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  <item rdf:about="https://ir.lib.ncu.edu.tw/handle/987654321/101954">
    <title>Tropospheric observations of CFC-114 and CFC-114a with a focus on long-term trends and emissions</title>
    <link>https://ir.lib.ncu.edu.tw/handle/987654321/101954</link>
    <description>title: Tropospheric observations of CFC-114 and CFC-114a with a focus on long-term trends and emissions abstract: 摘要： Chlorofluorocarbons (CFCs) are ozone-depleting substances as well as strong greenhouse gases, and the control of their production and use under the Montreal Protocol has had demonstrable benefits to both mitigation of increasing surface UV radiation and climate forcing. A global ban on consumption came into force in 2010, but there is evidence of continuing emissions of certain CFCs from a range of sources. One compound has received little attention in the literature, namely CFC-114 (C2Cl2F4). Of particular interest here is the differentiation between CFC-114 (CClF2CClF2) and its asymmetric isomeric form CFC-114a (CF3CCl2F) as atmospheric long-term measurements in the peer-reviewed literature to date have been assumed to represent the sum of both isomers with a time-invariant isomeric speciation. Here we report the first long-term measurements of the two isomeric forms separately, and find that they have different origins and trends in the atmosphere. Air samples collected at Cape Grim (41° S), Australia, during atmospheric background conditions since 1978, combined with samples collected from deep polar snow (firn) enable us to obtain a near-complete record of both gases since their initial production and release in the 1940s. Both isomers were present in the unpolluted atmosphere in comparably small amounts before 1960. The mixing ratio of CFC-114 doubled from 7.9 to 14.8 parts per trillion (ppt) between the start of the Cape Grim record in 1978 and the end of our record in 2014, while over the same time CFC-114a trebled from 0.35 to 1.03 ppt. Mixing ratios of both isomers are slowly decreasing by the end of this period. This is consistent with measurements of recent aircraft-based samples showing no significant interhemispheric mixing ratio gradient. We also find that the fraction of CFC-114a mixing ratio relative to that of CFC-114 increased from 4.2 to 6.9 % over the 37-year period. This contradicts the current tacit assumption used in international climate change and ozone depletion assessments that both isomers have been largely co-emitted and that their atmospheric concentration ratio has remained approximately constant in time. Complementary observations of air collected in Taiwan indicate a persisting source of CFC-114a in South East Asia which may have been contributing to the changing balance between the two isomers. In addition we present top-down global annual emission estimates of CFC-114 and CFC-114a derived from these measurements using a two-dimensional atmospheric chemistry-transport model. In general, the emissions for both compounds grew steadily during the 1980s, followed by a substantial reduction from the late 1980s onwards, which is consistent with the reduction of emission in response to the Montreal Protocol, and broadly consistent with bottom-up estimates derived by industry. However, we find that small but significant emissions of both isomers remain in 2014. Moreover the inferred changes to the ratio of emissions of the two isomers since the 1990s also indicate that the sources of the two gases are, in part, independent.
出版者： Katlenburg-Lindau: Copernicus GmbH
出版日期： 2016-12-09
出處： Atmospheric chemistry and physics, 2016-12, Vol.16 (23), p.15347-15358
資源來源： Agricultural &amp; Environmental Science Collection
版權： COPYRIGHT 2016 Copernicus GmbH
版權： Copyright Copernicus GmbH 2016
版權： 2016. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
版權： licence_http://creativecommons.org/publicdomain/zero
識別號： ISSN: 1680-7324
識別號： ISSN: 1680-7316
識別號： EISSN: 1680-7324
識別號： DOI: 10.5194/acp-16-15347-2016
&lt;br&gt;</description>
  </item>
  <item rdf:about="https://ir.lib.ncu.edu.tw/handle/987654321/101951">
    <title>Tropospheric observations of CFC-114 and CFC-114a with a focus on long-term trends and emissions</title>
    <link>https://ir.lib.ncu.edu.tw/handle/987654321/101951</link>
    <description>title: Tropospheric observations of CFC-114 and CFC-114a with a focus on long-term trends and emissions abstract: 摘要： Chlorofluorocarbons (CFCs) are ozone-depleting substances as well as strong greenhouse gases, and the control of their production and use under the Montreal Protocol has had demonstrable benefits to both mitigation of increasing surface UV radiation and climate forcing. A global ban on consumption came into force in 2010, but there is evidence of continuing emissions of certain CFCs from a range of sources. One compound has received little attention in the literature, namely CFC-114 (C2Cl2F4). Of particular interest here is the differentiation between CFC-114 (CClF2CClF2) and its asymmetric isomeric form CFC-114a (CF3CCl2F) as atmospheric long-term measurements in the peer-reviewed literature to date have been assumed to represent the sum of both isomers with a time-invariant isomeric speciation. Here we report the first long-term measurements of the two isomeric forms separately, and find that they have different origins and trends in the atmosphere. Air samples collected at Cape Grim (41° S), Australia, during atmospheric background conditions since 1978, combined with samples collected from deep polar snow (firn) enable us to obtain a near-complete record of both gases since their initial production and release in the 1940s. Both isomers were present in the unpolluted atmosphere in comparably small amounts before 1960. The mixing ratio of CFC-114 doubled from 7.9 to 14.8 parts per trillion (ppt) between the start of the Cape Grim record in 1978 and the end of our record in 2014, while over the same time CFC-114a trebled from 0.35 to 1.03 ppt. Mixing ratios of both isomers are slowly decreasing by the end of this period. This is consistent with measurements of recent aircraft-based samples showing no significant interhemispheric mixing ratio gradient. We also find that the fraction of CFC-114a mixing ratio relative to that of CFC-114 increased from 4.2 to 6.9 % over the 37-year period. This contradicts the current tacit assumption used in international climate change and ozone depletion assessments that both isomers have been largely co-emitted and that their atmospheric concentration ratio has remained approximately constant in time. Complementary observations of air collected in Taiwan indicate a persisting source of CFC-114a in South East Asia which may have been contributing to the changing balance between the two isomers. In addition we present top-down global annual emission estimates of CFC-114 and CFC-114a derived from these measurements using a two-dimensional atmospheric chemistry-transport model. In general, the emissions for both compounds grew steadily during the 1980s, followed by a substantial reduction from the late 1980s onwards, which is consistent with the reduction of emission in response to the Montreal Protocol, and broadly consistent with bottom-up estimates derived by industry. However, we find that small but significant emissions of both isomers remain in 2014. Moreover the inferred changes to the ratio of emissions of the two isomers since the 1990s also indicate that the sources of the two gases are, in part, independent.
出版者： Katlenburg-Lindau: Copernicus GmbH
出版日期： 2016-12-09
出處： Atmospheric chemistry and physics, 2016-12, Vol.16 (23), p.15347-15358
資源來源： Agricultural &amp; Environmental Science Collection
版權： COPYRIGHT 2016 Copernicus GmbH
版權： Copyright Copernicus GmbH 2016
版權： 2016. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
版權： licence_http://creativecommons.org/publicdomain/zero
識別號： ISSN: 1680-7324
識別號： ISSN: 1680-7316
識別號： EISSN: 1680-7324
識別號： DOI: 10.5194/acp-16-15347-2016
&lt;br&gt;</description>
  </item>
  <item rdf:about="https://ir.lib.ncu.edu.tw/handle/987654321/101948">
    <title>Nano-structured CuO-Cu2O Complex Thin Film for Application in CH3NH3PbI3 Perovskite Solar Cells</title>
    <link>https://ir.lib.ncu.edu.tw/handle/987654321/101948</link>
    <description>title: Nano-structured CuO-Cu2O Complex Thin Film for Application in CH3NH3PbI3 Perovskite Solar Cells abstract: 摘要： Nano-structured CuO-Cu 2 O complex thin film-based perovskite solar cells were fabricated on an indium tin oxide (ITO)-coated glass and studied. Copper (Cu) thin films with a purity of 99.995 % were deposited on an ITO-coated glass by magnetron reactive sputtering. To optimize the properties of the nano-structured CuO-Cu 2 O complex thin films, the deposited Cu thin films were thermally oxidized at various temperatures from 300 to 400 °C. A CH 3 NH 3 PbI 3 perovskite absorber was fabricated on top of CuO-Cu 2 O complex thin film by a one-step spin-coating process with a toluene washing treatment. Following optimization, the maximum power conversion efficiency (PCE) exceeded 8.1 %. Therefore, the low-cost, solution-processed, stable nano-structured CuO-Cu 2 O complex thin film can be used as an alternative hole transport layer (HTL) in industrially produced perovskite solar cells.
其他題名： Nanoscale Res Lett
出版者： New York: Springer Science and Business Media LLC
出版日期： 2016-12
出處： Nanoscale Research Letters, 2016-12, Vol.11 (1), p.402--402, Article 402
資源來源： Publicly Available Content Database
版權： The Author(s). 2016
版權： Copyright Springer Nature B.V. Dec 2016
識別號： ISSN: 1931-7573
識別號： ISSN: 1556-276X
識別號： EISSN: 1556-276X
識別號： DOI: 10.1186/s11671-016-1621-4
識別號： PMID: 27637894
&lt;br&gt;</description>
  </item>
  <item rdf:about="https://ir.lib.ncu.edu.tw/handle/987654321/101945">
    <title>Nano-structured CuO-Cu2O Complex Thin Film for Application in CH3NH3PbI3 Perovskite Solar Cells</title>
    <link>https://ir.lib.ncu.edu.tw/handle/987654321/101945</link>
    <description>title: Nano-structured CuO-Cu2O Complex Thin Film for Application in CH3NH3PbI3 Perovskite Solar Cells abstract: 摘要： Nano-structured CuO-Cu 2 O complex thin film-based perovskite solar cells were fabricated on an indium tin oxide (ITO)-coated glass and studied. Copper (Cu) thin films with a purity of 99.995 % were deposited on an ITO-coated glass by magnetron reactive sputtering. To optimize the properties of the nano-structured CuO-Cu 2 O complex thin films, the deposited Cu thin films were thermally oxidized at various temperatures from 300 to 400 °C. A CH 3 NH 3 PbI 3 perovskite absorber was fabricated on top of CuO-Cu 2 O complex thin film by a one-step spin-coating process with a toluene washing treatment. Following optimization, the maximum power conversion efficiency (PCE) exceeded 8.1 %. Therefore, the low-cost, solution-processed, stable nano-structured CuO-Cu 2 O complex thin film can be used as an alternative hole transport layer (HTL) in industrially produced perovskite solar cells.
其他題名： Nanoscale Res Lett
出版者： New York: Springer Science and Business Media LLC
出版日期： 2016-12
出處： Nanoscale Research Letters, 2016-12, Vol.11 (1), p.402--402, Article 402
資源來源： Accès Université Paris-Saclay - PubMed Central Open Access
版權： The Author(s). 2016
版權： Copyright Springer Nature B.V. Dec 2016
識別號： ISSN: 1931-7573
識別號： ISSN: 1556-276X
識別號： EISSN: 1556-276X
識別號： DOI: 10.1186/s11671-016-1621-4
識別號： PMID: 27637894
&lt;br&gt;</description>
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