibility and Invisibility Sundog disappears with the passage of wave packet. Wave packet was visible both within and away from sundog. Mechanism? Two Possibilities

Reorientation of Ice Crystals Disruption of Horizontal Orientation Wave passage causes turbulence White light shimmering. Waves visible outside of sundog area. Possibly due to increases and decreases in ice crystal densities.

Rapid Sublimation and Deposition of Ice Crystals Temperature increase of at least 25K needed at distance 300 m away. Increase of around 10K would only accelerate growth. Temperature perturbations usually drop off as 1/SQRT(distance).

My Experience at NASA GSFC What I Learned I was exposed to a wide variety of knowledge, from visibility of micrometeorites, to fundamentals of astrophysics. Insight to My Future Field of Study This internship helped strengthen my knowledge of physics and motivated me to continue with an added physics major. Thanks Dr. Dean Pesnell Dominic Dr. Clark ULA for flight data Peter Nishu Shea