Diode laser spectroscopy of H2O and CO2 in the 1.877-μm region for the in situ monitoring of the martian atmosphere
Identifieur interne : 008E43 ( Main/Repository ); précédent : 008E42; suivant : 008E44Diode laser spectroscopy of H2O and CO2 in the 1.877-μm region for the in situ monitoring of the martian atmosphere
Auteurs : RBID : Pascal:06-0185857Descripteurs français
- Pascal (Inist)
- Spectrométrie laser, Diode laser, Carbone dioxyde, Vapeur eau, Planète Mars, Atmosphère planétaire, Intensité raie, Laser réaction répartie, Laser semiconducteur, Gallium Indium Antimoniure, Composé ternaire, Base donnée, Méthode ab initio, Laser accordable, Spectrométrie absorption, Dispositif expérimental, Etude expérimentale, C O, CO2, 4262F.
- Wicri :
- concept : Base de données.
English descriptors
- KwdEn :
- Ab initio method, Absorption spectroscopy, Carbon dioxide, Database, Distributed feedback lasers, Experimental device, Experimental study, Gallium Indium Antimonides, Laser diodes, Laser spectroscopy, Line intensity, Mars planet, Planetary atmospheres, Semiconductor lasers, Steam, Ternary compounds, Tunable lasers.
Abstract
A diode laser spectrometer was used in the laboratory to study H2O and CO2 line intensities and self-broadening coefficients around 1.877 μm. The spectral region ranging from 5327 cm-1 to 5329 cm-1, which is suitable for the in situ sensing of water vapor and carbon dioxide in the Martian atmosphere, was studied using a distributed feedback GaInSb diode laser from Nanoplus GmbH. We have studied one line from the (011) ← (000) band of H2O and two lines from the (0112)I ← (000) band of CO2. The results of intensity and self-broadening measurements are compared to available databases, ab initio calculations and previous experimental determinations. Finally, we discuss the current development of the tunable diode laser absorption spectrometer instrument, a laser diode sensor devoted to the in situ measurement of H2O and CO2 in the Martian atmosphere.
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<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Diode laser spectroscopy of H<sub>2</sub>O and CO<sub>2</sub> in the 1.877-μm region for the in situ monitoring of the martian atmosphere</title><author><name sortKey="Le Barbu, T" uniqKey="Le Barbu T">T. Le Barbu</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039</s1><s2>51687 Reims</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Champagne-Ardenne</region><settlement type="city">Reims</settlement></placeName></affiliation><affiliation wicri:level="3"><inist:fA14 i1="02"><s1>Institut Pierre Simon Laplace (IPSL), Service d'Aéronomie, UMR 7620, CNRS-Réduit de Verrières, B.P. 3</s1><s2>91371 Verrières-le-Buisson</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Verrières-le-Buisson</settlement></placeName></affiliation></author><author><name sortKey="Parvitte, B" uniqKey="Parvitte B">B. Parvitte</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039</s1><s2>51687 Reims</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Champagne-Ardenne</region><settlement type="city">Reims</settlement></placeName></affiliation></author><author><name sortKey="Zeninari, V" uniqKey="Zeninari V">V. Zeninari</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039</s1><s2>51687 Reims</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Champagne-Ardenne</region><settlement type="city">Reims</settlement></placeName></affiliation></author><author><name sortKey="Vinogradov, I" uniqKey="Vinogradov I">I. Vinogradov</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Space Research Institute (IKI), 84/32 Profsoyuznaya</s1><s2>117997 Moscow</s2><s3>RUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ></inist:fA14><country>Russie</country><placeName><settlement type="city">Moscou</settlement><region>District fédéral central</region></placeName></affiliation></author><author><name sortKey="Korablev, O" uniqKey="Korablev O">O. Korablev</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Space Research Institute (IKI), 84/32 Profsoyuznaya</s1><s2>117997 Moscow</s2><s3>RUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ></inist:fA14><country>Russie</country><placeName><settlement type="city">Moscou</settlement><region>District fédéral central</region></placeName></affiliation></author><author><name sortKey="Durry, G" uniqKey="Durry G">G. Durry</name><affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039</s1><s2>51687 Reims</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Champagne-Ardenne</region><settlement type="city">Reims</settlement></placeName></affiliation><affiliation wicri:level="3"><inist:fA14 i1="02"><s1>Institut Pierre Simon Laplace (IPSL), Service d'Aéronomie, UMR 7620, CNRS-Réduit de Verrières, B.P. 3</s1><s2>91371 Verrières-le-Buisson</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>6 aut.</sZ></inist:fA14><country>France</country><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Verrières-le-Buisson</settlement></placeName></affiliation></author></titleStmt><publicationStmt><idno type="inist">06-0185857</idno><date when="2006">2006</date><idno type="stanalyst">PASCAL 06-0185857 INIST</idno><idno type="RBID">Pascal:06-0185857</idno><idno type="wicri:Area/Main/Corpus">009222</idno><idno type="wicri:Area/Main/Repository">008E43</idno></publicationStmt><seriesStmt><idno type="ISSN">0946-2171</idno><title level="j" type="abbreviated">Appl. phys., B Lasers opt. : (Print)</title><title level="j" type="main">Applied physics. B, Lasers and optics : (Print)</title></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Ab initio method</term><term>Absorption spectroscopy</term><term>Carbon dioxide</term><term>Database</term><term>Distributed feedback lasers</term><term>Experimental device</term><term>Experimental study</term><term>Gallium Indium Antimonides</term><term>Laser diodes</term><term>Laser spectroscopy</term><term>Line intensity</term><term>Mars planet</term><term>Planetary atmospheres</term><term>Semiconductor lasers</term><term>Steam</term><term>Ternary compounds</term><term>Tunable lasers</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Spectrométrie laser</term><term>Diode laser</term><term>Carbone dioxyde</term><term>Vapeur eau</term><term>Planète Mars</term><term>Atmosphère planétaire</term><term>Intensité raie</term><term>Laser réaction répartie</term><term>Laser semiconducteur</term><term>Gallium Indium Antimoniure</term><term>Composé ternaire</term><term>Base donnée</term><term>Méthode ab initio</term><term>Laser accordable</term><term>Spectrométrie absorption</term><term>Dispositif expérimental</term><term>Etude expérimentale</term><term>C O</term><term>CO2</term><term>4262F</term></keywords><keywords scheme="Wicri" type="concept" xml:lang="fr"><term>Base de données</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">A diode laser spectrometer was used in the laboratory to study H<sub>2</sub>O and CO<sub>2</sub> line intensities and self-broadening coefficients around 1.877 μm. The spectral region ranging from 5327 cm<sup>-1</sup> to 5329 cm<sup>-1</sup>, which is suitable for the in situ sensing of water vapor and carbon dioxide in the Martian atmosphere, was studied using a distributed feedback GaInSb diode laser from Nanoplus GmbH. We have studied one line from the (011) ← (000) band of H<sub>2</sub>O and two lines from the (01<sup>1</sup>2)<sub>I</sub> ← (000) band of CO<sub>2</sub>. The results of intensity and self-broadening measurements are compared to available databases, ab initio calculations and previous experimental determinations. Finally, we discuss the current development of the tunable diode laser absorption spectrometer instrument, a laser diode sensor devoted to the in situ measurement of H<sub>2</sub>O and CO<sub>2</sub> in the Martian atmosphere.</div></front></TEI><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0946-2171</s0></fA01><fA03 i2="1"><s0>Appl. phys., B Lasers opt. : (Print)</s0></fA03><fA05><s2>82</s2></fA05><fA06><s2>1</s2></fA06><fA08 i1="01" i2="1" l="ENG"><s1>Diode laser spectroscopy of H<sub>2</sub>O and CO<sub>2</sub> in the 1.877-μm region for the in situ monitoring of the martian atmosphere</s1></fA08><fA11 i1="01" i2="1"><s1>LE BARBU (T.)</s1></fA11><fA11 i1="02" i2="1"><s1>PARVITTE (B.)</s1></fA11><fA11 i1="03" i2="1"><s1>ZENINARI (V.)</s1></fA11><fA11 i1="04" i2="1"><s1>VINOGRADOV (I.)</s1></fA11><fA11 i1="05" i2="1"><s1>KORABLEV (O.)</s1></fA11><fA11 i1="06" i2="1"><s1>DURRY (G.)</s1></fA11><fA14 i1="01"><s1>Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 6089, UFR Sciences Exactes et Naturelles, Moulin de la Housse, BP 1039</s1><s2>51687 Reims</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>2 aut.</sZ><sZ>3 aut.</sZ><sZ>6 aut.</sZ></fA14><fA14 i1="02"><s1>Institut Pierre Simon Laplace (IPSL), Service d'Aéronomie, UMR 7620, CNRS-Réduit de Verrières, B.P. 3</s1><s2>91371 Verrières-le-Buisson</s2><s3>FRA</s3><sZ>1 aut.</sZ><sZ>6 aut.</sZ></fA14><fA14 i1="03"><s1>Space Research Institute (IKI), 84/32 Profsoyuznaya</s1><s2>117997 Moscow</s2><s3>RUS</s3><sZ>4 aut.</sZ><sZ>5 aut.</sZ></fA14><fA20><s1>133-140</s1></fA20><fA21><s1>2006</s1></fA21><fA23 i1="01"><s0>ENG</s0></fA23><fA43 i1="01"><s1>INIST</s1><s2>16194B</s2><s5>354000134989860250</s5></fA43><fA44><s0>0000</s0><s1>© 2006 INIST-CNRS. All rights reserved.</s1></fA44><fA45><s0>18 ref.</s0></fA45><fA47 i1="01" i2="1"><s0>06-0185857</s0></fA47><fA60><s1>P</s1></fA60><fA61><s0>A</s0></fA61><fA64 i1="01" i2="1"><s0>Applied physics. B, Lasers and optics : (Print)</s0></fA64><fA66 i1="01"><s0>DEU</s0></fA66><fC01 i1="01" l="ENG"><s0>A diode laser spectrometer was used in the laboratory to study H<sub>2</sub>O and CO<sub>2</sub> line intensities and self-broadening coefficients around 1.877 μm. The spectral region ranging from 5327 cm<sup>-1</sup> to 5329 cm<sup>-1</sup>, which is suitable for the in situ sensing of water vapor and carbon dioxide in the Martian atmosphere, was studied using a distributed feedback GaInSb diode laser from Nanoplus GmbH. We have studied one line from the (011) ← (000) band of H<sub>2</sub>O and two lines from the (01<sup>1</sup>2)<sub>I</sub> ← (000) band of CO<sub>2</sub>. The results of intensity and self-broadening measurements are compared to available databases, ab initio calculations and previous experimental determinations. Finally, we discuss the current development of the tunable diode laser absorption spectrometer instrument, a laser diode sensor devoted to the in situ measurement of H<sub>2</sub>O and CO<sub>2</sub> in the Martian atmosphere.</s0></fC01><fC02 i1="01" i2="3"><s0>001B40B62F</s0></fC02><fC03 i1="01" i2="3" l="FRE"><s0>Spectrométrie laser</s0><s5>50</s5></fC03><fC03 i1="01" i2="3" l="ENG"><s0>Laser spectroscopy</s0><s5>50</s5></fC03><fC03 i1="02" i2="3" l="FRE"><s0>Diode laser</s0><s5>51</s5></fC03><fC03 i1="02" i2="3" l="ENG"><s0>Laser diodes</s0><s5>51</s5></fC03><fC03 i1="03" i2="3" l="FRE"><s0>Carbone dioxyde</s0><s2>NK</s2><s5>52</s5></fC03><fC03 i1="03" i2="3" l="ENG"><s0>Carbon dioxide</s0><s2>NK</s2><s5>52</s5></fC03><fC03 i1="04" i2="3" l="FRE"><s0>Vapeur eau</s0><s5>53</s5></fC03><fC03 i1="04" i2="3" l="ENG"><s0>Steam</s0><s5>53</s5></fC03><fC03 i1="05" i2="3" l="FRE"><s0>Planète Mars</s0><s5>54</s5></fC03><fC03 i1="05" i2="3" l="ENG"><s0>Mars planet</s0><s5>54</s5></fC03><fC03 i1="06" i2="3" l="FRE"><s0>Atmosphère planétaire</s0><s5>55</s5></fC03><fC03 i1="06" i2="3" l="ENG"><s0>Planetary atmospheres</s0><s5>55</s5></fC03><fC03 i1="07" i2="3" l="FRE"><s0>Intensité raie</s0><s5>56</s5></fC03><fC03 i1="07" i2="3" l="ENG"><s0>Line intensity</s0><s5>56</s5></fC03><fC03 i1="08" i2="3" l="FRE"><s0>Laser réaction répartie</s0><s5>57</s5></fC03><fC03 i1="08" i2="3" l="ENG"><s0>Distributed feedback lasers</s0><s5>57</s5></fC03><fC03 i1="09" i2="3" l="FRE"><s0>Laser semiconducteur</s0><s5>58</s5></fC03><fC03 i1="09" i2="3" l="ENG"><s0>Semiconductor lasers</s0><s5>58</s5></fC03><fC03 i1="10" i2="3" l="FRE"><s0>Gallium Indium Antimoniure</s0><s2>NC</s2><s2>NA</s2><s5>59</s5></fC03><fC03 i1="10" i2="3" l="ENG"><s0>Gallium Indium Antimonides</s0><s2>NC</s2><s2>NA</s2><s5>59</s5></fC03><fC03 i1="11" i2="3" l="FRE"><s0>Composé ternaire</s0><s5>60</s5></fC03><fC03 i1="11" i2="3" l="ENG"><s0>Ternary compounds</s0><s5>60</s5></fC03><fC03 i1="12" i2="X" l="FRE"><s0>Base donnée</s0><s5>61</s5></fC03><fC03 i1="12" i2="X" l="ENG"><s0>Database</s0><s5>61</s5></fC03><fC03 i1="12" i2="X" l="SPA"><s0>Base dato</s0><s5>61</s5></fC03><fC03 i1="13" i2="X" l="FRE"><s0>Méthode ab initio</s0><s5>62</s5></fC03><fC03 i1="13" i2="X" l="ENG"><s0>Ab initio method</s0><s5>62</s5></fC03><fC03 i1="13" i2="X" l="SPA"><s0>Método ab initio</s0><s5>62</s5></fC03><fC03 i1="14" i2="3" l="FRE"><s0>Laser accordable</s0><s5>63</s5></fC03><fC03 i1="14" i2="3" l="ENG"><s0>Tunable lasers</s0><s5>63</s5></fC03><fC03 i1="15" i2="3" l="FRE"><s0>Spectrométrie absorption</s0><s5>64</s5></fC03><fC03 i1="15" i2="3" l="ENG"><s0>Absorption spectroscopy</s0><s5>64</s5></fC03><fC03 i1="16" i2="X" l="FRE"><s0>Dispositif expérimental</s0><s5>65</s5></fC03><fC03 i1="16" i2="X" l="ENG"><s0>Experimental device</s0><s5>65</s5></fC03><fC03 i1="16" i2="X" l="SPA"><s0>Dispositivo experimental</s0><s5>65</s5></fC03><fC03 i1="17" i2="3" l="FRE"><s0>Etude expérimentale</s0><s5>66</s5></fC03><fC03 i1="17" i2="3" l="ENG"><s0>Experimental study</s0><s5>66</s5></fC03><fC03 i1="18" i2="3" l="FRE"><s0>C O</s0><s4>INC</s4><s5>75</s5></fC03><fC03 i1="19" i2="3" l="FRE"><s0>CO2</s0><s4>INC</s4><s5>83</s5></fC03><fC03 i1="20" i2="3" l="FRE"><s0>4262F</s0><s4>INC</s4><s5>91</s5></fC03><fN21><s1>114</s1></fN21><fN44 i1="01"><s1>PSI</s1></fN44><fN82><s1>PSI</s1></fN82></pA></standard></inist></record>Pour manipuler ce document sous Unix (Dilib)
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