Radiation refers to the phenomenon that part of the electromagnetic energy emitted by the emission source (electromagnetic wave, etcelectromagnetic waveOr particles (such asalpha particle、Beta particleAnd so on).
All objects in nature, as long as the temperature isAbsolute temperatureZero degrees (approx-273.15 ℃)All of the above are in the form of electromagnetic waves and particles that constantly transmit heat to the outside. This way of transmitting energy is calledthermal radiation。
Radiated energy fromradiation sourceRadiates straight outward in all directions.The energy emitted by objects through radiation is calledradiant energy。Radiation pressRoentgen/Hourly (R) calculation.An important feature of radiation is that it is "equivalent".No matter the temperature of the object (gas) is high or low, it will radiate outward. Object A can radiate to object B, and at the same time, object B can radiate to Party A.It is commonly used inionizing radiation。
Radiation itself isNeuterHowever, radiation from certain substances may cause harm.
Chinese name
radiation
Foreign name
Radiation
Essence
Physical noun
Pinyin
fú shè
Applied discipline
Telecommunications Nuclear Physics Radiomedicine
Communication mode
It is emitted from the heat source in a straight line all around
According to the relationship with the field source,electromagnetic waveIt can be divided intoCommunication modeIt is a kind of radiation from the heat source along a straight line.Lightradio wavesThe propagation of electromagnetic waves is also called radiation.
Radiation principle
Announce
edit
radiationIt refers to energy in waves orSubatomic particleType transfer of the move.Radiated energy fromradiation sourceRadiates straight outward in all directions.
visible lightIt also belongs to radiation. Generally, it can be classified asionizing radiationorNonionizing radiation。The term is commonly used in ionizing radiation.Ionizing radiation has enough energy to ionize atoms or molecules, while non ionizing radiation does not.radiationActive substancesIt refers to the substance that can emit ionizing radiation.There are three main types of ionizing radiation: alpha, beta and gamma radiation (or radiation).
ionizing radiation
Radiation with high enough energy can ionize atoms.In general, ionization means that an electron is ionized fromElectron shellTo make an atomic bandpositive electricity。Because cells are made of atoms,IonizationCan cause cancer.A cell is made up of trillions of atoms.Induced by ionizing radiationcancerThe probability ofRadiation dose rateAnd radiation receiving organismsInductivity。α. β, γ radiation andNeutron radiationCan be accelerated to ionize atoms with high enough energy.
Nonionizing radiation
Nonionizing radiationIts energy is weaker than that of ionizing radiation.Non ionizing radiation will not ionize matter, but will change the rotation, vibration or valence electron orbital state of molecules or atoms.The effect of non ionizing radiation on living tissues has not been studied for a long time.Different non ionizing radiation can produce different biological effects.
Common radiation
Announce
edit
solar radiation
Solar orientationCosmic spaceElectromagnetic waves and particle streams emitted.The sun received by the earthRadiant energyOnly the sun radiates into spaceTotal radiation1/2 billion of energy, but it isEarth's atmosphereThe main energy source of sports.Reaching the upper boundary of the earth's atmospheresolar radiationEnergy is called astronomical solar radiation.On EarthAverage distance between the sun and the earthThe total energy of the full spectrum of solar radiation received by the unit area of the upper boundary of the earth's atmosphere perpendicular to the solar rays in unit time is calledSolar constant。Solar constantCUoMIs W/m2.Due to different observation methods and techniques, the solar constant values obtained are different.world meteorological organization(WMO) published the solar constant value of 1368 W/m2 in 1981.Upper bound of the earth's atmosphereSolar radiation spectrumMore than 99% of them are between 0.15 and 4.0 μ m in wavelength.About 50% of the solar radiation energy is in the visible spectral region (wavelength 0.4~0.76 μ m), and 7% is in the ultraviolet spectral region (wavelength 0.76 μ m),Maximum energyAt a wavelength of 0.475 microns.Since the wavelength of solar radiation is higher than that of ground andAtmospheric radiationThe wavelength (about 3-120 μ m) is much smaller, so it is also called solar radiationShortwave radiation, called ground and atmospheric radiationLong wave radiation。solar activityThe change of the distance from the sun to the earth will cause the change of the solar radiation energy in the upper boundary of the earth's atmosphere. The solar radiation passes through the atmosphere and some reaches the ground, which is called direct solar radiation;The other part is absorption, scattering and reflection of atmospheric molecules, dust and water vapor in the atmosphere.One part of the scattered solar radiation returns to the space, and the other part reaches the ground. The part that reaches the ground is called the scattered solar radiation.The sum of scattered solar radiation and direct solar radiation reaching the ground is called total radiation.When solar radiation passes through the atmosphere, its intensity and spectral energy distribution change.Ratio of solar radiation energy reaching the groundUpper bound of atmosphereMuch smaller, inSolar spectrumThe upper energy is distributed in the ultravioletSpectral regionAlmost extinct, reduced to 40% in the visible spectrum and increased to 60% in the infrared spectrum.
Astronomical radiationThe spatiotemporal variation characteristics of are as follows: ① Throughout the year, the equator receives the most radiation, while the polar region receives the least radiation.This heat is notuniform distribution, which will inevitably lead to differences in temperature at different latitudes of the earth's surface, and tropical, temperate andCold Climate ;②Astronomical radiation is larger in summer and smaller in winter, which leads to higher temperature in summer and lower temperature in winter.Weakening effect of atmosphere on solar radiationIt includes the absorption, scattering and reflection of solar radiation by the atmosphere.When solar radiation passes through the whole atmosphereultraviolet raysAlmost all are absorbed in the visible light areaAtmospheric absorptionvery seldom.There are strongAbsorption band。The substances in the atmosphere that absorb solar radiation mainly include oxygen, ozone, water vapor andLiquid water, followed bycarbon dioxide、methane、Nitrous oxideAnd dust, etc.Clouds can strongly absorb and scatter solar radiation, and also strongly absorb solar radiation reflected from the ground.Average of cloudreflectivity0.50-0.55.Reaching the ground after atmospheric weakeningDirect solar radiationandScattered radiationThe sum is calledTotal solar radiation。On the global average, the total solar radiation only accounts for 45% of the solar radiation reaching the upper boundary of the atmosphere.totalRadiationIt decreases with latitude and increases with altitude.The maximum value is around noon and 0 at night in a day;Summer is big and winter is small in a year.
electromagnetic radiation
electromagnetic wave(also known aselectromagnetic radiation)Is created byin-phaseOscillating and mutually perpendicular electric and magnetic fields move in the form of waves in space, and their propagation direction is perpendicular to the plane composed of electric and magnetic fields, effectively transferring energy and momentum.Electromagnetic radiation can be classified according to frequency, from low frequency to high frequency, includingradio waves, microwaveinfrared、visible light, UV, (ionizing radiation)X-rayandGamma raywait.The electromagnetic radiation that can be received by the human eye, whose wavelength is about 380 to 780 nm, is calledvisible light。As long as the temperature is greater thanAbsolute zeroAll objects can emit electromagnetic radiation, and there is no object whose temperature is equal to or lower than absolute zero in the world.Therefore, all objects around people are conducting electromagnetic radiation at all times.However, only in thevisible lightfrequency domainThe internal electromagnetic waves can be seen by people.Electromagnetic waves do not need to rely on media to propagate. The speed of various electromagnetic waves is fixed in vacuum, and the speed is the speed of light.[1]
1. CommonElectromagnetic radiation sourceGenerally speaking, radar system, TV, mobile phone and radio transmission system, radio frequency induction and mediaheating equipment , RF and microwaveMedical equipment, variousElectromachiningEquipment, communication transmitting station, satellite earthCommunication station, large power stations, power transmission and transformation equipment, high voltage andEHV transmissionLine, subway train, electric train and most household appliances are all electromagnetic radiation sources that can produce various forms, different frequencies and different intensities.
2. Electromagnetic
Division of radiation field area: electromagnetic radiation field area is generally divided intoFar-fieldandNear-field。
3.1. Near field and characteristics: centered on the field sourceWavelength rangeThe inner region is usually called the near-field, orInduction field。The near field usually has the following characteristics: within the near field,electric field intensityAndmagnetic field intensityThe size of is not proportional.That is, E ¹ 377H.Generally, for field sources with high voltage and low current (such asTransmitting antenna、feederThe electric field is much stronger than the magnetic field. For the field source with low voltage and large current (such as someInduction heating equipmentThe magnetic field is much larger than the electric field.The electromagnetic field intensity in the near field is much larger than that in the far field.From this point of view, electromagnetic protection should focus on the near field.The electromagnetic field intensity of the near field changes rapidly with distanceUniformityLarger.
3.2 The far-field and its characteristics are that the space range with the field source as the center and the radius outside of a wavelength is called far-field, or far-fieldradiation field。The main characteristics of the far-field are as follows: In the far-field, all electromagnetic energy basically radiates and propagates in the form of electromagnetic wavesradiation intensityThe attenuation of is much slower than the induction field.In the far field, the relationship between electric field strength and magnetic field strength is as follows:International System of UnitsIn, E=377H, the running directions of electric field and magnetic field are perpendicular to each other, and both are perpendicular to the propagation direction of electromagnetic wave.The far field isWeak fieldThe electromagnetic field strength is small.
3.3 Significance of the division of near field and far field: Generally, for a fixed electromagnetic radiation source that can produce a certain intensity, the electromagnetic field intensity of the near field radiation is large, so we should pay special attention to the protection of the near field of electromagnetic radiation.In addition, shouldYesAs for the concept of near-field, we are most familiar with the frequency range from 30MHz in short wave band to 3000MHz in micro wave band, and the wavelength range is from 10m to 0.1m.
thermal radiation
thermal radiation, is used for an objectelectromagnetic radiationA form of heat transfer in which heat is dissipated.It does not depend on any external conditions.It is one of the three main modes of heat conduction.
Any object is emittingradiant energyAt the same time, it also continuously absorbs the radiation energy from the surrounding objects.The difference between the energy radiated by an object and the energy absorbed by it is the net energy transmitted by it.The radiant capacity of an object (that is, the energy radiated from a unit surface in a unit time) increases rapidly with the increase of temperature.
The heat effect occurs when the radiant energy is absorbed by the object. The temperature generated by the different radiant energy absorbed by the object is also different.Therefore, radiation isenergy conversion An important way for heat.Radiant heat transfer(radial heat transfer)Electromagnetic wave radiationRealize between hot and cold objectsHeat transferIt is a non-contact heat transfer process that can also be carried out in vacuum.In theory, the electromagnetic waves emitted by objects are distributed in the whole spectrum range, but in the temperature range encountered in industry, what is of practical significance is the thermal radiation whose wavelength is between 0.38 and 1000 μ m, and most of them are located ininfrared(also known asThermal radiation)0.76~20 μ m in the section.so-calledInfrared heatingIs to use the heat radiation in this section.It is very important to study the heat radiation law for the reasonable design of heat transfer in the furnaceHigh temperature furnacejockeyOflabor protectionIt is also of positive significance.When a system needs insulation, even if the temperature of the system is not high, the impact of radiation heat transfer cannot be ignored.asvacuum flaskSilver plating on the gallbladder is to reduce the radiation heat transferHeat loss。
Generally speaking, when an object is radiated by other objects (energy is Q), the part absorbed into heat energy is QA, the part reflected is QR, and the part through the object is QD. Obviously, there is a relationship between these parts and the total energy as shown in the following formula:
QA+QR+QD=Q If A=QA/Q is calledabsorptivity, R=QR/Q is called reflectivity, D=QD/Q is called reflectivityPenetration,
Then: A+R+D=1 If the object's A=1, R=D=0, that is, the energy of the thermal radiation reaching the object's surface is completely absorbed. This object is calledAbsolute blackbody, referred to as boldface.
If R=1, A=D=0, the energy of thermal radiation reaching the surface of the object is fully reflected;
When the reflection is regular, the object is called a mirror;If it is random reflection, it is calledAbsolute white body。
If D=1, A=R=0, that is, the energy of the thermal radiation reaching the surface of the object passes through the object completely. This object is calledDiathermy。
In fact, there is no absolute black body and absolute white body, only some objects are close to absolute black body or absolute white body.
For example: matteBlack paintThe surface is close to the black body, and its absorption rate is 0.97~0.98;The polished copper surface is close toWhite bodyIts reflectivity can reach 0.97.
The absorption and reflection properties of solid surface are mainly affected by the surface condition and color, and the influence of surface condition is often greater than that of color.Solids and liquids are generally impermeable to heat.The energy of thermal radiation passes through the surface of a solid or liquid only after a short distance (generally less than 1mm, and passes through the metal surface only 1 μ m), and is thenComplete absorption。The gas has almost no ability to reflect the thermal radiation energy. Single atom and symmetric diatomic gas (such asAr、He, H2.N2.O2, etc.), can be regarded as a heat permeable body,Polyatomic gas(e.g. CO2H2O、SO2、NH3, CH4, etc.)Absorptive capacity。
The first weak effect phenomenon observed isNucleusOfBeta decay。Later, it was observed thatmeson、baryonandLeptonThrough the decay of weak action andneutrinoScattering and other weak interaction processes.Weak actingRange of forceIt is the shortest of the four functionslow-energyThe process can be approximately regarded as the action of particles participating in the weak interaction process at the same point.
After analyzing the experiment, we found that,FermionThe weak action at one point (called Fermi action) is twoFermionWeakly activecouplingThe so-called weak interaction current is equivalent to the current of electromagnetic action.Coupling constantGAndProton massQuadraticThe product of isDimensionlessSpecific to electromagnetic actionFine structure constant1000 times smaller.This ratio reflects the difference in the intensity of the two actions at low energy.
Weak interaction andElectromagnetic interactionAlthough very different, there are similarities.The weak interaction current is conserved as the current, and there is a relationship between them based on symmetry.
There are two weak interactions, one isLepton(Electronic e,neutrinoν,MuonAnd theirAntiparticle)Participating reactions, such as beta decay, positive beta decay, muon decay andPionDecay, etc;The other one is "K"mesonAnd ΛHyperonThe decay of.The strength of the two weak interactions is the same, both are 10 ^ 12 times weaker than the strong interaction, and the interaction time is about 10 ^ (- 6)~10 ^ (- 8) s.
Protons and neutrons can interact through the following weak interaction processes: 1. Protons+electrons=(reversible) neutrons+Electron neutrino2. Protons+Antielectron neutrino=Neutron+positron
Mobile phone radiationAnd mobile phonesBase station radiationIs different.Generally, the electromagnetic radiation value of a mobile phone is 0.03-0.7, while the radiation value of a mobile phone base station is 10 microwatts.The radiation value generated by a mobile phone base station is much higher than that of a mobile phone.In addition, the closer the distance and the longer the radiation time are, the deeper the damage will be.The distance from the mobile phone base station installed on the roof of ordinary residential buildings to us issafe distance , so the impact is relatively small.