Modeling of radiative transfer through a spherical planetary atmosphere : application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR

During the last years and decades issues related to the physics and chemistry of the Earthś atmosphere have attracted much scientific and public interest. The most important problems are stratospheric ozone loss and the ò̀zone hole ́́above Antarctica, global warming and climate change, and tropospheric air pollution. The understanding of the impact of human activities on the Earthś atmosphere requires measurements on a global scale. These enable the spatial and temporal variability of the atmospheric constituents to be investigated. Recently efforts have been made to establish a global observation system comprising satellite instruments and ground-based networks. To process data supplied by the instruments which belong to the global observation system, the development of radiative transfer models and retrieval algorithms is essential. This thesis contributes to the development of the radiative transfer models and retrieval algorithms intended to interprete measurements of the spectral radiance scattered in the atmosphere or transmitted through the atmosphere in UV-Vis-NIR spectral region performed by a new-generation remote sensing satellite spectrometer SCIAMACHY. In this study, main problems of radiative transfer through a spherical planetary atmosphere compared to a plane-parallel atmosphere are investigated. An efficient spherical radiative transfer model intended to simulate SCIAMACHY limb measurements was developed and validated. The model can also be used for the interpretation of measurements performed by other space-borne instruments as well as to compute air mass factors for ground-based measurements. An approximate approach allowing the simulation of limb measurements to be substantially accelerated was developed and its accuracy was investigated. Furthermore, a numerical radiative transfer model intended to simulate SCIAMACHY occultation measurements was developed and then coupled with an appropriate selected inverse technique. Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Rozanov, Alexei
Hochschulschrift:	Bremen, Univ., Diss, 2001

Format:	E-Book
Sprache:	Englisch

Erschienen:	2001

Schlagwörter:	Atmosphäre / Spurengas / Satellitenfernerkundung / Strahlungstransport / NIR-Spektroskopie / UV-VIS-Spektroskopie
Formangabe:	Hochschulschrift

Umfang:	Online-Ressource (150 S.)

Links:	Link aufrufen Volltext Volltext Volltext

Katalog-ID:	358553342

Internformat


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matchkey_str	rozanovalexei:2001----:oeigfaitvtasetruhshrcl
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topic_facet	Atmosphäre Spurengas Satellitenfernerkundung Strahlungstransport NIR-Spektroskopie UV-VIS-Spektroskopie
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title	Modeling of radiative transfer through a spherical planetary atmosphere application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR
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title_full	Modeling of radiative transfer through a spherical planetary atmosphere application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR vorgelegt von Alexei Rozanov
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title_sub	application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR
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title_sort	modeling of radiative transfer through a spherical planetary atmosphereapplication to atmospheric trace gases retrieval from occultation- and limb-measurements in uv-vis-nir
title_auth	Modeling of radiative transfer through a spherical planetary atmosphere application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR
abstract	During the last years and decades issues related to the physics and chemistry of the Earthś atmosphere have attracted much scientific and public interest. The most important problems are stratospheric ozone loss and the ò̀zone hole ́́above Antarctica, global warming and climate change, and tropospheric air pollution. The understanding of the impact of human activities on the Earthś atmosphere requires measurements on a global scale. These enable the spatial and temporal variability of the atmospheric constituents to be investigated. Recently efforts have been made to establish a global observation system comprising satellite instruments and ground-based networks. To process data supplied by the instruments which belong to the global observation system, the development of radiative transfer models and retrieval algorithms is essential. This thesis contributes to the development of the radiative transfer models and retrieval algorithms intended to interprete measurements of the spectral radiance scattered in the atmosphere or transmitted through the atmosphere in UV-Vis-NIR spectral region performed by a new-generation remote sensing satellite spectrometer SCIAMACHY. In this study, main problems of radiative transfer through a spherical planetary atmosphere compared to a plane-parallel atmosphere are investigated. An efficient spherical radiative transfer model intended to simulate SCIAMACHY limb measurements was developed and validated. The model can also be used for the interpretation of measurements performed by other space-borne instruments as well as to compute air mass factors for ground-based measurements. An approximate approach allowing the simulation of limb measurements to be substantially accelerated was developed and its accuracy was investigated. Furthermore, a numerical radiative transfer model intended to simulate SCIAMACHY occultation measurements was developed and then coupled with an appropriate selected inverse technique.
abstractGer	During the last years and decades issues related to the physics and chemistry of the Earthś atmosphere have attracted much scientific and public interest. The most important problems are stratospheric ozone loss and the ò̀zone hole ́́above Antarctica, global warming and climate change, and tropospheric air pollution. The understanding of the impact of human activities on the Earthś atmosphere requires measurements on a global scale. These enable the spatial and temporal variability of the atmospheric constituents to be investigated. Recently efforts have been made to establish a global observation system comprising satellite instruments and ground-based networks. To process data supplied by the instruments which belong to the global observation system, the development of radiative transfer models and retrieval algorithms is essential. This thesis contributes to the development of the radiative transfer models and retrieval algorithms intended to interprete measurements of the spectral radiance scattered in the atmosphere or transmitted through the atmosphere in UV-Vis-NIR spectral region performed by a new-generation remote sensing satellite spectrometer SCIAMACHY. In this study, main problems of radiative transfer through a spherical planetary atmosphere compared to a plane-parallel atmosphere are investigated. An efficient spherical radiative transfer model intended to simulate SCIAMACHY limb measurements was developed and validated. The model can also be used for the interpretation of measurements performed by other space-borne instruments as well as to compute air mass factors for ground-based measurements. An approximate approach allowing the simulation of limb measurements to be substantially accelerated was developed and its accuracy was investigated. Furthermore, a numerical radiative transfer model intended to simulate SCIAMACHY occultation measurements was developed and then coupled with an appropriate selected inverse technique.
abstract_unstemmed	During the last years and decades issues related to the physics and chemistry of the Earthś atmosphere have attracted much scientific and public interest. The most important problems are stratospheric ozone loss and the ò̀zone hole ́́above Antarctica, global warming and climate change, and tropospheric air pollution. The understanding of the impact of human activities on the Earthś atmosphere requires measurements on a global scale. These enable the spatial and temporal variability of the atmospheric constituents to be investigated. Recently efforts have been made to establish a global observation system comprising satellite instruments and ground-based networks. To process data supplied by the instruments which belong to the global observation system, the development of radiative transfer models and retrieval algorithms is essential. This thesis contributes to the development of the radiative transfer models and retrieval algorithms intended to interprete measurements of the spectral radiance scattered in the atmosphere or transmitted through the atmosphere in UV-Vis-NIR spectral region performed by a new-generation remote sensing satellite spectrometer SCIAMACHY. In this study, main problems of radiative transfer through a spherical planetary atmosphere compared to a plane-parallel atmosphere are investigated. An efficient spherical radiative transfer model intended to simulate SCIAMACHY limb measurements was developed and validated. The model can also be used for the interpretation of measurements performed by other space-borne instruments as well as to compute air mass factors for ground-based measurements. An approximate approach allowing the simulation of limb measurements to be substantially accelerated was developed and its accuracy was investigated. Furthermore, a numerical radiative transfer model intended to simulate SCIAMACHY occultation measurements was developed and then coupled with an appropriate selected inverse technique.
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title_short	Modeling of radiative transfer through a spherical planetary atmosphere
url	http://webdoc.sub.gwdg.de/ebook/diss/2003/sub-bremen/dissertations/E-Diss182_thesis.pdf http://elib.suub.uni-bremen.de/publications/dissertations/E-Diss182ṯhesis.pdf http://d-nb.info/963150235
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GND_str_mv	Hochschulschrift Erdatmosphäre Atmosphäre Spurengas Satellit / Fernerkundung Satellitenfernerkundung Radiative transfer Radiation transport Strahlungstransport Nahinfrarot-Spektroskopie NIR-Spektroskopie Sichtbar-Ultraviolett-Spektroskopie Ultraviolett-VIS-Spektroskopie UVIS-Spektroskopie UV-VIS-Spektroskopie Rozanov, Aleksej Rozanov, Alexei
GND_txt_mv	Hochschulschrift Erdatmosphäre Atmosphäre Spurengas Satellit / Fernerkundung Satellitenfernerkundung Radiative transfer Radiation transport Strahlungstransport Nahinfrarot-Spektroskopie NIR-Spektroskopie Sichtbar-Ultraviolett-Spektroskopie Ultraviolett-VIS-Spektroskopie UVIS-Spektroskopie UV-VIS-Spektroskopie Rozanov, Aleksej Rozanov, Alexei
GND_txtF_mv	Hochschulschrift Erdatmosphäre Atmosphäre Spurengas Satellit / Fernerkundung Satellitenfernerkundung Radiative transfer Radiation transport Strahlungstransport Nahinfrarot-Spektroskopie NIR-Spektroskopie Sichtbar-Ultraviolett-Spektroskopie Ultraviolett-VIS-Spektroskopie UVIS-Spektroskopie UV-VIS-Spektroskopie Rozanov, Aleksej Rozanov, Alexei
mediatype_str_mv	c
isOA_txt	false
hochschulschrift_bool	true
author2_role	oth
up_date	2024-07-04T22:47:40.144Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000cam a2200265 4500</leader><controlfield tag="001">358553342</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240130011353.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">030102s2001 gw \|\|\|\|\|om 00\| \|\|eng c</controlfield><datafield tag="015" ind1=" " ind2=" "><subfield code="a">03,H01,1031</subfield><subfield code="2">dnb</subfield></datafield><datafield tag="016" ind1="7" ind2=" "><subfield code="a">963150235</subfield><subfield code="2">DE-101</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)358553342</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)DNB963150235</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)175066594</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="044" ind1=" " ind2=" "><subfield code="c">XA-DE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">31</subfield><subfield code="2">sdnb</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Modeling of radiative transfer through a spherical planetary atmosphere</subfield><subfield code="b">application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR</subfield><subfield code="c">vorgelegt von Alexei Rozanov</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2001</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">Online-Ressource (150 S.)</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="502" ind1=" " ind2=" "><subfield code="a">Bremen, Univ., Diss, 2001</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">During the last years and decades issues related to the physics and chemistry of the Earthś atmosphere have attracted much scientific and public interest. 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Modeling of radiative transfer through a spherical planetary atmosphere : application to atmospheric trace gases retrieval from occultation- and limb-measurements in UV-Vis-NIR

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