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Benchmarks: Henri Becquerel discovers radioactivity on February
Benchmarks: Henri Becquerel discovers radioactivity on February

REVIEW OF CONCEPTS, QUANTITIES, UNITS AND
REVIEW OF CONCEPTS, QUANTITIES, UNITS AND

... between the energy and the variables time, surface, volume, and solid angle. The quantity energy and its time derivative, energy flux or power, (columns 2 and 3 of Table 1), are most frequently applied to characterize a source. In some fields they may also be termed "radiant energy" and "radiant pow ...
capacitive transducer
capacitive transducer

... polymer films can also be used as piezoelectric materials. For piezoelectric effect, the crystal should have natural asymmetrical charge distribution. Because of this asymmetric charge distribution, the lattice deformation takes place. The lattice deformation is nothing but relative displacement of ...
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... Metamorphism refers to mineralogical and textural changes that occur in rocks as a consequence of changing conditions. Many rocks at the surface of the Earth are out of chemical equilibrium (that is to say, their minerals do not represent the most stable possible physiochemical assemblage). When sub ...
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5. DIMENSIONS, TOLERANCES AND SURFACE

Turning Empty Air Space into Thermal Resistance
Turning Empty Air Space into Thermal Resistance

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Exciton quantum confinement in nanocones formed on a surface of

... The decrease of Zn atoms concentration in the top layer with increased intensity of LR, according to the proposed model, leads to the ‘red shift’ of the exciton bands in PL spectra, as was shown in [21], but increase of the Zn atoms concentration in the buried CdZnTe layer manifests itself in the bl ...
Thermodynamic properties of liquid mercury to 520 K and 7 GPa
Thermodynamic properties of liquid mercury to 520 K and 7 GPa

... We however emphasize that, while this imaging configuration is thus very powerful (both thickness and sound velocity of the sample are determined using a self consistent method), it has the main disadvantage to be very time consuming nothing compare to the couple of seconds needed by the ”temporal m ...
Radiation Pressure of a Monochromatic Plane Wave on a Flat Mirror
Radiation Pressure of a Monochromatic Plane Wave on a Flat Mirror

Il`ja M. Frank - Nobel Lecture
Il`ja M. Frank - Nobel Lecture

... along the path of the particle remains unchanged. For example, if a uniformly moving charged particle crosses the boundary of two media with different indices of refraction, there appears transition radiation. Radiation appears because the jump which the magnitude of the phase velocity of light unde ...
Chapter 30 Maxwell`s Equations and Electromagnetic Waves
Chapter 30 Maxwell`s Equations and Electromagnetic Waves

... absorption. The cross-sectional area of the atom for resonant absorption is approximately equal to λ2, where λ is the wavelength of the laser light. (a) Estimate the acceleration of a rubidium atom (molar mass 85 g/mol) in a laser beam whose wavelength is 780 nm and intensity is 10 W/m2. (b) About h ...
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Hydraulic Press tonnage calculation Diameter (inches) Pressure

... Example: To draw a 5" diameter cup of .040" stock with a tensile strength of 46,000 psi would require the following tonnage: (5 x 3.1416) x .040 x (46000/2000) = 14.44 tons A 20-ton press would be recommended ...
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Charged Particle Measurements during Cruise and on Mars with the

Definitions of Quantities used in Radiation Theory
Definitions of Quantities used in Radiation Theory

... wavelength (it is zero outside the range of sensitivity of the eye!), and for heterochromatic radiation the conversion between lumens and watts requires some careful computation. The number of lumens generated by a lightbulb per watt of power input is called the luminous efficiency of the lightbulb. ...
Rocket Science and Technology, 4363 Motor Ave
Rocket Science and Technology, 4363 Motor Ave

... point passes through a normal shock before being isentropically compressed to zero speed. Equation (100) of ref. (1) is the Rayleigh pitot formula. It states that pT/p∞ = [½ ( M∞2][( /M∞2]1/( The stagnation pressure coefficient is, by definition, CpT = (p ...
Lecture 1: Astrophysics
Lecture 1: Astrophysics

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The physico-chemical history of Falling Evaporating Bodies around

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Photoprocesses in protoplanetary disks

SOFIA`s Invisible Universe - Deutsches SOFIA Institut
SOFIA`s Invisible Universe - Deutsches SOFIA Institut

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OPTICAL PROPERTIES of Nanomaterials

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Solids and Fluids

... real objects when forces are applied are often too important to ignore (causing deformations) • Stress characterizes the strength of the forces causing the deformation (force per unit area) • Strain describes the resulting deformation • When the stress and strain are small enough, the two are direct ...
chapter4
chapter4

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Peer Review 12/5/03 - Colorado Space Grant Consortium
Peer Review 12/5/03 - Colorado Space Grant Consortium

... node. This does not determine how much is reflected or absorbed, but simply how much is incident. The inputs for this program include the view factors each node has with the sun and earth determined by Supview, as well as the positions given by FindB6 that we are interested in solving for. This file ...
The Institute of Physical Chemistry of the Polish Academy of Sciencies
The Institute of Physical Chemistry of the Polish Academy of Sciencies

... with theoretical model predictions. It turned out that the negative compressibility of sodium amidoborane crystals has to be a consequence of the elongation of the chemical bonds between nitrogen and hydrogen and boron and nitrogen, caused by the abrupt formation of new hydrogen bonds between adjace ...
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Radiation pressure



Radiation pressure is the pressure exerted upon any surface exposed to electromagnetic radiation. Radiation pressure implies an interaction between electromagnetic radiation and bodies of various types, including clouds of particles or gases. The interactions can be absorption, reflection, or some of both (the common case). Bodies also emit radiation and thereby experience a resulting pressure.The forces generated by radiation pressure are generally too small to be detected under everyday circumstances; however, they do play a crucial role in some settings, such as astronomy and astrodynamics. For example, had the effects of the sun's radiation pressure on the spacecraft of the Viking program been ignored, the spacecraft would have missed Mars orbit by about 15,000 kilometers.This article addresses the macroscopic aspects of radiation pressure. Detailed quantum mechanical aspects of interactions are addressed in specialized articles on the subject. The details of how photons of various wavelengths interact with atoms can be explored through links in the See also section.
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