Destructive Effects of Nuclear Weapons

Slides:



Advertisements
Similar presentations
Theory of Explosives C3 Slide 1.
Advertisements

Supernova Remnants Shell-type versus Crab-like Phases of shell-type SNR.
“ a disturbance or variation that transfers energy progressively from point to point in a medium and that may take the form of an elastic deformation or.
Example 3.1 Air flows from a reservoir where P = 300 kPa and T = 500 K through a throat to section 1 in Fig. 3.4, where there is a normal – shock wave.
The Nature of the Blast  Efficiency of explosion  Kind and shape of blasts  Blast effects, range & damage  Thermal effects  Radiation effects The.
The nature of weapon tests  High Altitude Air Blast: fireball > 100,000 ft (>3000m)  Low Altitude Air Blast: fireball < 100,000 ft (without touching.
Reactive and Explosive Materials An Introduction.
Incident Date:1/11/2012 Time:07:30 AM Fatality: 25 injuries: 131 Total losses:
Cutnell/Johnson Physics 8th edition Reading Quiz Questions
1 Fall 2004 Physics 3 Tu-Th Section Claudio Campagnari Lecture 3: 30 Sep Web page:
Destructive Effects of Nuclear Weapons Blast damage Thermal damage Radiation damage EM-pulse  The generation of a mechanical shock through sudden increase.
Cloud Altitude Maximum altitude for cloud rise is reached after ~ 4min. RATE OF RISE OF THE RADIOACTIVE CLOUD FROM a I-MEGATON AIRBURST Height Time Rate.
Enclosure Fire Dynamics
PHYSICS 103: Lecture 17 Agenda for Today: Temperature and Heat
Radiation Definitions and laws Heat transfer by conduction and convection required the existence of a material medium, either a solid or a.
Waves Transferring Energy. Waves: traveling disturbance that carries energy from one place to another Waves travel through water, but they do not carry.
AOS 100 Lecture 3 Atmospheric Variables Chapter 1 Homework #1 Due September 19, 2014 TYU Ch1: 3,4,5,8,11,13,16,19; TYPSS Ch 1: 1 TYU Ch 2: 1,2,6,9,13,16,20,22,23,25;
CHAPTER 37 : INTERFERENCE OF LIGHT WAVES
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.
Pro-Science 4 th International Conference of Hydrogen Safety, September 12-14, 2011, SAN FRANCISCO, USA EXPERIMENTAL STUDY OF IGNITED UNSTEADY HYDROGEN.
CHAPTER 5 Concentration Models: Diffusion Model.
Means & Methods of Homogeneous Charge Combustion P M V Subbarao Professor Mechanical Engineering Department A Sudden Combustion, Yet Needs A Care & takes.
FIRES AND EXPLOSION LECTURE 10.
The Effects of Nuclear Weapons: Terrorist Threat.
Potential Energy and Conservative Forces
Nuclear Weapons Number of operational warheads in the U.S. nuclear stockpile, according to the Pentagon. The figure is down from a peak of 31,225.
Explosion An explosion is a rapid expansion of gases resulting in a rapid moving pressure or shock wave. The expansion can be mechanical or it can be.
Chapter 17 Sound Waves: part two HW 2 (problems): 17.22, 17.35, 17.48, 17.58, 17.64, 34.4, 34.7, Due Friday, Sept. 11.
Energy: Warming the Earth & the Atmosphere
The Sun.
Spectra What determines the “color” of a beam of light? The answer is its frequency, or equivalently, its wavelength. We see different colors because.
Photon Statistics Blackbody Radiation 1.The energy loss of a hot body is attributable to the emission of electromagnetic waves from the body. 2.The.
LT. 1.2 Radiological Defense.. Enabling Objectives. (page 1) 1.4 Recognize the characteristics and effects of nuclear weapons in accordance with fm 3-3-1,
Physics 101: Lecture 33 Sound
 Students will be able to identify three properties of the atmosphere and how they interact.  Students will be able to explain why atmospheric properties.
Violent Storms. THUNDERSTORMS FORM IN WARM,MOIST UNSTABLE AIR. CUMULONIMBUS CLOUDS. ATTAIN HEIGHTS OF 20 KM. TORRENTIAL RAIN,DAMAGING WINDS, LIGHTNING,
{ Week 22 Physics.  Understand that a star is in equilibrium under the action of two opposing forces, gravitation and the radiation pressure of the star.
Thermodynamics. Temperature  How hot or cold something feels compared to a standard  Typically water is our standard  Function of kinetic energy 
Nuclear Bombs Note 5/_/03. What is a nuclear bomb Fission bombs – Alamargordo & Nagasaki Hydrogen bombs – fission-fusion-fission bombs\
Motion Observing To observe an object in motion, you must use a referenced object. The one sitting still is considered to be the reference point. When.
Radioactive Decay By: Nathaniel Hunt.
Green House Effect and Global Warming. Do you believe that the planet is warming? 1.Yes 2.No.
Earth’s Energy Budget. Modes of Energy Travel Heat Energy can be transferred in three specific ways: Heat Energy can be transferred in three specific.
Underwater Blasts. Cloud formation in underwater tests Baker (fat man design) Bikini Atoll 1946; 23 kT Formation of spray dome & condensation cloud from.
THE LITTLE BOY. Development  The Little Boy bomb was constructed through the Manhattan Project during World War II.  Creation of the bomb started in.
Try this: - Get colored pencils: - Red, Orange,Yellow,Green,Blue,Violet – Use the spectroscope to look at the lights in the room and then out the window.
Flow of Compressible Fluids. Definition A compressible flow is a flow in which the fluid density ρ varies significantly within the flowfield. Therefore,
Light Waves Physics 1 L Mrs. Snapp. Light Light is a transverse wave. Light waves are electromagnetic waves--which means that they do NOT need a medium.
Quantum Theory and the Electronic Structure of Atoms Chapter 7.
CHARACTERISTICS OF WAVES Properties of Waves. WHAT ARE THE AMPLITUDE, WAVELENGTH, FREQUENCY, AND SPEED OF A WAVE?  Waves vary greatly.  Waves can be.
Heat Transfer RADIATION HEAT TRANSFER FUNDAMENTALS.
Physical Principles of Remote Sensing: Electromagnetic Radiation
The nature of radiation
Chapter 13 The Transfer of Heat.
Basic Science in Remote Sensing
THUNDERSTORMS.
Electromagnetic Radiation
Radiation  = 1 for blackbody (emissivity) Qr = T4
Natural Environments: The Atmosphere
FIGURE 2.1 Comparison of Kelvin, Celsius, and Fahrenheit scales.
Nuclear Bombs.
Radiation in the Atmosphere
20 miles.
Physics 2 – Mar 6, 2018 Do Now – How much power is generated by a windmill if it’s blades are 1.30 m long, the density of air is 1.15 kg/m3 and the wind.
Introduction and Basic Concepts
Wind Velocity One of the effects of wind speed is to dilute continuously released pollutants at the point of emission. Whether a source is at the surface.
Chapter 13 The Transfer of Heat.
It is 1950 the sound you hear is an air raid warning of a possible nuclear attack. Immediately get under your desk and cover yourself with your arms protecting.
WAVES.
Presentation transcript:

Destructive Effects of Nuclear Weapons Blast damage Thermal damage Radiation damage EM-pulse The generation of a mechanical shock through sudden increase of pressure causes mechanical damages The generation of a heat wave expanding with the shock causes incineration The distribution of radiation through Short range and atmospheric fallout causes short term and long term radiation sickness effects Electromagnetic shock leads to break-down of communication systems

The mechanical shock pressure shock velocity: vs sound speed: cs 0.10 ms 0.24 ms shock velocity: vs sound speed: cs specific heat: =1.4 peak pressure: p air pressure: p0=15 psi wind velocity: vw dynamic pressure: q 0.38 ms 0.52 ms pressure 0.66 ms 0.80 ms 0.94 ms

Example Depending on the peak pressure (atmospheric pressure 15 psi) and the speed of sound (cs=330 m/s in atmospheric gas) you receive the following values for shock and wind velocity and dynamic pressure

Shock characteristics Shock on flat surface causes reflection which is expressed by reflected overpressure pr! for large dynamic pressure for small dynamic pressure

Example shock front against house

example 250 kT blast Nevada 1953 effect on houses in different distance from center of blast 2.65 miles 5.3 miles

over pressure – wind velocity Even an over pressure of 2 psi generates hurricane like storm conditions!

The American Home

Shock expansion Shock expands radially from explosion center. Amplitude decreases, but after time t5 the pressure behind shock front falls below atmospheric pressure, Under-pressure which causes the air to be sucked in.

Overpressure and Mach Stem

Pressure conditions with transversing shock Shock hits generates strong wind Shock decreases Underpressure Wind direction changes Normal air pressure Wind calms down

Pressure induced wind effects

Scaling laws for blast effects Shock/blast expands over volume ~d3, the following scaling law can be applied for estimating distance effects between different blast strengths Normalized to a standard 1kT blast the following expression can be applied:

Distance Effects Scaling for blast intensities 100 kT e.g. the effect which occurs for a 1 kT blast at distance d1 occurs for a 100kT blast at distance d. d1=10,000ft d=24,662ft. 1 kT Peak over pressure as function of distance for a 1kT blast

Distance effects of airburst damage comparison for a 1000 kT and a 500 kT bomb using the scaling law with respect to 200 kT bomb

Scaling in Altitude often scaled to W1 = 1 kT Similar scaling relation for altitude dependence of blast effects. For altitudes less than 5000 ft (1700 m) normal atmospheric conditions can be assumed. For higher altitude effects changes, altitude dependence of air pressure and sound speed need to be taken into account.

Peak overpressure in height & distance Suppose you have 80 kT bomb at 860 ft height, what is the distance to which 1000psi overpressure extends? Normalization: W1=1kT Corresponding height for 1kT burst (or scaled height) Distance of 1000 psi overpressure

Surface burst versus airburst Suppose you have 500 kT bomb at 1.1 mile height, what is the distance to which 2 psi overpressure extends and compare with ground zero detonation. Scaled height for 1 kT bomb; h1 = h/W1/3 = 0.14 miles ≈ 765 ft. This corresponds to d1 = 3800 ft = 0.69 miles. The distance for the 2 psi overpressure on the ground from the 500 kT blast would be d = d1·W1/3 = 0.69·5001/3 = 5.5 miles. Surface burst: d1=2500 ft=0.45 miles, d = d1·W1/3 = 0.45·5001/3 = 3.6 miles.

Blast effects on humans

Thermal effects Approximately 35 percent of the energy from a nuclear explosion is an intense burst of thermal radiation, i.e., heat. Thermal effects are mainly due to originated heat from blast which expands with wind velocity and incinerates everything within expansion radius. The thermal radiation from a nuclear explosion can directly ignite kindling materials. Ignitable materials outside the house, such as leaves, are not surrounded by enough combustible material to generate a self-sustaining fire. Fires more likely to spread are those caused by thermal radiation passing through windows to ignite beds and overstuffed furniture inside houses. Fallout 10% Blast 50% Thermal 35% Initial Radiation 5%

Thermal Energy Release For a fireball with radius r the heat emitting surface is: Total energy emitted per cm2 and second is described by the Stefan Boltzmann law Total thermal energy emission from fireball is therefore: With radius r in units m and temperature T in Kelvin

The thermal power of the fireball changes with time. Thermal energy release should be expressed in terms of maximum power Pmax (scaled power) and in terms of scaled time tmax which corresponds of time of the maximum thermal energy release from the fireball. Fireball power Fraction of emitted thermal energy

For air bursts below 15,000 ft altitude the maximum power Pmax & the maximum time tmax are related to the bomb yield W (in kT) e.g. for a 500 kT burst in 5000 ft altitude: According to the scaling laws expressed in the figure, total power and fraction of heat release can be calculated for any time; e.g. the total amount of thermal energy emitted at t=1sec is: Fraction of thermal energy released at 1 s is 40%!