NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver
Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line...
Ausführliche Beschreibung
Gespeichert in:
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
|---|---|
| Übergeordnetes Werk: |
in: Infrared Physics - Amsterdam : Elsevier, 17(1977), 6, Seite 431-439 |
| Übergeordnetes Werk: |
volume:17 ; year:1977 ; number:6 ; pages:431-439 |
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| 520 | |a Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. | ||
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(DE-627)NLEJ179225200 (DE-599)GBVNLZ179225200 DE-627 ger DE-627 rakwb eng NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Kostiuk, T. oth Mumma, M.J. oth Hillman, J.J. oth Buhl, D. oth Brown, L.W. oth Faris, J.L. oth Spears, D.L. oth in Infrared Physics Amsterdam : Elsevier 17(1977), 6, Seite 431-439 (DE-627)NLEJ17762003X (DE-600)2139338-2 0020-0891 nnns volume:17 year:1977 number:6 pages:431-439 http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 17 1977 6 431-439 |
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(DE-627)NLEJ179225200 (DE-599)GBVNLZ179225200 DE-627 ger DE-627 rakwb eng NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Kostiuk, T. oth Mumma, M.J. oth Hillman, J.J. oth Buhl, D. oth Brown, L.W. oth Faris, J.L. oth Spears, D.L. oth in Infrared Physics Amsterdam : Elsevier 17(1977), 6, Seite 431-439 (DE-627)NLEJ17762003X (DE-600)2139338-2 0020-0891 nnns volume:17 year:1977 number:6 pages:431-439 http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 17 1977 6 431-439 |
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(DE-627)NLEJ179225200 (DE-599)GBVNLZ179225200 DE-627 ger DE-627 rakwb eng NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Kostiuk, T. oth Mumma, M.J. oth Hillman, J.J. oth Buhl, D. oth Brown, L.W. oth Faris, J.L. oth Spears, D.L. oth in Infrared Physics Amsterdam : Elsevier 17(1977), 6, Seite 431-439 (DE-627)NLEJ17762003X (DE-600)2139338-2 0020-0891 nnns volume:17 year:1977 number:6 pages:431-439 http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 17 1977 6 431-439 |
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(DE-627)NLEJ179225200 (DE-599)GBVNLZ179225200 DE-627 ger DE-627 rakwb eng NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Kostiuk, T. oth Mumma, M.J. oth Hillman, J.J. oth Buhl, D. oth Brown, L.W. oth Faris, J.L. oth Spears, D.L. oth in Infrared Physics Amsterdam : Elsevier 17(1977), 6, Seite 431-439 (DE-627)NLEJ17762003X (DE-600)2139338-2 0020-0891 nnns volume:17 year:1977 number:6 pages:431-439 http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 17 1977 6 431-439 |
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(DE-627)NLEJ179225200 (DE-599)GBVNLZ179225200 DE-627 ger DE-627 rakwb eng NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver 1977 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Kostiuk, T. oth Mumma, M.J. oth Hillman, J.J. oth Buhl, D. oth Brown, L.W. oth Faris, J.L. oth Spears, D.L. oth in Infrared Physics Amsterdam : Elsevier 17(1977), 6, Seite 431-439 (DE-627)NLEJ17762003X (DE-600)2139338-2 0020-0891 nnns volume:17 year:1977 number:6 pages:431-439 http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5 GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 17 1977 6 431-439 |
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nh"3 spectral line measurements on earth and jupiter using a 10 μm superheterodyne receiver |
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NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver |
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Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. |
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Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. |
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Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">NLEJ179225200</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20210706094336.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">070505s1977 xx |||||o 00| ||eng c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ179225200</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVNLZ179225200</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">NH"3 spectral line measurements on Earth and Jupiter using a 10 μm superheterodyne receiver</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1977</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">z</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zu</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Measurements of absolute line positions and shapes of eleven absorption lines of NH"3 were made using an infrared heterodyne spectrometer. Line profiles were obtained with 5 MHz resolution. NH"3 line positions relative to ^1^2C^1^6O"2 and ^1^3C^1^6O"2 local oscillator laser line emission frequencies were determined to +/-3 MHz. Using the obtained data a search list for NH"3 spectral lines on Jupiter was generated. Observations of Jovian polar regions in search of NH"3 aR(1,1) and sQ(2,1) auroral emission revealed possible strong nonthermal features. The line widths were consistent with low local kinetic temperatures. The relatively high line intensities, determined by local pumping mechanisms, corresponded to temperatures of several hundred Kelvins. Experimental details and implications of these measurements are discussed.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">Elsevier Journal Backfiles on ScienceDirect 1907 - 2002</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kostiuk, T.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Mumma, M.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hillman, J.J.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Buhl, D.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Brown, L.W.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Faris, J.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Spears, D.L.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">in</subfield><subfield code="t">Infrared Physics</subfield><subfield code="d">Amsterdam : Elsevier</subfield><subfield code="g">17(1977), 6, Seite 431-439</subfield><subfield code="w">(DE-627)NLEJ17762003X</subfield><subfield code="w">(DE-600)2139338-2</subfield><subfield code="x">0020-0891</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:17</subfield><subfield code="g">year:1977</subfield><subfield code="g">number:6</subfield><subfield code="g">pages:431-439</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">http://linkinghub.elsevier.com/retrieve/pii/0020-0891(77)90049-5</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_H</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-SDJ</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_NL_ARTICLE</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">17</subfield><subfield code="j">1977</subfield><subfield code="e">6</subfield><subfield code="h">431-439</subfield></datafield></record></collection>
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