Infrared Filters of Controllable Transmission
When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread unif...
Ausführliche Beschreibung
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E-Artikel |
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1930 |
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Online-Ressource 6 |
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Reproduktion: |
APS Digital Backfile Archive 1893-2003 |
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Übergeordnetes Werk: |
Enthalten in: The physical review - Lancaster, Pa. [u.a.], 1893, 36(1930), 1, Seite 71-76 |
Übergeordnetes Werk: |
volume:36 ; year:1930 ; number:1 ; pages:71-76 ; extent:6 |
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520 | |a When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. | ||
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(DE-627)NLEJ25145763X (DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf DE-627 ger DE-627 rakwb Infrared Filters of Controllable Transmission 1930 Online-Ressource 6 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. APS Digital Backfile Archive 1893-2003 Pfund, A. H. oth Enthalten in The physical review Lancaster, Pa. [u.a.], 1893 36(1930), 1, Seite 71-76 (DE-627)NLEJ24823790X (DE-600)2177092-X 1536-6065 nnns volume:36 year:1930 number:1 pages:71-76 extent:6 https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 36 1930 1 71-76 6 |
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(DE-627)NLEJ25145763X (DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf DE-627 ger DE-627 rakwb Infrared Filters of Controllable Transmission 1930 Online-Ressource 6 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. APS Digital Backfile Archive 1893-2003 Pfund, A. H. oth Enthalten in The physical review Lancaster, Pa. [u.a.], 1893 36(1930), 1, Seite 71-76 (DE-627)NLEJ24823790X (DE-600)2177092-X 1536-6065 nnns volume:36 year:1930 number:1 pages:71-76 extent:6 https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 36 1930 1 71-76 6 |
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(DE-627)NLEJ25145763X (DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf DE-627 ger DE-627 rakwb Infrared Filters of Controllable Transmission 1930 Online-Ressource 6 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. APS Digital Backfile Archive 1893-2003 Pfund, A. H. oth Enthalten in The physical review Lancaster, Pa. [u.a.], 1893 36(1930), 1, Seite 71-76 (DE-627)NLEJ24823790X (DE-600)2177092-X 1536-6065 nnns volume:36 year:1930 number:1 pages:71-76 extent:6 https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 36 1930 1 71-76 6 |
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(DE-627)NLEJ25145763X (DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf DE-627 ger DE-627 rakwb Infrared Filters of Controllable Transmission 1930 Online-Ressource 6 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. APS Digital Backfile Archive 1893-2003 Pfund, A. H. oth Enthalten in The physical review Lancaster, Pa. [u.a.], 1893 36(1930), 1, Seite 71-76 (DE-627)NLEJ24823790X (DE-600)2177092-X 1536-6065 nnns volume:36 year:1930 number:1 pages:71-76 extent:6 https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 36 1930 1 71-76 6 |
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(DE-627)NLEJ25145763X (DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf DE-627 ger DE-627 rakwb Infrared Filters of Controllable Transmission 1930 Online-Ressource 6 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. APS Digital Backfile Archive 1893-2003 Pfund, A. H. oth Enthalten in The physical review Lancaster, Pa. [u.a.], 1893 36(1930), 1, Seite 71-76 (DE-627)NLEJ24823790X (DE-600)2177092-X 1536-6065 nnns volume:36 year:1930 number:1 pages:71-76 extent:6 https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 36 1930 1 71-76 6 |
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Infrared Filters of Controllable Transmission |
abstract |
When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. |
abstractGer |
When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. |
abstract_unstemmed |
When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">NLEJ25145763X</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20231114111724.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">231114s1930 xx |||||o 00| ||und c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ25145763X</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-601)aps:19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf</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="245" ind1="1" ind2="0"><subfield code="a">Infrared Filters of Controllable Transmission</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1930</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">6</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">When using an echelette grating for work in the infrared it is necessary to eliminate overlapping, higher orders. Since no adequate series of true filters covering the entire infrared is known, a new type of filter has been developed. Essentially, this type of filter consists of a powder spread uniformly over a surface of polished speculum. Short wave-length radiations are reflected diffusely while long wavelength radiations are largely transmitted since the Rayleigh scattering for long waves is feeble. The region of transition from opacity to transparency is controlled by choosing powders of proper particle-size and by depositing these in layers of appropriate thickness.Specific examples, involving the use of particles whose mean diameter covers the range: 0.22μ to 2.5μ, are presented to show how filters for almost any portion of the spectral range: 2μ to 7.5μ may be largely freed from the effects of superposed, higher orders. Filters for greater wave-lengths may be produced by much the same methods.</subfield></datafield><datafield tag="533" ind1=" " ind2=" "><subfield code="f">APS Digital Backfile Archive 1893-2003</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pfund, A. H.</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The physical review</subfield><subfield code="d">Lancaster, Pa. [u.a.], 1893</subfield><subfield code="g">36(1930), 1, Seite 71-76</subfield><subfield code="w">(DE-627)NLEJ24823790X</subfield><subfield code="w">(DE-600)2177092-X</subfield><subfield code="x">1536-6065</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:36</subfield><subfield code="g">year:1930</subfield><subfield code="g">number:1</subfield><subfield code="g">pages:71-76</subfield><subfield code="g">extent:6</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://www.tib.eu/de/suchen/id/aps%3A19d6d71bc3feedc7a2ff76396cd0bbcadf250bcf</subfield><subfield code="x">Verlag</subfield><subfield code="z">Deutschlandweit zugänglich</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_U</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-1-APS</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">36</subfield><subfield code="j">1930</subfield><subfield code="e">1</subfield><subfield code="h">71-76</subfield><subfield code="g">6</subfield></datafield></record></collection>
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