{"id":6709,"date":"2024-11-23T20:48:39","date_gmt":"2024-11-23T20:48:39","guid":{"rendered":"https:\/\/workhouse.sweetdishy.com\/?p=6709"},"modified":"2024-11-23T20:48:40","modified_gmt":"2024-11-23T20:48:40","slug":"reckoning-of-time","status":"publish","type":"post","link":"https:\/\/workhouse.sweetdishy.com\/index.php\/2024\/11\/23\/reckoning-of-time\/","title":{"rendered":"Reckoning of time"},"content":{"rendered":"\n<p id=\"P0025\">In solar energy calculations, apparent solar time (AST) must be used to express the time of day. AST is based on the apparent angular motion of the sun across the sky. The time when the sun crosses the meridian of the observer is the local solar noon. It usually does not coincide with the 12:00 o\u2019clock time of a locality. To convert the local standard time (LST) to AST, two corrections are applied; the equation of time (ET) and longitude correction. These are analyzed next.<\/p>\n\n\n\n<h3 class=\"wp-block-heading\" id=\"CESECTITLE0025\">Equation of time<\/h3>\n\n\n\n<p id=\"P0030\">Due to factors associated with the earth\u2019s orbit around the sun, the earth\u2019s orbital velocity varies throughout the year, so the AST varies slightly from the mean time kept by a clock running at a uniform rate. The variation is called the&nbsp;<em>equation of time<\/em>&nbsp;(ET). The ET arises because the length of a day, that is, the time required by the earth to complete one revolution about its own axis with respect to the sun, is not uniform throughout the year. Over the year, the average length of a day is 24&nbsp;h; however, the length of a day varies due to the eccentricity of the earth\u2019s orbit and the tilt of the earth\u2019s axis from the normal plane of its orbit. Due to the ellipticity of the orbit, the earth is closer to the sun on January 3 and furthest from the sun on July 4. Therefore the earth\u2019s orbiting speed is faster than its average speed for half the year (from about October through March) and slower than its average speed for the remaining half of the year (from about April through September).<\/p>\n\n\n\n<p id=\"P0035\">The values of the ET as a function of the day of the year (<em>N<\/em>) can be obtained approximately from the following equations:<\/p>\n\n\n\n<p id=\"FD1\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/learning.oreilly.com\/api\/v2\/epubs\/urn:orm:book:9780123972705\/files\/images\/F000029si1.png\" alt=\"image\" width=\"346\" height=\"16\"><strong>(2.1)<\/strong><\/p>\n\n\n\n<p>and<\/p>\n\n\n\n<p id=\"FD2\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/learning.oreilly.com\/api\/v2\/epubs\/urn:orm:book:9780123972705\/files\/images\/F000029si2.png\" alt=\"image\" width=\"124\" height=\"34\"><strong>(2.2)<\/strong><\/p>\n\n\n\n<p id=\"P0040\">A graphical representation of\u00a0Eq (2.1)\u00a0is shown in\u00a0Figure 2.2, from which the ET can be obtained directly.<\/p>\n\n\n\n<figure class=\"wp-block-image\"><img decoding=\"async\" src=\"https:\/\/learning.oreilly.com\/api\/v2\/epubs\/urn:orm:book:9780123972705\/files\/images\/F000029f02-02-9780123972705.jpg\" alt=\"image\"\/><\/figure>\n\n\n\n<p><strong>FIGURE 2.2<\/strong>&nbsp;<a><\/a>Equation of time.<\/p>\n\n\n\n<h3 class=\"wp-block-heading\" id=\"CESECTITLE0030\">Longitude correction<\/h3>\n\n\n\n<p id=\"P0045\">The standard clock time is reckoned from a selected meridian near the center of a time zone or from the standard meridian, the Greenwich, which is at longitude of 0\u00b0. Since the sun takes 4&nbsp;min to transverse<a><\/a>&nbsp;1\u00b0 of longitude, a longitude correction term of 4\u00d7 (Standard longitude [SL]&nbsp;\u2212&nbsp;Local longitude [LL]) should be either added or subtracted to the standard clock time of the locality. This correction is constant for a particular longitude, and the following rule must be followed with respect to sign convention. If the location is east of the standard meridian, the correction is added to the clock time. If the location is west, it is subtracted. The general equation for calculating the AST is:<\/p>\n\n\n\n<p id=\"FD3\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/learning.oreilly.com\/api\/v2\/epubs\/urn:orm:book:9780123972705\/files\/images\/F000029si3.png\" alt=\"image\" width=\"254\" height=\"16\"><strong>(2.3)<\/strong><\/p>\n\n\n\n<p>where<a><\/a><\/p>\n\n\n\n<p id=\"U0010\"><a><\/a>LST&nbsp;=&nbsp;local standard time.<\/p>\n\n\n\n<p id=\"U0015\"><a><\/a>ET&nbsp;=&nbsp;equation of time.<\/p>\n\n\n\n<p id=\"U0020\"><a><\/a>SL&nbsp;=&nbsp;standard longitude.<\/p>\n\n\n\n<p id=\"U0025\"><a><\/a>LL&nbsp;=&nbsp;local longitude.<\/p>\n\n\n\n<p id=\"U0030\"><a><\/a>DS&nbsp;=&nbsp;daylight saving (it is either 0 or 60&nbsp;min).<\/p>\n\n\n\n<p id=\"P0075\">If a location is east of Greenwich, the sign of\u00a0Eq (2.3)\u00a0is minus (\u2212), and if it is west, the sign is plus (+). If a daylight saving time is used, this must be subtracted from the LST. The term DS depends on whether daylight saving time is in operation (usually from end of March to end of October) or not. This term is usually ignored from this equation and considered only if the estimation is within the DS period.<\/p>\n\n\n\n<p>EXAMPLE 2.1<\/p>\n\n\n\n<p id=\"P0080\">Find the equation of AST for the city of Nicosia, Cyprus.<\/p>\n\n\n\n<p id=\"BOXSECTITLE0010\">Solution<\/p>\n\n\n\n<p id=\"P0085\">For the locality of Cyprus, the SL is 30\u00b0E. The city of Nicosia is at a LL of 33.33\u00b0 east of Greenwich. Therefore, the longitude correction is \u22124 \u00d7 (30\u201333.33)\u00a0=\u00a0+13.32\u00a0min. Thus,\u00a0Eq (2.3)\u00a0can be written as:<\/p>\n\n\n\n<figure class=\"wp-block-image is-resized\"><img decoding=\"async\" src=\"https:\/\/learning.oreilly.com\/api\/v2\/epubs\/urn:orm:book:9780123972705\/files\/images\/F000029si4.png\" alt=\"image\" style=\"width:486px;height:auto\"\/><\/figure>\n\n\n\n<h2 class=\"wp-block-heading\" id=\"CESECTITLE0035\"><\/h2>\n","protected":false},"excerpt":{"rendered":"<p>In solar energy calculations, apparent solar time (AST) must be used to express the time of day. AST is based on the apparent angular motion of the sun across the sky. The time when the sun crosses the meridian of the observer is the local solar noon. It usually does not coincide with the 12:00 [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":6687,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-6709","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-blog"],"jetpack_featured_media_url":"https:\/\/workhouse.sweetdishy.com\/wp-content\/uploads\/2024\/11\/environmentalism.png","_links":{"self":[{"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/posts\/6709","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/comments?post=6709"}],"version-history":[{"count":1,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/posts\/6709\/revisions"}],"predecessor-version":[{"id":6710,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/posts\/6709\/revisions\/6710"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/media\/6687"}],"wp:attachment":[{"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/media?parent=6709"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/categories?post=6709"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/workhouse.sweetdishy.com\/index.php\/wp-json\/wp\/v2\/tags?post=6709"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}