Solar radiation - what is it? Total solar radiation. Solar radiation: types

Prominence on the surface

Radiation from the Sun, which is known as sunlight, is a mixture electromagnetic waves, from infrared (IR) to ultraviolet (UV) rays. It includes visible light, which falls between IR and UV on the electromagnetic spectrum.

Speed ​​of propagation of electromagnetic waves

All electromagnetic waves (EM) travel at a speed of approximately 3.0x10*8 m/s in a vacuum. Space is not a perfect vacuum, it actually contains particles in low concentration, electromagnetic waves, neutrinos and magnetic fields. Since the average distance between the Earth and the Sun is more than 149.6 million km, it takes about 8 minutes for the radiation to reach the Earth. The sun shines not only in the IR, visible and UV ranges. Basically, it emits high energy gamma rays.

However, gamma ray photons travel a long way to the surface, they are constantly absorbed by solar plasma and re-emitted with a change in their frequency.

By the time they reach the surface, the gamma ray photons are in the IR, visible and UV spectrum. Infrared radiation is the heat that we feel. Without him and visible light, life on Earth would be impossible. During solar flares, it also emits X-rays. When electromagnetic radiation from the Sun reaches the Earth's atmosphere, some of it is absorbed while the rest reaches the Earth's surface.

In particular, UV radiation is absorbed ozone layer and is re-radiated as heat, resulting in warming of the stratosphere.

SOLAR RADIATION

SOLAR RADIATION- electromagnetic and corpuscular radiation from the Sun. Electromagnetic radiation travels as electromagnetic waves at the speed of light and penetrates the earth's atmosphere. To earth's surface Solar radiation comes in the form of direct and diffuse radiation.
Solar radiation - main source energy for all physical and geographical processes occurring on the earth's surface and in the atmosphere (see Insolation). Solar radiation is usually measured by its thermal effect and is expressed in calories per unit surface area per unit time. In total, the Earth receives less than one two billionth of its radiation from the Sun.
The spectral range of electromagnetic radiation from the Sun is very wide - from radio waves to X-rays - but its maximum intensity falls on the visible (yellow-green) part of the spectrum.
There is also a corpuscular part of solar radiation, consisting mainly of protons moving from the Sun at speeds of 300-1500 km/s (solar wind). During solar flares, high-energy particles (mainly protons and electrons) are also produced, forming the solar component of cosmic rays.
The energy contribution of the corpuscular component of solar radiation to its overall intensity is small compared to the electromagnetic one. Therefore, in a number of applications the term “solar radiation” is used in a narrow sense, meaning only its electromagnetic part.
The amount of solar radiation depends on the height of the sun, time of year, and transparency of the atmosphere. Actinometers and pyrheliometers are used to measure solar radiation. The intensity of solar radiation is usually measured by its thermal effect and is expressed in calories per unit surface area per unit time.
Solar radiation strongly affects the Earth only during the daytime, of course - when the Sun is above the horizon. Also, solar radiation is very strong near the poles, during polar days, when the Sun is above the horizon even at midnight. However, in winter, in the same places, the Sun does not rise above the horizon at all, and therefore does not affect the region. Solar radiation is not blocked by clouds, and therefore still reaches the Earth (when the Sun is directly above the horizon). Solar radiation is a combination of the bright yellow color of the Sun and heat, heat also passes through clouds. Solar radiation is transmitted to Earth by radiation, not by thermal conduction.
The amount of radiation received by a celestial body depends on the distance between the planet and the star - as the distance doubles, the amount of radiation received from the star to the planet decreases fourfold (proportional to the square of the distance between the planet and the star). Thus, even minor changes the distances between the planet and the star (depending on the eccentricity of the orbit) lead to a significant change in the amount of radiation entering the planet. The eccentricity of the earth's orbit is also not constant - over the course of millennia it changes, periodically forming an almost perfect circle, sometimes the eccentricity reaches 5% (currently it is 1.67%), that is, at perihelion the Earth currently receives 1.033 more solar radiation than at aphelion, and at the greatest eccentricity - more than 1.1 times. However, the amount of incoming solar radiation depends much more strongly on the changes of the seasons - currently the total amount of solar radiation entering the Earth remains practically unchanged, but at latitudes of 65 N.Sh (the latitude of the northern cities of Russia and Canada) in the summer the amount of incoming solar radiation more than 25% more than in winter. This occurs because the Earth is tilted at an angle of 23.3 degrees in relation to the Sun. Winter and summer changes are mutually compensated, but nevertheless, as the latitude of the observation site increases, the gap between winter and summer becomes larger and larger, so at the equator there is no difference between winter and summer. Beyond the Arctic Circle, solar radiation is very high in summer and very low in winter. This shapes the climate on Earth. In addition, periodic changes in the eccentricity of the Earth's orbit can lead to the emergence of different geological eras: for example,

Solar radiation

Solar radiation

electromagnetic radiation emanating from the Sun and entering the earth's atmosphere. Solar radiation wavelengths are concentrated in the range from 0.17 to 4 µm with a max. at a wavelength of 0.475 µm. OK. 48% energy solar radiation falls on the visible part of the spectrum (wavelength from 0.4 to 0.76 microns), 45% - in the infrared (more than 0.76 microns), and 7% - in the ultraviolet (less than 0.4 microns). Solar radiation is the main source of energy for processes in the atmosphere, ocean, biosphere, etc. It is measured in units of energy per unit area per unit time, for example. W/m². Solar radiation at the upper boundary of the atmosphere on Wednesday. the distance of the Earth from the Sun is called solar constant and amounts to approx. 1382 W/m². As solar radiation passes through the earth's atmosphere, it changes in intensity and spectral composition due to absorption and scattering on air particles, gas impurities and aerosol. At the Earth's surface, the spectrum of solar radiation is limited to 0.29–2.0 μm, and the intensity is significantly reduced depending on the content of impurities, altitude and cloud cover. Direct radiation, weakened when passing through the atmosphere, as well as scattered radiation, formed when the direct line is scattered in the atmosphere, reaches the earth's surface. Part of the direct solar radiation is reflected from the earth's surface and clouds and goes into space; scattered radiation also partially escapes into space. The rest of the solar radiation is mainly turns into heat, heating the earth's surface and partly the air. Solar radiation, i.e., is one of the main. components of the radiation balance.

Geography. Modern illustrated encyclopedia. - M.: Rosman. Edited by prof. A. P. Gorkina. 2006 .


See what “solar radiation” is in other dictionaries:

    Electromagnetic and corpuscular radiation of the Sun. Electromagnetic radiation covers the wavelength range from gamma radiation to radio waves, its energy maximum falls on the visible part of the spectrum. Corpuscular component of the solar... ... Big Encyclopedic Dictionary

    solar radiation- The total flow of electromagnetic radiation emitted by the Sun and falling on the Earth... Dictionary of Geography

    This term has other meanings, see Radiation (meanings). This article lacks links to sources of information. Information must be verifiable, otherwise it may be called into question... Wikipedia

    All surface processes globe, whatever they are, have solar energy as their source. Are purely mechanical processes being studied, chemical processes in air, water, soil, physiological processes or whatever... ... Encyclopedic Dictionary F.A. Brockhaus and I.A. Ephron

    Electromagnetic and corpuscular radiation of the Sun. Electromagnetic radiation covers a range of wavelengths from gamma radiation to radio waves, its energy maximum falls in the visible part of the spectrum. Corpuscular component of the solar... ... Encyclopedic Dictionary

    solar radiation- Saulės spinduliuotė statusas T sritis fizika atitikmenys: engl. solar radiation vok. Sonnenstrahlung, f rus. solar radiation, n; solar radiation, f; solar radiation, n pranc. rayonnement solaire, m … Fizikos terminų žodynas

    solar radiation- Saulės spinduliuotė statusas T sritis ekologija ir aplinkotyra apibrėžtis Saulės atmosferos elektromagnetinė (infraraudonoji 0.76 nm sudaro 45%, matomoji 0.38–0.76 nm – 48%, ultravioletinė 0.38 nm – 7 %) šviesos, radijo bangų, gama kvantų ir… … Ekologijos terminų aiškinamasis žodynas

    Radiation from the Sun of electromagnetic and corpuscular nature. S. r. the main source of energy for most processes occurring on Earth. Corpuscular S. r. consists mainly of protons, which have velocities of 300–1500 near the Earth… … Great Soviet Encyclopedia

    Email mag. and corpuscular radiation from the Sun. Email mag. radiation covers a range of wavelengths from gamma radiation to radio waves, its energy. the maximum falls on the visible part of the spectrum. Corpuscular component of S. r. consists of ch. arr. from… … Natural science. Encyclopedic Dictionary

    direct solar radiation- Solar radiation coming directly from the solar disk... Dictionary of Geography

Books

  • Solar radiation and climate of the Earth, Fedorov Valery Mikhailovich. The book presents the results of studies of variations in Earth's insolation associated with celestial-mechanical processes. Low-frequency and high-frequency changes in solar climate are analyzed...

The intensity of sunlight that reaches the earth varies depending on the time of day, year, location and weather conditions. Total quantity energy calculated per day or per year is called irradiation (or else “incoming solar radiation”) and shows how powerful the solar radiation was. Irradiation is measured in W*h/m² per day, or other period.

The intensity of solar radiation in free space at a distance equal to the average distance between the Earth and the Sun is called the solar constant. Its value is 1353 W/m². As sunlight passes through the atmosphere, it is attenuated primarily by absorption infrared radiation water vapor, ultraviolet radiation— ozone and radiation scattering by atmospheric dust particles and aerosols. Indicator atmospheric influence the intensity of solar radiation reaching the earth's surface is called “air mass” (AM). AM is defined as the secant of the angle between the Sun and zenith.

Figure 1 shows the spectral distribution of solar radiation intensity in different conditions. The upper curve (AM0) corresponds to the solar spectrum beyond earth's atmosphere(for example, on board spaceship), i.e. at zero air mass. It is approximated by the distribution of the radiation intensity of a completely black body at a temperature of 5800 K. Curves AM1 and AM2 illustrate the spectral distribution of solar radiation on the Earth's surface when the Sun is at its zenith and at an angle between the Sun and the zenith of 60°, respectively. In this case, the total radiation power is approximately 925 and 691 W/m², respectively. The average radiation intensity on Earth approximately coincides with the radiation intensity at AM = 1.5 (the Sun is at an angle of 45° to the horizon).

Near the surface of the Earth you can take average value solar radiation intensity 635 W/m². On a very clear sunny day, this value ranges from 950 W/m² to 1220 W/m². The average value is approximately 1000 W/m². Example: Total radiation intensity in Zurich (47°30′N, 400 m above sea level) on a surface perpendicular to the radiation: May 1 12:00 1080 W/m²; December 21 12:00 930 W/m² .

To simplify the calculation of solar energy arrival, it is usually expressed in hours of sunshine with an intensity of 1000 W/m². Those. 1 hour corresponds to the arrival of solar radiation of 1000 W*h/m². This roughly corresponds to the period when the sun shines in the summer in the middle of a sunny, cloudless day on a surface perpendicular to the sun's rays.

Example
Bright sun shines with an intensity of 1000 W/m² onto a surface perpendicular to the sun's rays. In 1 hour, 1 kWh of energy drops per 1 m² (energy is equal to power times time). Similarly, an average solar radiation arrival of 5 kWh/m² during the day corresponds to 5 peak sunshine hours per day. Don't confuse peak hours with actual duration daylight hours. During the day, the sun shines with different intensities, but in total it gives the same amount of energy as if it shone for 5 hours at maximum intensity. It is the peak hours of sunshine that are used in the calculations of solar energy installations.

The arrival of solar radiation varies throughout the day and from place to place, especially in mountainous areas. Irradiation varies on average from 1000 kWh/m² per year for Northern European countries, to 2000-2500 kWh/m² per year for deserts. Weather conditions and the declination of the sun (which depends on the latitude of the area) also leads to differences in the arrival of solar radiation.

In Russia, contrary to popular belief, there are many places where it is profitable to convert solar energy into electricity using. Below is a map of solar energy resources in Russia. As you can see, in most of Russia it can be successfully used in seasonal mode, and in areas with more than 2000 hours of sunshine per year - all year round. Naturally, in winter period energy production from solar panels is significantly reduced, but still the cost of electricity is from solar power plant remains significantly lower than from a diesel or gasoline generator.

It is especially advantageous to use it where there are no centralized electrical networks and the energy supply is provided by diesel generators. And there are a lot of such areas in Russia.

Moreover, even where networks exist, the use of solar panels operating in parallel with the network can significantly reduce energy costs. Given the current trend towards increasing tariffs of natural energy monopolies in Russia, installations solar panels becomes a smart investment.

General hygiene. Solar radiation and its hygienic significance.

By solar radiation we mean the entire flux of radiation emitted by the Sun, which is electromagnetic oscillations of various wavelengths. From a hygienic point of view, the optical part of sunlight, which occupies the range from 280-2800 nm, is of particular interest. Longer waves are radio waves, shorter ones are gamma rays, ionizing radiation do not reach the Earth's surface because they are retained in the upper layers of the atmosphere, in the ozone layer in particular. Ozone is distributed throughout the atmosphere, but at an altitude of about 35 km it forms the ozone layer.

The intensity of solar radiation depends primarily on the height of the sun above the horizon. If the sun is at its zenith, then the path taken by the sun's rays will be much shorter than their path if the sun is at the horizon. By increasing the path, the intensity of solar radiation changes. The intensity of solar radiation also depends on the angle at which the sun's rays fall, and the illuminated area also depends on this (as the angle of incidence increases, the area of ​​illumination increases). Thus, the same solar radiation falls on a larger surface, so the intensity decreases. The intensity of solar radiation depends on the mass of air through which the sun's rays pass. The intensity of solar radiation in the mountains will be higher than above sea level, because the layer of air through which the sun's rays pass will be less than above sea level. Special significance represents the influence of the state of the atmosphere and its pollution on the intensity of solar radiation. If the atmosphere is polluted, then the intensity of solar radiation decreases (in the city, the intensity of solar radiation is on average 12% less than in rural areas). The voltage of solar radiation has a daily and annual background, that is, the voltage of solar radiation changes throughout the day, and also depends on the time of year. The highest intensity of solar radiation is observed in summer, the lowest in winter. In terms of its biological effect, solar radiation is heterogeneous: it turns out that each wavelength has an different action on the human body. In this regard, the solar spectrum is conventionally divided into 3 sections:

1. ultraviolet rays, from 280 to 400 nm

2. visible spectrum from 400 to 760 nm

3. infrared rays from 760 to 2800 nm.

With daily and annual solar radiation, the composition and intensity of individual spectra undergo changes. The rays of the UV spectrum undergo the greatest changes.

We estimate the intensity of solar radiation based on the so-called solar constant. The solar constant is the amount of solar energy received per unit time per unit area located at the upper boundary of the atmosphere at right angles to the sun's rays at the average distance of the Earth from the Sun. This solar constant was measured by satellite and is equal to 1.94 calories/cm 2

per minute Passing through the atmosphere, the sun's rays are significantly weakened - scattered, reflected, absorbed. On average, with a clean atmosphere on the Earth's surface, the intensity of solar radiation is 1.43 - 1.53 calories/cm2 per minute.

Voltage sun rays at noon in May in Yalta 1.33, in Moscow 1.28, in Irkutsk 1.30, in Tashkent 1.34.

Biological significance of the visible part of the spectrum.

The visible part of the spectrum is a specific irritant of the organ of vision. Light is a necessary condition for the functioning of the eye, the most subtle and sensitive sense organ. Light provides approximately 80% of information about the outside world. This is the specific effect of visible light, but also the general biological effect of visible light: it stimulates the body’s vital activity, enhances metabolism, improves overall well-being, affects the psycho-emotional sphere, and increases performance. Light makes you healthier environment. With a lack of natural light, changes occur in the organ of vision. Fatigue sets in quickly, performance decreases, and work-related injuries increase. The body is affected not only by illumination, but also different colors have different effects on the psycho-emotional state. The best performance indicators were obtained with the preparation under yellow and white lighting. Psychophysiologically, colors act opposite to each other. In this regard, 2 groups of colors were formed:
1) warm colors - yellow, orange, red. 2) cold tones - blue, blue, violet. Cold and warm tones have different physiological effects on the body. Warm tones increase muscle tension, increase blood pressure, and increase the breathing rate. Cold tones, on the contrary, lower blood pressure and slow down the rhythm of the heart and breathing. This is often used in practice: for patients with high temperature Wards painted purple are most suitable; dark ocher improves the well-being of patients with low blood pressure. Red color increases appetite. Moreover, the effectiveness of the drug can be increased by changing the color of the tablet. Patients suffering from depressive disorders were given the same medicine in tablets of different colors: red, yellow, green. Treatment with yellow tablets brought the best results.

Color is used as a carrier of coded information, for example in production to indicate danger. There is a generally accepted standard for signal identification colors: green - water, red - steam, yellow - gas, orange - acids, purple - alkalis, brown - flammable liquids and oils, blue - air, gray - other.

From a hygienic point of view, the assessment of the visible part of the spectrum is carried out according to the following indicators: natural and artificial lighting are assessed separately. Natural lighting is assessed according to 2 groups of indicators: physical and lighting. The first group includes:

1. light coefficient -- characterizes the ratio of the area of ​​the glazed surface of the windows to the floor area.

2. Angle of incidence - characterizes the angle at which the rays fall. According to the norm, the minimum angle of incidence should be at least 270.

3. The angle of the hole - characterizes the illumination by heavenly light (must be at least 50). On the first floors of Leningrad houses - wells, this angle is virtually absent.

4. The depth of the room is the ratio of the distance from the top edge of the window to the floor to the depth of the room (the distance from the outer to the inner wall).

Lighting indicators are indicators determined using a device - a lux meter. Absolute and relative illumination is measured. Absolute illumination is the illumination on the street. Illuminance coefficient (KEO) is defined as the ratio of relative illuminance (measured as the ratio of relative illuminance (measured in a room) to absolute, expressed in %. Illumination in a room is measured at the workplace. The principle of operation of a lux meter is that the device has a sensitive photocell (selenium - since selenium is close in sensitivity to the human eye). The approximate illumination on the street can be determined using a light climate graph.

To evaluate artificial lighting of premises, brightness, lack of pulsation, color, etc. are important.

Infrared rays. The main biological effect of these rays is thermal, and this effect also depends on the wavelength. Short rays carry more energy, so they penetrate deeper and have a strong thermal effect. The long section exerts its thermal effect on the surface. This is used in physiotherapy to warm up areas at different depths.

In order to measure infrared rays, there is a device - an actinometer. Infrared radiation is measured in calories per cm2\min. The adverse effects of infrared rays are observed in hot shops, where they can lead to occupational diseases - cataracts (clouding of the lens). Cataracts are caused by short infrared rays. A preventative measure is the use of protective glasses and protective clothing.

Features of the impact of infrared rays on the skin: burns occur - erythema. It occurs due to thermal expansion of blood vessels. Its peculiarity is that it has different boundaries and appears immediately.

Due to the action of infrared rays, 2 conditions of the body can occur: heatstroke and sunstroke. Sunstroke is the result of direct exposure to sunlight on the human body, mainly with damage to the central nervous system. Sunstroke affects those who spend many hours in a row under the scorching rays of the sun with their heads uncovered. The meninges are warmed up.

Heat stroke occurs due to overheating of the body. It can happen to those who perform heavy physical work in a hot room or in hot weather. Heat strokes were especially common among our military personnel in Afghanistan.

In addition to actinometers for measuring infrared radiation, there are various types of pyramidometers. The basis of this action is the absorption of radiant energy by the black body. The receptive layer consists of blackened and white plates, which, depending on infrared radiation, heat up differently. A current is generated on the thermopile and the intensity of infrared radiation is recorded. Since the intensity of infrared radiation is important in production conditions, there are standards for infrared radiation for hot shops in order to avoid adverse effects on the human body, for example, in a pipe-rolling shop the bench is 1.26 - 7.56, iron smelting 12.25. Radiation levels exceeding 3.7 are considered significant and require preventive measures - the use of protective screens, water curtains, and special clothing.

Ultraviolet rays (UV).

This is the most biologically active part of the solar spectrum. It is also heterogeneous. In this regard, a distinction is made between long-wave and short-wave UV. UV promotes tanning. When UV enters the skin, 2 groups of substances are formed in it: 1) specific substances, these include vitamin D, 2) non-specific substances - histamine, acetylcholine, adenosine, that is, these are products of protein breakdown. The tanning or erythema effect comes down to a photochemical effect - histamine and other biologically active substances contribute to vasodilation. The peculiarity of this erythema is that it does not appear immediately. Erythema has clearly defined boundaries. Ultraviolet erythema always leads to a more or less pronounced tan, depending on the amount of pigment in the skin. The mechanism of tanning action has not yet been sufficiently studied. It is believed that first erythema occurs, nonspecific substances such as histamine are released, the body converts the products of tissue breakdown into melanin, as a result of which the skin acquires a peculiar shade. Tanning, therefore, is a test of the body's protective properties (a sick person does not tan, tans slowly).

The most favorable tanning occurs under the influence of UV rays with a wavelength of approximately 320 nm, that is, when exposed to the long-wavelength part of the UV spectrum. In the south, short-wave UFLs predominate, and in the north, long-wave UFLs predominate. Short-wavelength rays are most susceptible to scattering. And dispersion occurs best in a clean atmosphere and in the northern region. Thus, the most useful tan in the north is longer, darker. UFL are a very powerful factor in the prevention of rickets. With a lack of UVB, rickets develops in children, and osteoporosis or osteomalacia in adults. This is usually encountered in the Far North or among groups of workers working underground. In the Leningrad region, from mid-November to mid-February, the UV part of the spectrum is practically absent, which contributes to the development of solar starvation. To prevent sunburn, artificial tanning is used. Light starvation is a long-term absence of the UV spectrum. When exposed to UV in the air, ozone is formed, the concentration of which must be controlled.

UV rays have a bactericidal effect. It is used to disinfect large wards, food products, water.

The intensity of UV radiation is determined by the photochemical method by the amount of oxalic acid decomposed under the influence of UV in quartz test tubes (ordinary glass does not transmit UV light). The intensity of UV radiation is also determined by an ultraviolet meter. For medical purposes, ultraviolet radiation is measured in biodoses.