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<front>
<journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/amt-7-4103-2014</article-id>
<title-group>
<article-title>Recovering long-term aerosol optical depth series (1976–2012) from an astronomical potassium-based resonance scattering spectrometer</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Barreto</surname>
<given-names>A.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Cuevas</surname>
<given-names>E.</given-names>
<ext-link>https://orcid.org/0000-0003-1843-8302</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pallé</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Romero</surname>
<given-names>P. M.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Guirado</surname>
<given-names>C.</given-names>
<ext-link>https://orcid.org/0000-0002-4578-8204</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wehrli</surname>
<given-names>C. J.</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Almansa</surname>
<given-names>F.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Izaña Atmospheric Research Center, Meteorological State Agency of Spain (AEMET), Santa Cruz de Tenerife, Spain</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Cimel Electronique, Paris, France</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Instituto de Astrof\&apos;isica de Canarias (IAC), Santa Cruz de Tenerife, Spain</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Atmospheric Optics Group, Valladolid University (GOA-UVA), Valladolid, Spain</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Physikalisch-Meteorologisches Observatorium, Davos, World Radiation Center, Davos, Switzerland</addr-line>
</aff>
<pub-date pub-type="epub">
<day>03</day>
<month>12</month>
<year>2014</year>
</pub-date>
<volume>7</volume>
<issue>12</issue>
<fpage>4103</fpage>
<lpage>4116</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2014 A. Barreto et al.</copyright-statement>
<copyright-year>2014</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://amt.copernicus.org/articles/7/4103/2014/amt-7-4103-2014.html">This article is available from https://amt.copernicus.org/articles/7/4103/2014/amt-7-4103-2014.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/7/4103/2014/amt-7-4103-2014.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/7/4103/2014/amt-7-4103-2014.pdf</self-uri>
<abstract>
<p>A 37-year long-term
  series of monochromatic aerosol optical depth (AOD) has been
  recovered from solar irradiance measurements performed with the
  solar spectrometer Mark-I, deployed at Izaña mountain since
  1976. The instrument operation is based on the method of resonant
  scattering, which affords wavelength absolute reference and stability
  (long-term stability and high precision)
  in comparison to other instruments based purely on interference
  filters. However, it has been specifically designed as a reference
  instrument for helioseismology, and its ability to determine AOD from
  transmitted and scattered monochromatic radiation at 769.9 nm inside
  a potassium vapour cell in the presence of a permanent magnetic field
  is evaluated in this paper. Particularly, the use of an exposed
  mirror arrangement to collect sunlight as well as the
  Sun–laboratory velocity dependence of the scattered component
  introduces some important inconveniences to overcome
  when we perform the instrument&apos;s calibration. We have solved this problem
  using a quasi-continuous
  Langley calibration technique and a refinement procedure to correct
  for calibration errors as well as for the fictitious diurnal cycle
  on AOD data. Our results showed similar calibration errors retrieved
  by means of this quasi-continuous Langley technique applied in different
  aerosol load events (from 0.04 to 0.3),
  provided aerosol concentration remains constant
  throughout the calibration interval.  It assures the validity of this
  technique when it is applied in
  those periods with relatively high aerosol content. The comparative analysis
  between the recovered AOD data set from the Mark-I and collocated
  quasi-simultaneous data from the Cimel-AErosol RObotic NETwork (AERONET)
  and Precision Filter Radiometer (PFR) instruments showed an absolute
  mean bias &amp;leq; 0.01 in the 10- and 12-year comparison,
  respectively. High correlation coefficients between AERONET and Mark-I
  and PFR/Mark-I pairs confirmed a very good linear relationship
  between instruments, proving that recovered AOD data series from
  Mark-I can be used together with PFR and AERONET AOD data to build
  a long-term AOD data series at the Izaña site (1976–now), suitable for
  future analysis of aerosols trends and inter-annual
  variability. Finally, the AOD preliminary trend analysis in the
  29-year period from 1984 to 2012 with Mark-I AOD revealed no
  significant trends.</p>
</abstract>
<counts><page-count count="14"/></counts>
</article-meta>
</front>
<body/>
<back>
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