172 lines
9.1 KiB
Plaintext
172 lines
9.1 KiB
Plaintext
# translation of kstars_flux.po to
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# Copyright (C) 2005 Free Software Foundation, Inc.
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#
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# Nick Shaforostoff <shafff@ukr.net>, 2005.
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# Alexandr Gudulin <sagodphp@gmail.com>, 2010.
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msgid ""
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msgstr ""
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"Project-Id-Version: kstars_flux\n"
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"Report-Msgid-Bugs-To: https://bugs.kde.org\n"
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"POT-Creation-Date: 2021-03-28 16:23+0000\n"
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"PO-Revision-Date: 2010-11-26 16:13+0300\n"
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"Last-Translator: Alexandr Gudulin <sagodphp@gmail.com>\n"
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"Language-Team: Russian <kde-russian@lists.kde.ru>\n"
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"Language: ru\n"
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"MIME-Version: 1.0\n"
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"Content-Type: text/plain; charset=UTF-8\n"
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"Content-Transfer-Encoding: 8bit\n"
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"X-Generator: Lokalize 1.1\n"
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"Plural-Forms: nplurals=4; plural=n==1 ? 3 : n%10==1 && n%100!=11 ? 0 : n"
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"%10>=2 && n%10<=4 && (n%100<10 || n%100>=20) ? 1 : 2;\n"
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"X-Environment: kde\n"
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"X-Accelerator-Marker: \n"
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"X-Text-Markup: docbook4\n"
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#. Tag: author
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#: flux.docbook:5
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#, no-c-format
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msgid "<firstname>Jasem</firstname> <surname>Mutlaq</surname>"
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msgstr "<firstname>Jasem</firstname> <surname>Mutlaq</surname>"
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#. Tag: title
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#: flux.docbook:13
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#, no-c-format
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msgid "<title>Flux</title>"
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msgstr "<title>Поток</title>"
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#. Tag: primary
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#: flux.docbook:14
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#, no-c-format
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msgid "<primary>Flux</primary>"
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msgstr "<primary>Поток</primary>"
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#. Tag: seealso
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#: flux.docbook:15
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#, no-c-format
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msgid "Luminosity"
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msgstr "Светимость"
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#. Tag: para
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#: flux.docbook:18
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#, no-c-format
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msgid ""
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"The <firstterm>flux</firstterm> is the amount of energy that passes through "
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"a unit area each second."
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msgstr ""
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"<firstterm>Поток</firstterm> - сумма всей энергии, проходящей через "
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"единичную площадь в единицу времени."
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#. Tag: para
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#: flux.docbook:22
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#, no-c-format
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msgid ""
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"Astronomers use flux to denote the apparent brightness of a celestial body. "
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"The apparent brightness is defined as the amount of light received from a "
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"star above the earth atmosphere passing through a unit area each second. "
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"Therefore, the apparent brightness is simply the flux we receive from a star."
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msgstr ""
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"Астрономы используют поток, чтобы описать видимую светимость небесного тела. "
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"Видимая светимость определяется как сумма испущенного звездой света, "
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"прошедшего через единичную площадку, расположенную за атмосферой, в единицу "
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"времени. Поэтому видимая светимость — это просто поток света, который "
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"мы получаем со звезды."
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#. Tag: para
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#: flux.docbook:27
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#, fuzzy, no-c-format
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#| msgid ""
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#| "The flux measures the <emphasis>rate of flow</emphasis> of energy that "
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#| "passes through each cm^2 (or any unit area) of an object's surface each "
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#| "second. The detected flux depends on the distance from the source that "
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#| "radiates the energy. This is because the energy has to spread over a "
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#| "volume of space before it reaches us. Let us assume that we have an "
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#| "imaginary balloon that encloses a star. Each dot on the balloon "
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#| "represents a unit of energy emitted from the star. Initially, the dots in "
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#| "an area of one cm^2 are in close proximity to each other and the flux "
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#| "(energy emitted per square centimeter per second) is high. After a "
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#| "distance d, the volume and surface area of the balloon increased causing "
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#| "the dots to <emphasis>spread away</emphasis> from each. Consequently, the "
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#| "number of dots (or energy) enclosed in one cm^2 has decreased as "
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#| "illustrated in Figure 1."
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msgid ""
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"The flux measures the <emphasis>rate of flow</emphasis> of energy that "
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"passes through each cm<superscript>2</superscript> (or any unit area) of an "
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"object's surface each second. The detected flux depends on the distance from "
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"the source that radiates the energy. This is because the energy has to "
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"spread over a volume of space before it reaches us. Let us assume that we "
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"have an imaginary balloon that encloses a star. Each dot on the balloon "
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"represents a unit of energy emitted from the star. Initially, the dots in an "
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"area of one cm<superscript>2</superscript> are in close proximity to each "
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"other and the flux (energy emitted per square centimeter per second) is "
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"high. After a distance d, the volume and surface area of the balloon "
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"increased causing the dots to <emphasis>spread away</emphasis> from each. "
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"Consequently, the number of dots (or energy) enclosed in one "
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"cm<superscript>2</superscript> has decreased as illustrated in Figure 1."
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msgstr ""
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"Поток измеряется как <emphasis>скорость потока</emphasis> энергии, которая "
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"каждую секунду уходит с каждого см^2 (или другой единицы площади) "
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"поверхности объекта. Величина потока зависит от расстояния, на котором "
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"располагается источник. Это происходит потому, что энергия рассеивается в "
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"пространстве, прежде чем достигнет наблюдателя. Допустим, что мы окружили "
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"звезду оболочкой. Каждая точка оболочки поглощает энергию, излучённую "
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"звездой. Сперва, точки на площадке в 2 см^2 очень близко расположены и, "
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"таким образом, поток (энергия, проходящая через один квадратный сантиметр в "
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"секунду) высокий. На расстоянии d объём и площадь поверхности оболочки "
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"увеличиваются, и точки <emphasis>разбегаются</emphasis> в разные стороны. "
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"Следовательно, число точек (или энергии), попадающих на один см^2 "
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"уменьшается, как это показано на рис. 1."
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#. Tag: phrase
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#: flux.docbook:40
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#, no-c-format
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msgid "Figure 1"
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msgstr "Рисунок 1"
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#. Tag: para
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#: flux.docbook:44
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#, fuzzy, no-c-format
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#| msgid ""
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#| "The flux is inversely proportional to distance by a simple r^2 relation. "
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#| "Therefore, if the distance is doubled, we receive 1/2^2 or 1/4th of the "
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#| "original flux. From a fundamental standpoint, the flux is the <link "
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#| "linkend=\"ai-luminosity\">luminosity</link> per unit area:"
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msgid ""
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"The flux is inversely proportional to distance by a simple r<superscript>2</"
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"superscript> relation. Therefore, if the distance is doubled, we receive "
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"1/2<superscript>2</superscript> or 1/4th of the original flux. From a "
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"fundamental standpoint, the flux is the <link linkend=\"ai-luminosity"
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"\">luminosity</link> per unit area:"
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msgstr ""
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"Поток обратно пропорционален квадрату расстояния (r^2). Таким образом, если "
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"расстояние увеличивается в два раза, то мы получим (1/2)^2 = 1/4 от "
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"первоначального потока. С фундаментальной точки зрения, поток — это "
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"<link linkend=\"ai-luminosity\">Светимость</link> на единицу площади:"
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#. Tag: para
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#: flux.docbook:55
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#, fuzzy, no-c-format
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#| msgid ""
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#| "where (4 * PI * R^2) is the surface area of a sphere (or a balloon!) with "
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#| "a radius R. Flux is measured in Watts/m^2/s or as commonly used by "
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#| "astronomers: Ergs/cm^2/s. For example, the luminosity of the sun is L = "
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#| "3.90 * 10^26 W. That is, in one second the sun radiates 3.90 * 10^26 "
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#| "joules of energy into space. Thus, the flux we receive passing through "
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#| "one square centimeter from the sun at a distance of one AU (1.496 * 10^13 "
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#| "cm) is:"
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msgid ""
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"where (4 * π * R<superscript>2</superscript>) is the surface area of a "
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"sphere (or a balloon!) with a radius R. Flux is measured in Watts/"
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"m<superscript>2</superscript>/s or as commonly used by astronomers: Ergs/"
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"cm<superscript>2</superscript>/s. For example, the luminosity of the sun is "
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"L = 3.90 * 10<superscript>26</superscript> W. That is, in one second the sun "
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"radiates 3.90 * 10<superscript>26</superscript> joules of energy into space. "
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"Thus, the flux we receive passing through one square centimeter from the sun "
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"at a distance of one AU (1.496 * 10<superscript>13</superscript> cm) is:"
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msgstr ""
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"где (4 * PI * R^2) — площадь поверхности сферы (нашей оболочки) "
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"радиуса R. Поток измеряется в Вт/(с * см^2). Например, светимость Солнца L = "
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"3.90 * 10^26 Вт. Это значит, что Солнце излучает 3.90 * 10^26 джоулей "
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"энергии каждую секунду в космос. Соответственно, поток энергии от солнца, "
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"проходящий через один см^2, с расстояния одной а.е. (астрономической единицы "
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"= 1.496 * 10^13 см) равен:"
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