Title: An Action due to Thermal Inequilibrium
1An Action due to Thermal Inequilibrium
- P M V Subbarao
- Professor
- Mechanical Engineering Department
Every member of earth wants it for A Refresh
.... A Natural Happening ..
2A Wake-up Call to Earth
3A Means of Generating Primary Wealth on Earth
- Development and ripening of vegetable substances
demand the light and the heat of the Sun. - The source of energy to the Organic Sphere.
- The energy of winds and water originate from the
heat of the Sun. - The winds arise from air currents due to the
heating of the air by the Sun on Earth's surface. - In order to fall, water must first be raised - by
evaporation, which due to the heat of the Sun
persists at the surface of the seas and Earth. - Hence the heat of the Sun maintains all
meteorological, climatic, geological and organic
processes of Earth.
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5The Sun enlightens Every Life
- Kowsalya supraja Rama poorva sandhya
pravarthatheUthishta narasardoola karthavyam
daivamahnikam
6A Natural Engineering Process for the Existence,
Growth and Performance.
- A True Design Reason behind Existence of Natural
Systems.. - A Strong Design Modification for the Performance
of Artificial Systems.
7The Engineering Process Responsible for Evolution
8The Geometry of Natural Products
- An orange is about double the diameter of a
lemon, but could in principle hold eight times
more juice in volume. - Same goes for Elephants.
- Elephants are warm blooded tetrapods.
- Warm blooded animals desire to remain at an
isothermal body temperature of 35 to 42 C
(varies between animals). - The body temperature is maintained at the desired
value with a built-in thermo-regulatory
mechanism. - This mechanism either releases the excess heat
produced in the metabolism or - triggers the body to generate higher metabolic
rate at times, when the body temperature falls
below the desired value.
9Why I Am Different ?
?
10Geometry of An Elephent ?!?!?!
- A bigger warm blooded animal should in principle
generate more metabolic heat energy simply
because it has more volume hence more flesh and
cells. - This metabolic heat release has to be regulated
if it is excess only through the heat transfer
across the skin surface area. - Firstly, in such a situation, having a fur coat
of a hair structure is the least desired thing
and hence Elephants are mostly bald. - The hotter the climate in which they live, the
balder they are. - Secondly, Elephants have large ears which are
packed with capillary structure through which
sizable quantity of blood flows. - The ear flaps of the elephant serve as an
enormous convection fin - a flapping one at that
- to enhance heat transfer from the elephant body
to the environment.
11Classification of Elephants
12Mammoths, living in a cold tundra region, have
fur coats and small hairy ears.
13An Exotic Artificial Device
- The basic invention is due to other sciences
- The final and reliable existence is due to Heat
Transfer
14The Pentium 4 Processor
15Basic Location on A Mother Board
16Heat Sinks for Pentium 4
17Pentium 4 While Performing
18Heat Sinks of Cooling of Electronics
19Heat Sinks Guided Flow
20Heat Sinks Guided Flow with Different Fin Shapes
21Heat Sinks Curious Paired Video
Card-Motherboard Design
22What is Heat Transfer?
- Thermal energy is related to the temperature of
matter. - For a given material and mass, the higher the
temperature, the greater its thermal energy. - Heat transfer is a study of the exchange of
thermal energy through a body or between bodies
which occurs when there is a temperature
difference. - When system and its surroundings are at different
temperatures, thermal energy transfers from the
one with higher temperature to the one with lower
temperature. - Thermal Energy always travels from hot to cold.
- This spontaneous act is called Heat Action or
Heat Transfer.
23Heat Transfer Between System Surroundings
- Heat transfer is typically given the symbol Q,
and is expressed in joules (J) in SI units. - The rate of heat transfer is measured in watts
(W), equal to joules per second, and is denoted
by q. - The heat flux, or the rate of heat transfer per
unit area, is measured in watts per area (W/m2),
and uses q" for the symbol.
24Heat Transfer What Happens to the System ?
- The thermal energy of the system may decrease or
increase. - However, temperature may or may not change
- What is the other property, which is directly
affected by heat transfer? - Specific Heat?
- Any couple like pressure and volume during work
transfer? - Not now .. May be later.
25Modes of Heat Mass Transfer
- Conduction or Diffusion
- Radiation
- Convection
26Thermal conduction through Earth's crust
- Two problems of Geophysics created a concern
about heat conduction - To what extent affects the heat of Earth's
interior by conduction the temperature at the
surface ? - How far inward and in what manner propagate daily
and seasonal temperature variations at Earth's
surface? - The answer through the theory of Kelvin to the
first question is - A stationary thermal state near Earth's surface,
which maintains the heat of its interior, demands
a uniform temperature gradient per metre inwards
from the surface to the centre, provided all the
different layers have the same thermal
conductivity. - Depending on their locations, temperature
measurements in bore holes have yielded different
results, on the average about 1ºC per 33m (medium
geothermal depth gradient). - An answer to the second question is best based on
the observations of the Edinburgh Observatory
(since 1837).
27Conduction Heat Transfer
- Conduction is a significant mode of transfer when
system and surroundings consist of solids or
stationery fluids. - When you touch a hot object, the heat you feel is
transferred through your skin by conduction. - Two mechanisms explain how heat is transferred by
conduction lattice vibration and particle
collision. - Conduction through solids occurs by a combination
of the two mechanisms heat is conducted through
stationery fluids primarily by molecular
collisions.
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30Fourier law of heat conduction
A Constitutive Relation
- The rate of heat transfer through the wall
increases when - The temperatures difference between the left and
right surfaces increase, - The wall surface area increases,
- The wall thickness reduces,
- The wall is changed from brick to aluminum.
- If we measure temperatures of the wall from left
to right and plot the temperature variation with
the wall thickness, we get
This is called as Fourier Law of Conduction
31Thermal Image of Laptop Casing
32Graphite Covering
33Thermal Image of Laptop Casing with Graphite cover
34Most General form of Fourier Law of Conduction
35Radiative Mode of Heat Transfer
- Any body (gt absolute zero) emits radiation at
various wavelengths. - Transparent bodies radiate energy in spherical
space.
- Non-transparent bodies radiate energy in
hemi-spherical space.
- The radiation energy emitted by a body is
distributed in space at various wavelengths. - This complex phenomenon requires simplified laws
for engineering use of radiation.
36Planck Radiation Law
- The primary law governing blackbody radiation is
the Planck Radiation Law. - This law governs the intensity of radiation
emitted by unit surface area of a blackbody as a
function of wavelength for a fixed temperature.
- The Planck Law can be expressed through the
following equation.
h 6.625 X 10-27 erg-sec (Planck Constant) K
1.38 X 10-16 erg/K (Boltzmann Constant) C
Speed of light in vacuum
37Stefan-Boltzmann Law
- The maximum emissive power at a given temperature
is the black body emissive power (Eb). - Integrating Planks Law over all wavelengths gives
Eb.
- Driving forces Heat transfer by radiation is
driven by differences in emissive power
(proportional to T4.
38Radiation from a Thermodynamic System
The total energy emitted by a real system,
regardless of the wavelengths, is given by
- where esys is the emissivity of the system,
- Asys-surface is the surface area,
- Tsys is the temperature, and
- s is the Stefan-Boltzmann constant, equal to
5.6710-8 W/m2K4. - Emissivity is a material property, ranging from 0
to 1, which measures how much energy a surface
can emit with respect to an ideal emitter (e 1)
at the same temperature