<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JAMP</journal-id><journal-title-group><journal-title>Journal of Applied Mathematics and Physics</journal-title></journal-title-group><issn pub-type="epub">2327-4352</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jamp.2015.35064</article-id><article-id pub-id-type="publisher-id">JAMP-56537</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  A New Method of Measurement of the True Temperature and Emissivity of Non-Black Body Using One Component of Wien’s Spectrum of Thermal Radiation
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>.</surname><given-names>Ya. Svet</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Joint Institute for High Temperatures of the Russian Academy of Sciences, Moscow, Russian Federation</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>vsvetd@mail.ru</email></corresp></author-notes><pub-date pub-type="epub"><day>11</day><month>05</month><year>2015</year></pub-date><volume>03</volume><issue>05</issue><fpage>524</fpage><lpage>529</lpage><history><date date-type="received"><day>11</day>	<month>March</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>20</month>	<year>May</year>	</date><date date-type="accepted"><day>22</day>	<month>May</month>	<year>2015</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  It is shown that the measurement of only one component of the Wein’s spectrum of thermal radiation in range 
  λT ≤ 3000 (
  &amp;deg
  ;C μm) is sufficient to estimate the true temperature and spectral emissivity of the selected component with sufficient accuracy, although more than one hundred years this statement was considered as incorrect. The proposed method is based on the formation of the linear dependence of the logarithm of the emissivity of not real wavelengths and artificially generated “virtual” spectral components.
 
</p></abstract><kwd-group><kwd>True Temperature</kwd><kwd> Spectral Emissivity</kwd><kwd> Wein’s Law</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Since the discovery of Wien’s exponential law of thermal radiation the concepts of emissivity and black-body factor were firmly established in physics. And measuring of the true temperature and emissivity became a problem “idem per idem” (the same through the same): To measure the true temperature it is necessary to know the emissivity and vice versa. A close look at this problem (on which the author spent more than sixty years) showed that its solution exists. Moreover, it was found that the measurement of any of the spectral components of radiation following to an exponential Wien’s law is enough to determine the value of true temperature and spectral emissivity of this component. Below we shall describe the proposed method which implements this statement<sup>1</sup>.</p></sec><sec id="s2"><title>2. Method</title><p>The method is based on the principle of double spectral ratio, based on the linear dependence of the logarithm of the emissivity for three selected components of the spectrum of thermal radiation, proposed in [<xref ref-type="bibr" rid="scirp.56537-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.56537-ref2">2</xref>] , which is widely represented in the literature [<xref ref-type="bibr" rid="scirp.56537-ref3">3</xref>] . However, application of this principle is limited by the requirement on the linearity a priory. This takes place practically only for wavelengths with very closed spacing, which in turn leads to increasing of the value of equivalent wavelength, i.e. to an unacceptable increasing error of measured temperature.</p><p>In proposed method a linear dependence of the three components, two of which are “virtual”, is generated artificially relative the selected spectral component and the requirement of proximity of wavelengths is eliminated.</p><p>Thus, only one spectral component is extracted from the Wien’s spectrum that is logarithmic,</p><disp-formula id="scirp.56537-formula572"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x5.png"  xlink:type="simple"/></disp-formula><p>where:</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x6.png" xlink:type="simple"/></inline-formula>―wavelength;</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x7.png" xlink:type="simple"/></inline-formula>―temperature in ˚C;</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x8.png" xlink:type="simple"/></inline-formula>―spectral emissivity at wavelength λ<sub>1</sub>;</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x9.png" xlink:type="simple"/></inline-formula>―14,388 μm/˚C―second pyrometer constant.</p><p>The value of the second pyrometer signal is determining by multiplying <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x10.png" xlink:type="simple"/></inline-formula> on the ratio <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x11.png" xlink:type="simple"/></inline-formula> which is proportional to a “virtual” spectral component at a selected wavelength<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x12.png" xlink:type="simple"/></inline-formula>, more or less than<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x13.png" xlink:type="simple"/></inline-formula>. For exam- ple, let’s choose <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x14.png" xlink:type="simple"/></inline-formula><sub> </sub></p><disp-formula id="scirp.56537-formula573"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x15.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x16.png" xlink:type="simple"/></inline-formula></p><p>Further, let’s form a third pyrometer signal proportional to the “virtual” component with a wavelength<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x17.png" xlink:type="simple"/></inline-formula>, which, for example, defined by the half-sum of inverse values of wavelengths</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x18.png" xlink:type="simple"/></inline-formula>, i.e.</p><disp-formula id="scirp.56537-formula574"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x19.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.56537-formula575"><label>(4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x20.png"  xlink:type="simple"/></disp-formula><p>Thus</p><disp-formula id="scirp.56537-formula576"><label>(5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x21.png"  xlink:type="simple"/></disp-formula><p>Having these three pyrometer signals<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x23.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x24.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x23.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x24.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x25.png" xlink:type="simple"/></inline-formula> we can form a linear dependence of the logarithm of the emissivity versus wavelength.</p><p>Graphically this is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>, where the emissivity’s of these three signals marked by ordinates<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x26.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x27.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x26.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x28.png" xlink:type="simple"/></inline-formula> and, as it is seen (dotted lines) they form a linear polyline of emissivity versus wave-</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Emissivity versus wavelength</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/7-1720274x29.png"/></fig><p>length.</p><p>For the linearization of this dependence and formation of a linear dependence (this is a straight line <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x30.png" xlink:type="simple"/></inline-formula> on <xref ref-type="fig" rid="fig1">Figure 1</xref>) we shall use expression from [<xref ref-type="bibr" rid="scirp.56537-ref4">4</xref>] .</p><p>This formula determines the value of the true temperature at known a’priory linearity of logarithm of emis- sivity from the wavelength and has the form:</p><disp-formula id="scirp.56537-formula577"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x31.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x32.png" xlink:type="simple"/></inline-formula> determines the true temperature at the wavelength<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x33.png" xlink:type="simple"/></inline-formula>, at the linear dependence of the logarithm of the emissivity from the wavelength, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x32.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x34.png" xlink:type="simple"/></inline-formula> which is set during calibration.</p><p>Usually for method of double spectral ratio the relation <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x35.png" xlink:type="simple"/></inline-formula> is using and that requires equidistant spacing of wavelengths; wherein the equivalent wavelength is rather big that increase the error of measuring. According [<xref ref-type="bibr" rid="scirp.56537-ref4">4</xref>] spacing of wavelengths can be arbitrary and not equidistant and that can decrease equivalent wave- length and improve the accuracy of measured temperature.</p><p>Thus, substituting the values of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x36.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x37.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x36.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x37.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x38.png" xlink:type="simple"/></inline-formula> in Equation (6) we will receive</p><disp-formula id="scirp.56537-formula578"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x39.png"  xlink:type="simple"/></disp-formula><p>And get the expression for the “resultant” emissivity in the form of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x40.png" xlink:type="simple"/></inline-formula></p><disp-formula id="scirp.56537-formula579"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x41.png"  xlink:type="simple"/></disp-formula><p>If to follow to the linear dependence of emissivity from wavelength the “resultant” emissivity must be equal to zero,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x42.png" xlink:type="simple"/></inline-formula>. However, it is obvious that<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x42.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x43.png" xlink:type="simple"/></inline-formula>.</p><p>This can be seen from the formula (7) for V and illustrated in <xref ref-type="fig" rid="fig1">Figure 1</xref>, where: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x44.png" xlink:type="simple"/></inline-formula>is not straight line and linear polyline marked by dots. Therefore for linearization of this relationship it is necessary to change the values <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x45.png" xlink:type="simple"/></inline-formula> or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x44.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x45.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x46.png" xlink:type="simple"/></inline-formula>.</p><p>Let’s change the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x47.png" xlink:type="simple"/></inline-formula>. From Equation (7) it is seen that the values<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x48.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x49.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x47.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x48.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x49.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x50.png" xlink:type="simple"/></inline-formula> differ only by constant coefficients.</p><p>Thus, we determine the value of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x51.png" xlink:type="simple"/></inline-formula>, where the “resultant” dependence of logarithm of emissivity will be linear.</p><disp-formula id="scirp.56537-formula580"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x52.png"  xlink:type="simple"/></disp-formula><p>Substituting the expression for <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x53.png" xlink:type="simple"/></inline-formula> into<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x54.png" xlink:type="simple"/></inline-formula>, we obtain the value <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x53.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x54.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x55.png" xlink:type="simple"/></inline-formula> as:</p><disp-formula id="scirp.56537-formula581"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x56.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x57.png" xlink:type="simple"/></inline-formula> (10)</p><p>Thus, the expression (6) for V, specifying the desired value of the true temperature at a linear dependence of the logarithm of the emissivity will have the form:</p><disp-formula id="scirp.56537-formula582"><label>(11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x58.png"  xlink:type="simple"/></disp-formula><p>or <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x59.png" xlink:type="simple"/></inline-formula> (12)</p><p>Moreover,</p><disp-formula id="scirp.56537-formula583"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x60.png"  xlink:type="simple"/></disp-formula><p>Thus, the desired value of the true temperature will be equal to</p><disp-formula id="scirp.56537-formula584"><label>(13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x61.png"  xlink:type="simple"/></disp-formula><p>where,</p><disp-formula id="scirp.56537-formula585"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x62.png"  xlink:type="simple"/></disp-formula><p>And the emissivity will be equal to</p><disp-formula id="scirp.56537-formula586"><label>(14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/7-1720274x63.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Example</title><p>As an example of proposed method let’s present the result of calculation of the true temperature for steel; data are taken from [<xref ref-type="bibr" rid="scirp.56537-ref5">5</xref>] . This work contains the following data:</p><p>Steel<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x64.png" xlink:type="simple"/></inline-formula>; T = 1600˚C at a wavelength<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x65.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x66.png" xlink:type="simple"/></inline-formula>;<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x64.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x65.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x66.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x67.png" xlink:type="simple"/></inline-formula>, the value of</p><disp-formula id="scirp.56537-formula587"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x68.png"  xlink:type="simple"/></disp-formula><p>Let’s now choose a second “virtual” wavelength from the spectrum of thermal radiation, for example,<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x69.png" xlink:type="simple"/></inline-formula>. Then the second pyrometer signal can be written as:</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x70.png" xlink:type="simple"/></inline-formula>, where.</p><p>Then<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x72.png" xlink:type="simple"/></inline-formula>, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x72.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x73.png" xlink:type="simple"/></inline-formula>.</p><p>The third signal <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x74.png" xlink:type="simple"/></inline-formula> which is equal to half the sum of the first two will be equal to</p><disp-formula id="scirp.56537-formula588"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x75.png"  xlink:type="simple"/></disp-formula><p>where:<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x76.png" xlink:type="simple"/></inline-formula>, and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x76.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x77.png" xlink:type="simple"/></inline-formula>, and</p><disp-formula id="scirp.56537-formula589"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x78.png"  xlink:type="simple"/></disp-formula><p>To provide the linearity of logarithm of emissivity let’s change the value<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x79.png" xlink:type="simple"/></inline-formula>, using formula (9), and</p><disp-formula id="scirp.56537-formula590"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x80.png"  xlink:type="simple"/></disp-formula><p>Now by substituting <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x81.png" xlink:type="simple"/></inline-formula> into the expression for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x82.png" xlink:type="simple"/></inline-formula>, we will get the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x81.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x82.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x83.png" xlink:type="simple"/></inline-formula> in the form of</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x84.png" xlink:type="simple"/></inline-formula>,</p><p>where: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x85.png" xlink:type="simple"/></inline-formula></p><p>Therefore <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x86.png" xlink:type="simple"/></inline-formula> and the value of <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x86.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x87.png" xlink:type="simple"/></inline-formula> in accordance with formula (11) will be equal to</p><disp-formula id="scirp.56537-formula591"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x88.png"  xlink:type="simple"/></disp-formula><p>or<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x89.png" xlink:type="simple"/></inline-formula>.</p><p>Therefore, the required temperature will be equal to <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x90.png" xlink:type="simple"/></inline-formula></p><p>And the resulting error will be</p><disp-formula id="scirp.56537-formula592"><graphic  xlink:href="http://html.scirp.org/file/7-1720274x91.png"  xlink:type="simple"/></disp-formula><p>The value of the logarithm of the emissivity will be equal to</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x92.png" xlink:type="simple"/></inline-formula>.</p><p>And the resulting error will be</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x93.png" xlink:type="simple"/></inline-formula>at a wavelength of<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x93.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x94.png" xlink:type="simple"/></inline-formula>.</p><p>From this example we can see that proposed method based on selection of “virtual” components provides rather good accuracy.</p><p>Note that if to select the second “virtual” component of the spectrum with a wavelength<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x95.png" xlink:type="simple"/></inline-formula>, that will reduce the equivalent wavelength Λ, and the error of true temperature will be less. For example for<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x96.png" xlink:type="simple"/></inline-formula>, i.e.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x97.png" xlink:type="simple"/></inline-formula>, then <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x95.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x96.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x97.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x98.png" xlink:type="simple"/></inline-formula> and the error will be reduced in 1.5 times, i.e.</p><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x99.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s4"><title>4. Conclusion</title><p>The described method and calculations performed on its base show that it can estimate fairly accurately the value of the true temperature and emissivity using only one real spectral component and two complementary “virtual” components of the emissivity spectrum which follows to Wien’s law and additional virtual spectral components can be selected rather arbitrarily. From a mathematical point of view, the proposed method is not rigorous, because formally Equation (1) includes two unknown parameters and the proposed heuristic approach is rather geometric in nature, but it provides, and quite simply, accurate measurements of true temperature and emissivity in spectral region<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/7-1720274x100.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s5"><title>Acknowledgements</title><p>I am grateful to the staff of the Academic Council of the Joint Institute for High Temperatures of the Russian Academy of Sciences for fruitful discussion of this work.</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.56537-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Svet, D.Ya. (1975) Color Pyrometer of True Temperature. Certificate of Invention, No. 476464. Bulletin of Inventions, Moscow.</mixed-citation></ref><ref id="scirp.56537-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Svet, D.Ya. (1982) Optical Methods for Measuring the True Temperature. Nauka, Moscow, 145.</mixed-citation></ref><ref id="scirp.56537-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Hornbeck, G.A. (1962) Temperature: Its Measurement and Control in Science and Industry. Reinhold V.I., New-York, 262.</mixed-citation></ref><ref id="scirp.56537-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Svet, D.Ya. (1985) 3-Wavelength Radiation Pyrometer. Certificate of Invention No. 1284336. Bulletin of Inventions, Moscow.</mixed-citation></ref><ref id="scirp.56537-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Shvarev, K.M., Gushchin, V.S., Baum, B.A. and Held, V.P. (1979) Optical Constants of Iron-Carbon Alloys in the Temperature Range 20&amp;deg;C - 1600&amp;deg;C. Teplofizika, 17, 66-71.</mixed-citation></ref></ref-list></back></article>