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When writing a Lewis structure we restrict a molecule s electrons to certain well defined locations either linking two atoms by a covalent bond or as unshared electrons on a sm gle atom Sometimes more than one Lewis structure can be written for a molecule espe cially those that contain multiple bonds An example often cited m introductory chem istry courses is ozone (O3) Ozone occurs naturally m large quantities m the upper atmosphere where it screens the surface of the earth from much of the sun s ultraviolet rays Were it not for this ozone layer most forms of surface life on earth would be dam aged or even destroyed by the rays of the sun The following Lewis structure for ozone satisfies fhe ocfef rule all fhree oxygens have eighf elecfrons m fheir valence shell... [Pg.24]

Measurements of ozone (O3) concentrations in the atmosphere are of particular importance. Ozone absorbs strongly in the ultraviolet region and it is this absorption which protects us from a dangerously high dose of ultraviolet radiation from the sun. The vitally important ozone layer lies in the stratosphere and is typically about 10 km thick with a maximum concentration about 25 km above the surface of the earth. Extreme depletion of ozone in a localised part of the atmosphere creates what is known as an ozone hole. [Pg.380]

The ionosphere is part of the larger magnetosphere, a cavity in the stream of particles from the sun. The cavity is produced by the earth s magnetic field (56,57). The ionosphere and the Van AHen radiation belt He within the plasmasphere, which extends to a maximum distance of about 15,000 km above the earth s surface. [Pg.113]

In modem PMR constmction, thermal iasulation that is unaffected by water or that can be kept dry ia some manner is required. Extmded polystyrene (XEPS) foam iasulation boards ate commonly employed (see Insulation, thermal). They ate placed on top of the waterproofing roof membrane, which is next to the deck. The iasulation should not be adhered to the membrane. Ballast at the rate of >48.8 kg/m (1000 lb/100 ft ) holds the iasulation ia place and offers protection from the sun. The iasulation joiats ate open and drainage must be provided. Various other materials, eg, patio blocks and concrete slabs, ate also used as sutfaciags and ballast. The extra weight imposes mote exacting requirements on constmction. [Pg.211]

The use of wind as a renewable energy source involves the conversion of power contained in moving air masses to rotating shaft power. These air masses represent the complex circulation of winds near the surface of Earth caused by Earth s rotation and by convective heating from the sun. The actual conversion process utilizes basic aerodynamic forces, ie, lift or drag, to produce a net positive torque on a rotating shaft, resulting in the production of mechanical power, which can then be used directly or converted to electrical power. [Pg.232]

Trace amounts of vanadium have been found in meteorites and seawater, and it has been identified in the spectmm of many stars including the earth s sun. The occurrence of vanadium in oak and beech trees and some forms of aquatic sea life indicates its biological importance. [Pg.381]

An accompanyiag effect of eutrophication that is more readily observable ia Table 1 is a decrease ia siUca coaceatratioa ia Lake Oatario. Some decliae ia dissolved siUca appareatiy has occurred ia all of the lakes except Lake Superior. This decliae is brought about by the growth of diatoms, a species of aquatic microorganisms ia the upper layers of lake water that is widespread ia all types of water impouadmeats where the water is clear and exposed to the sun. The siUca is used by these microorganisms to form their skeletons and is later precipitated and becomes part of the bed sediment. [Pg.203]

Nucleation tempering of the stiU molten fat is necessary because the cocoa butter, if left to itself, can soHdify in a number of different physical forms, ie, into an unstable form if cooled rapidly, or into an equally unacceptable super stable form if cooled too slowly, as commonly happens when a chocolate turns gray or white after being left in the sun. The coarse white fat crystals that can form in the slowly cooled center of a very thick piece of chocolate are similarly in a super stable form known in the industry as fat bloom. [Pg.95]

Because the system likely is nonisothermal, the analysis of a closed-desiccant system requites knowledge of the temperature of the desiccant as well as the dew point (ice point) or water concentration (partial pressure) specification. Indeed, the whole system may undergo periodic temperature transients that may compHcate the analysis. Eor example, in dual-pane windows the desiccant temperature is approximately the average of the indoor and outdoor temperatures after a night of cooling. However, after a day in the sun, the desiccant temperature becomes much warmer than the outdoor temperature. When the sun sets, the outdoor pane cools quickly while the desiccant is still quite warm. The appropriate desiccant for such an appHcation must have sufficient water capacity and produce satisfactory dew points at the highest temperatures experienced by the desiccant. [Pg.509]

This occurs when the nocturnal inversion is dissipated by heat from the morning sun. The lapse layer usually starts at the ground and works its way upward (less rapidly in winter than in summer). Fumigation may also occur in sea-breeze circulations during late morning or early afternoon. The shaded zone of strong concentration is that portion of the plume which has not yet been mixed downward. [Pg.2184]

All of the energy that drives the atmosphere is derived from a minor star in the universe—our sun. The planet that we inhabit, earth, is 150 million km from the sun. The energy received from the sun is radiant energy—electromagnetic radiation. The electromagnetic spectrum is shown in Fig. 17-1. Although this energy is, in part, furnished to the atmosphere, it is primarily received at the earth s surface and redistributed by several... [Pg.243]

Because of the tilt of the earth s axis by 23.5° with respect to the plane of the earth s revolution around the sun, the north pole is tilted toward the sun on June 22 and away from the sun on December 21 (Fig. 17- 2). This tilt causes the solar beam to have perpendicular incidence at different latitudes depending on the date. The zenith angle Z is determined from ... [Pg.247]

Radiative heat transfer is perhaps the most difficult of the heat transfer mechanisms to understand because so many factors influence this heat transfer mode. Radiative heat transfer does not require a medium through which the heat is transferred, unlike both conduction and convection. The most apparent example of radiative heat transfer is the solar energy we receive from the Sun. The sunlight comes to Earth across 150,000,000 km (93,000,000 miles) through the vacuum of space. FIcat transfer by radiation is also not a linear function of temperature, as are both conduction and convection. Radiative energy emission is proportional to the fourth power of the absolute temperature of a body, and radiative heat transfer occurs in proportion to the difference between the fourth power of the absolute temperatures of the two surfaces. In equation form, q/A is defined as ... [Pg.613]

Th ese manufactured light sources are, perhaps ironically, largely dependent on the Sun. The radiant energy from the Sun has been stored in the fossilized remains of billions of creatures over millions of years and is used to power the electric light sources created by modern humans. The power generated by hydroelectric sources also is a result of solar evaporation and subsequent rainfall. Only nuclear reactors provide power independent of the Sun, which is, of course, the largest nuclear reactor in the solar system. [Pg.709]

Heppenheimer, T. A. (1984). The Man Made Sun The Quest for Fusion Power. Boston Little, Brown and Company. [Pg.878]

Rhodes, R. (1995). Dark Sun The Making of the Hydrogen Bomb. NewYork Simon Schuster. [Pg.878]

Solar array efficiency depends on its orientation to the sun. The best result is achieved if the array faces the sun at an angle of 90° to S5°. Precise orientation can be achieved either through the rotation of the whole spacecraft, or the rotation of the solar arrays only. To ensure constant electricity flow regardless of changes in spacecraft orientation, solar arrays charge... [Pg.1077]

Solar Arrays Visual solar -Long life-span -Require precision Sun The most widely used... [Pg.1078]

We do not need a hand lens to feel the energy of light rays. Just remember those lazy afternoons you spent last summer soaking up the warmth of the sun. The afternoon pleasure... [Pg.253]

The substances we can use come primarily from the earth. In its movement around the sun, the earth sweeps through space and collects material from meteors and some cosmic dust, but the amount of gathered material is small compared with the amount present in the earth. We shall consider the material of the earth and see how it is put to use by mankind. [Pg.437]

Our solar system consists of the Sun, the planets and their moon satellites, asteroids (small planets), comets, and meteorites. The planets are generally divided into two categories Earth-like (terrestrial) planets—Mercury, Venus, Earth, and Mars and Giant planets—Jupiter, Saturn, Uranus, and Neptune. Little is known about Pluto, the most remote planet from Earth. [Pg.444]

OXAZOLIDINEDIONES. Drowsiness is the most common adverse reaction and, as with the other anticonvulsants, tends to subside with continued use Visual disturbances may also occur. The patient with a visual disturbance is assisted with ambulation and oriented carefully to the environment. The nurse ensures that the environment is safe The patient may be especially sensitive to bright lights and may want the room light to be kept dim. Because photosensitivity can occur, the nurse must keep the patient out of the sun. The nurse instructs the patient to use sunscreens and protective clothing until the individual effects of the drug are known. [Pg.261]

Sulfur dioxide is a reducing bleach and can counter the effects of oxidizing bleaches, thus preserving color in fruits dried in the sun. The combination of fruit acids and ultraviolet light would otherwise react with the colorful compounds, making the fruit pale. [Pg.13]

Why Do We Need to Know This Material The topics described in this chapter may one day unlock a virtually inexhaustible supply of clean energy supplied daily by the Sun. The key is electrochemistry, the study of the interaction of electricity and chemical reactions. The transfer of electrons from one species to another is one of the fundamental processes underlying life, photosynthesis, fuel cells, and the refining of metals. An understanding of how electrons are transferred helps us to design ways to use chemical reactions to generate electricity and to use electricity to bring about chemical reactions. Electrochemical measurements also allow us to determine the values of thermodynamic quantities. [Pg.603]

The composition of the Earth was determined both by the chemical composition of the solar nebula, from which the sun and planets formed, and by the nature of the physical processes that concentrated materials to form planets. The bulk elemental and isotopic composition of the nebula is believed, or usually assumed to be identical to that of the sun. The few exceptions to this include elements and isotopes such as lithium and deuterium that are destroyed in the bulk of the sun s interior by nuclear reactions. The composition of the sun as determined by optical spectroscopy is similar to the majority of stars in our galaxy, and accordingly the relative abundances of the elements in the sun are referred to as "cosmic abundances." Although the cosmic abundance pattern is commonly seen in other stars there are dramatic exceptions, such as stars composed of iron or solid nuclear matter, as in the case with neutron stars. The... [Pg.14]

Table II shows, as an example, the combinations of low and high levels for three factors selected by a design team for an accelerated test Involving photovoltaic solar cells. In column 2 the three factors are seen to be temperature T (50 C, 95 C), relative humidity RH (60%, 85%), and ultraviolet radiation UV (five suns, 15 suns). The eight combinations of the high and low levels are shown, together with the predicted months to failure for each combination. In this example the documentation to support each prediction is symbolically referenced as shown in the last column. The documentation includes assumptions, calculations, references to the literature, laboratory data, computer simulation results, and other related material. Such a factorial table is first completed by each scientist independently. Subsequently, the team alms to generate a single consensus factorial table has the same form as that shown in Table II. Table II shows, as an example, the combinations of low and high levels for three factors selected by a design team for an accelerated test Involving photovoltaic solar cells. In column 2 the three factors are seen to be temperature T (50 C, 95 C), relative humidity RH (60%, 85%), and ultraviolet radiation UV (five suns, 15 suns). The eight combinations of the high and low levels are shown, together with the predicted months to failure for each combination. In this example the documentation to support each prediction is symbolically referenced as shown in the last column. The documentation includes assumptions, calculations, references to the literature, laboratory data, computer simulation results, and other related material. Such a factorial table is first completed by each scientist independently. Subsequently, the team alms to generate a single consensus factorial table has the same form as that shown in Table II.

See other pages where The Sun is mentioned: [Pg.2809]    [Pg.348]    [Pg.298]    [Pg.396]    [Pg.355]    [Pg.244]    [Pg.273]    [Pg.24]    [Pg.7]    [Pg.888]    [Pg.144]    [Pg.1050]    [Pg.1063]    [Pg.1067]    [Pg.340]    [Pg.367]    [Pg.16]    [Pg.27]    [Pg.46]    [Pg.122]    [Pg.130]    [Pg.138]    [Pg.154]    [Pg.641]    [Pg.13]   
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See also in sourсe #XX -- [ Pg.132 ]

See also in sourсe #XX -- [ Pg.14 , Pg.48 , Pg.57 , Pg.72 , Pg.96 , Pg.106 , Pg.127 , Pg.129 , Pg.150 ]




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A Place in the Sun

Acceleration due to gravity on the sun, moon, and planets

Arsenic in the Sun, Moon, and planets

Aspects to the Sun

Back to the Sun

Drying in the sun

Energy from the sun

Essence of the Sun

Heart of the Sun

Helium in the Sun

Here Comes the Sun

History of the Sun

Irradiance of the sun

Light from the sun

Neutrinos from the Sun

Nuclear reactions in the Sun

Relative abundance of elements in the sun

Solar Panel Orientation Requirements to Achieve Optimum Power from the Sun

Spectroscopic observations of the Sun

Surface of the sun

The Early Sun and Evolution of Terrestrial Planets

The Morning Sun and Star (detail from Plate

The Setting Sun

The Sun Sign Combinations

The Sun and Solar-Type Main Sequence Stars

The Sun as Radiation Source

The Sun as reference

The Sun-Earth system

UV Energy from the Sun

Water Signatures in Spectra of Late Type Stars and the Sun

Why do surfaces exposed to the sun get so dusty

Why do we get hot when lying in the sun

Why do we get hot while lying in the sun

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