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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ESSD</journal-id>
<journal-title-group>
<journal-title>Earth System Science Data</journal-title>
<abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1866-3516</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/essd-8-165-2016</article-id><title-group><article-title>A long-term record of blended satellite and in situ sea-surface temperature for climate monitoring, modeling and environmental studies</article-title>
      </title-group><?xmltex \runningtitle{A long-term record of blended satellite and in situ sea-surface temperature}?><?xmltex \runningauthor{V.~Banzon et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Banzon</surname><given-names>Viva</given-names></name>
          <email>viva.banzon@noaa.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Smith</surname><given-names>Thomas M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Chin</surname><given-names>Toshio Mike</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Liu</surname><given-names>Chunying</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff4">
          <name><surname>Hankins</surname><given-names>William</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>NOAA National Centers for Environmental Information (NCEI), 151 Patton Ave., Asheville, NC 28801, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>NOAA/STAR/SCSB/ESSIC University of Maryland, College Park, MD 20740, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Earth Resources Technology, 14401 Sweitzer Lane Suite 300, Laurel, MD 20707, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Viva Banzon (viva.banzon@noaa.gov)</corresp></author-notes><pub-date><day>28</day><month>April</month><year>2016</year></pub-date>
      
      <volume>8</volume>
      <issue>1</issue>
      <fpage>165</fpage><lpage>176</lpage>
      <history>
        <date date-type="received"><day>17</day><month>December</month><year>2015</year></date>
           <date date-type="rev-request"><day>19</day><month>January</month><year>2016</year></date>
           <date date-type="rev-recd"><day>5</day><month>April</month><year>2016</year></date>
           <date date-type="accepted"><day>8</day><month>April</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016.html">This article is available from https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016.html</self-uri>
<self-uri xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016.pdf</self-uri>


      <abstract>
    <p>This paper describes a blended sea-surface temperature
(SST) data set that is part of the National Oceanic and Atmospheric
Administration (NOAA) Climate Data Record (CDR) program product suite. Using
optimum interpolation (OI), in situ and satellite observations are combined
on a daily and 0.25<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial grid to form an SST analysis, i.e., a
spatially complete field. A large-scale bias adjustment of the input
infrared SSTs is made using buoy and ship observations as a reference. This
is particularly important for the time periods when volcanic aerosols from
the El Chichón and Mt. Pinatubo eruptions are widespread globally. The main
source of SSTs is the Advanced Very High Resolution Radiometer (AVHRR),
available from late 1981 to the present, which is also the temporal span of
this CDR. The input and processing choices made to ensure a consistent
data set that meets the CDR requirements are summarized. A brief history and
an explanation of the forward production schedule for the preliminary and
science-quality final product are also provided. The data set is produced and
archived at the newly formed National Centers for Environmental Information
(NCEI) in Network Common Data Form (netCDF) at <ext-link xlink:href="http://dx.doi.org/10.7289/V5SQ8XB5" ext-link-type="DOI">10.7289/V5SQ8XB5</ext-link>.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Sea-surface temperature (SST) is an essential climate variable (ECV). The
Global Climate Observing System (GCOS) project developed a list of ECVs to
focus worldwide observation efforts on a limited set of variables that are
climate relevant, technically feasible, and cost effective (Bojinski et al.,
2014). Collectively, ECVs can help develop adaptation and mitigation
strategies, assess risks, allow attribution and prediction, and support
climate services. SST is useful for monitoring El Niño events and
multi-decadal ocean changes. It is also relevant to quantification and
modeling of many other aspects of climate such as air–sea interaction, ocean
acidification to determine solubility of carbon dioxide, biophysical
processes, and marine organism distributions. However, models require not
just observations but also complete data fields, also referred to as analyses.
Today, satellites offer high spatial and temporal coverage and are,
therefore, the main source of SST observations. Additional processing is
applied to satellite data to form analyses to allow for bias corrections and
gap-filling and thereby increase spatiotemporal consistency.</p>
      <p>The objective of this work is to describe the National Oceanic and
Atmospheric Administration (NOAA) 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
daily Optimum Interpolation SST version 2 (or dOISST.v2,
herein), an analysis that has been selected by the NOAA Climate Data Record (CDR) program as an
operational CDR. This implies that the dOISST.v2 meets the definition of CDR
put forward by the National Research Council (2004): it is of sufficient
length, consistency, and continuity to determine climate variability.
Furthermore, operational NOAA CDRs undergo a research-to-operations process
to ensure systematic production and quality assessment, thereby increasing
the data set maturity in aspects like transparency, usability, and data
preservation following metadata standards. A preliminary assessment using
the maturity matrix of Bates and Privette (2012) indicated that dOISST.v2
has a high maturity in both science and applications, but it needed
improvements in accessibility and transparency to users. As part of the
effort to address this deficiency, this paper describes the dOISST.v2 CDR
data set, in the context of its historical beginnings and evolution,
current temporal and spatial characteristics, and data set formats and access, and provides examples of applications. Much of this information is
publicly available but has not been summarized in a single document.</p>
</sec>
<sec id="Ch1.S2">
  <title>Historical background</title>
      <p>Here, precursors to the dOISST.v2 that have evolved into the current CDR are
briefly reviewed to highlight the original motivation and subsequent
modifications. Historically, the widely-used name “Reynolds SST” has been
applied to all current and precursor products, and is therefore ambiguous
and not used here. Reynolds (1988) first introduced the concept of a blended
SST analysis that takes advantage of the sea truth offered by in situ data
and the high coverage of satellite data. Prior to 1980, ships were the only
source of observations, and the spatial–temporal coverage was sufficient
only for a coarse-scale analysis. Starting in late 1981, satellite-based SST
observations became available daily from an infrared instrument, the
Advanced Very High Resolution Radiometer (AVHRR), with Global Area Coverage
(GAC) resolution at <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4 km. Using high-quality drifting buoys
as reference, Reynolds (1988) found that monthly analyses, based on AVHRR
SSTs alone or blended with in situ data, were slightly more accurate than
those based on in situ data alone (with drifter data withheld). However, for
infrared SSTs, notable satellite biases can occur under specific situations,
e.g., at cloud edges or dust plumes (e.g., Bogdanoff et al., 2015;
Vázquez-Cuervo et al., 2004). On a global scale, significant widespread
biases have also been observed in the presence of volcanic aerosols,
especially following the Mt Pinatubo and El Chichón eruptions, with AVHRR
SSTs cooler than in situ observations by over 1 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Zhang et al.,
2004; Reynolds, 1988, 1993). For these post-eruption periods,
reliable global SST fields could be produced if in situ data were used to
benchmark the satellite data to form blended analyses (Reynolds, 1988;
Reynolds and Marisco, 1993). This large-scale benchmarking is also referred
to as a “satellite bias adjustment”.</p>
      <p>Reynolds and Smith (1994) adopted the optimum interpolation (OI) method to
increase the effective resolution of the blended analysis to 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
and the temporal frequency from monthly to weekly and later to daily. This
was the first time the name OISST was used. Along the marginal ice zone
where observations were sparse, the interpolation was relaxed to the
freezing point of seawater (<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.8 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). This was slightly modified
in the follow-up version 2 (also referred to as OI.V2 in Reynolds et al.,
2002), where a regression equation was used to estimate proxy SSTs from sea-ice concentrations. NCEP continues to produce the 1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> weekly OI.V2
for seasonal forecasting. The next section describes the original and
current versions of dOISST. The core methodology for both versions is
described in Reynolds et al. (2007). Appendix A presents minor improvements
made by Reynolds in response to feedback from users (mostly added smoothing
to reduce noise) and to extend the series back to 1981. Note that Appendix A
contains material from Reynolds (2009), an online document, and has been
included in this paper for preservation purposes.</p>
</sec>
<sec id="Ch1.S3">
  <title>The climate data record</title>
      <p>Reynolds et al. (2007) introduced major methodological changes to increase
the OISST resolution to the current daily, 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid.
The new bias correction scheme employed empirical orthogonal teleconnections
(EOTs) modes rather than the Poisson method used in the weekly OI.V2. The
use of EOTs also had the additional advantage of allowing estimation of
the bias error. Moreover, the earlier OISST analyses used operational (i.e.,
near-real-time) satellite data, but for the 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
daily OISST higher-quality input data sets reprocessed from the start of the
mission were used preferentially over operational data. Most significant was
the AVHRR Pathfinder reprocessing, which improved SST retrievals using
nighttime buoy data to compute a revised set of coefficients for each NOAA
satellite (e.g., Kilpatrick et al., 2001; Casey et al., 2010; Vázquez-Cuervo
et al., 2010). However, the cold bias associated with the eruptions of El
Chichón and Mt. Pinatubo remained a challenge even in the more recent AVHRR
SST reprocessing efforts. Another change from the weekly OI.V2 was that the
proxy SST calculation was restricted closer to the ice margin, i.e., where
sea-ice concentrations exceed 50 %, to avoid potentially erroneous SST
estimates in the more open waters, where the fit was much noisier.</p>
      <p>Reynolds et al. (2007) referred to the above product as AVHRR-only, in
reference to the source of satellite SSTs. The same paper describes a
companion analysis that uses the same methodology but includes data from the
Advanced Microwave Scanning Radiometer on the Earth Observing System
(AMSR-E). This product, called AVHRR<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>AMSR, is not a CDR, due to the short
period of record (2002 to 2011) of AMSR-E data. It should be noted that the
Climate Forecast System Reanalysis (CFSR) at NCEP uses the same Reynolds et
al. (2007) methodology to generate their initial SST fields (Saha et al.,
2010, 2014), but may use different inputs (e.g., both infrared and microwave
satellite SSTs, like the AVHRR<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>AMSR) over time and therefore will differ
from this CDR.</p>
      <p>As discussed in Appendix A, the 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> daily OISST was
upgraded to version 2 primarily to increase temporal stability and to
include Pathfinder AVHRR data from 1981 to 1985 that had become available
(Casey et al., 2010). The treatment of in situ data was slightly modified.
Historically, in situ observations were predominantly from ships. In the
21st century, more accurate buoy data had become increasingly dominant
over ship data, providing a better reference temperature. A constant
(<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.14 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) was subtracted from the ship data to
compensate for the global-average ship–buoy difference (Reynolds and Chelton,
2010; Appendix A). Modern ship measurements tend to be warmer because they
typically use intake samples that can be warmed when taken into the ship
engine room. However, there is much scatter in individual differences and
better understanding of ship bias is needed to reduce the uncertainty in
this correction. The net effect of this adjustment is that the daily OISST
tends to be cooler than the weekly OI.V2 particularly in the 1980s and 1990s
when ship data were dominant, making the long-term trend slightly steeper.
Some of the differences between the current weekly OI.V2 and the current
CDR, i.e., the dOISST.v2, including the impact on trends and climatologies,
are discussed in greater detail in Banzon et al. (2014) and Huang et al. (2016).</p>
<sec id="Ch1.S3.SS1">
  <title>Data set description</title>
      <p>The daily OISST is available in netCDF and binary (FORTRAN IEEE big-endian)
formats. In this paper, the archived netCDF files, publicly available at the
National Centers for Environmental Information (NCEI) website, are
described. However, the same data are repackaged and distributed elsewhere
for specific projects or organizations such as the Group for High Resolution
SST (or GHRSST) and Observations for Model Intercomparison Projects
(Obs4MIPs), with accompanying metadata and documentation, but are not
described here. The heritage binary format will be eventually phased out.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Examples of the four variables in a singles file: <bold>(a)</bold> dOISST.v2,
<bold>(b)</bold> dOISST anomaly, <bold>(c)</bold> error, and <bold>(d)</bold> median sea-ice
concentrations. Data are shown for 20 June 2015.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f01.png"/>

        </fig>

      <p>A single netCDF file contains four global gridded fields (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>1440</mml:mn><mml:mo>×</mml:mo><mml:mn>720</mml:mn></mml:mrow></mml:math></inline-formula>)
pertaining to 1 day. The primary variable is the analyzed SST (units in <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C;
Fig. 1a). Since buoys are used as a reference, this is
sometimes referred to as a “bulk” SST, at a nominal buoy depth of 1 m. The
SST input data types (AVHRR daytime, AVHRR nighttime, buoys, ships, proxy
SST; Table 1) are first averaged to 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> superobservations. The in
situ data (consisting of the buoy and adjusted ship data) are collectively
used to make large-scale adjustments to satellite data using the EOT modes.
All data are merged during the interpolation, using the pre-computed error
characteristics as weights. More details can be found in Reynolds et al. (2007).
Grid points corresponding to land, permanent ice shelves, and most
inland waters are not processed and assigned a missing value of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>999.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Input data sets to the daily OISST version 2. The data sources are
explained in detail in Reynolds et al. (2007). For version 1, ICOADS 2.1 was
used.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Input type</oasis:entry>  
         <oasis:entry colname="col2">Reprocessed or higher-quality data sets</oasis:entry>  
         <oasis:entry colname="col3">Operational data sets</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Satellite (AVHRR SSTs)</oasis:entry>  
         <oasis:entry colname="col2">Pathfinder 5.0/5.1 (1981–2006)</oasis:entry>  
         <oasis:entry colname="col3">Navy (2007–present)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">In situ SSTs</oasis:entry>  
         <oasis:entry colname="col2">ICOADS 2.4 (1981–2006)</oasis:entry>  
         <oasis:entry colname="col3">NCEP (2007–present)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Sea-ice concentrations</oasis:entry>  
         <oasis:entry colname="col2">GSFC NASA (1981–2004)</oasis:entry>  
         <oasis:entry colname="col3">NCEP (2005–present)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>Three other gridded fields at the same 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial resolution
complement the daily analysis.
<list list-type="bullet"><list-item>
      <p>Anomalies (i.e., the daily OISST minus the 1971–2000 climatological mean;
units in <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; Fig. 1b) represent departures from “normal” or
average conditions. The anomalies are provided so users can easily compute
climate indices, such as the NINO3.4 (Fig. 2a). The 1971–2000 climatology is
partly based on an in situ analysis for the years that satellite data are
not available (1971–1981) and on the weekly OISST for years satellite data
are available from 1982 onward (Xue et al., 2003). A climatological mean
computed from daily OISST (1982–2011) is now available and is more suitable
to use with this data set, as explained in Banzon et al. (2014). It will be
used in the next version. User should consider that with a long-term
warming, a more recent period may produce a warmer climatological mean;
thus, when subtracted from the analyzed SSTs, it produces cooler anomalies.</p></list-item><list-item>
      <p>The standard error (with units in <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; Fig. 1c) provides a measure
of uncertainty in the estimated SST, allowing users to exclude (using a
threshold) or to minimize (using weights) the importance of grid point
values with greater errors, as needed for the specific application, e.g.,
resource management, risk analysis, or assimilation into a model.</p></list-item><list-item>
      <p>The 7-day median of daily sea-ice concentrations (expressed as a real
fraction from 0.0 to 1.0; Fig. 1d) is the basis of the proxy SST estimate in
the marginal ice zone. Aside from reducing noise, the temporal median
populates the time series in the early 1980s when satellite sea-ice
observations were available only every other day. There are no sea-ice data
from 4 December 1997 to 14 January 1998. This field is effectively also an
ice mask when the user opts to exclude areas with high ice concentrations.</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p><bold>(a)</bold> Temporal progression of the 1997 daily OISST in the NINO3.4
region (solid line) and the 1982–2011 climatological mean (short dash) for
the same area. The offset from the mean by plus and minus 1 standard
deviation (long dash) shows characteristic variability. <bold>(b)</bold> Same but in 2012
in the Gulf of Maine (after Mills et al., 2013). Titles show coordinates
used to compute the area weighted means.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f02.pdf"/>

        </fig>

      <p>The input data sets to dOISST.v2 are listed in Table 1 and have been
evaluated in more detail in Reynolds et al. (2007). While reprocessed inputs
are used whenever possible, only operational data sets meet the low latency
needs of the daily updates. Users should be aware that sensor problems are
typically cannot be addressed in near real time. The release date of the
dOISST.v2 was November 2008. To minimize the impact of near-real-time sensor
problems, data from two AVHRRs are used from 2007 onward (Table 2).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><caption><p>Platform time spans of AVHRR inputs to the daily OISST. Note that
two satellites at a time are used beginning January 2007.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.90}[.90]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Data set</oasis:entry>  
         <oasis:entry colname="col2">Start date</oasis:entry>  
         <oasis:entry colname="col3">End date</oasis:entry>  
         <oasis:entry colname="col4">Platform</oasis:entry>  
         <oasis:entry colname="col5">Sensor</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Pathfinder</oasis:entry>  
         <oasis:entry colname="col2">24 Aug 1981</oasis:entry>  
         <oasis:entry colname="col3">3 Jan 1985</oasis:entry>  
         <oasis:entry colname="col4">NOAA-7</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">4 Jan 1985</oasis:entry>  
         <oasis:entry colname="col3">7 Nov 1988</oasis:entry>  
         <oasis:entry colname="col4">NOAA-9</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">8 Nov 1988</oasis:entry>  
         <oasis:entry colname="col3">13 Sep 1994</oasis:entry>  
         <oasis:entry colname="col4">NOAA-11</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">14 Sep 1994</oasis:entry>  
         <oasis:entry colname="col3">21 Jan 1995</oasis:entry>  
         <oasis:entry colname="col4">NOAA-9</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">22 Jan 1995</oasis:entry>  
         <oasis:entry colname="col3">11 Oct 2000</oasis:entry>  
         <oasis:entry colname="col4">NOAA-14</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/2</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">12 Oct 2000</oasis:entry>  
         <oasis:entry colname="col3">31 Dec 2002</oasis:entry>  
         <oasis:entry colname="col4">NOAA-16</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">1 Jan 2003</oasis:entry>  
         <oasis:entry colname="col3">4 Jun 2005</oasis:entry>  
         <oasis:entry colname="col4">NOAA-17</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">5 Jun 2005</oasis:entry>  
         <oasis:entry colname="col3">31 Dec 2006</oasis:entry>  
         <oasis:entry colname="col4">NOAA-18</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Navy</oasis:entry>  
         <oasis:entry colname="col2">1 Jan 2006</oasis:entry>  
         <oasis:entry colname="col3">31 Dec 2008</oasis:entry>  
         <oasis:entry colname="col4">NOAA-17</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">1 Jan 2007</oasis:entry>  
         <oasis:entry colname="col3">15 Aug 2011</oasis:entry>  
         <oasis:entry colname="col4">NOAA-18</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">1 Jan 2009</oasis:entry>  
         <oasis:entry colname="col3">Present</oasis:entry>  
         <oasis:entry colname="col4">MetOP-A</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">16 Aug 2011</oasis:entry>  
         <oasis:entry colname="col3">Present</oasis:entry>  
         <oasis:entry colname="col4">NOAA-19</oasis:entry>  
         <oasis:entry colname="col5">AVHRR/3</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p>The analysis for the first day in the record used climatology as a first
guess. For all other days the previous analysis is used as a first guess.
For the daily update, a 1-day delayed analysis is produced. Two weeks later,
after more data have become available, the analysis is repeated to produce
higher-quality “final” product. The final and preliminary runs can be
identified in the global attributes of the netCDF file, and the preliminary
filename also contains the word “preliminary”. Only the “final” product
is archived.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Basic characterization</title>
      <p>The daily OISST is available for the full period of record from
September 1981 to the present. The data set is similar to other global daily
SST analyses in that monthly, seasonal, and multi-year averages can be computed
on global, regional, and local scales. For climate applications, the daily
OISST is unique because it extends from late 1981 to the present and
therefore spans over 30 years, often cited as the minimum period needed to
distinguish interannual variations from long-term variations. The
characteristic seasonal SST cycle, represented here by the 1982–2011
climatological mean, varies by location. In the tropics, it is exemplified
by the NINO3.4 region (Fig. 1a), where the seasonal signal is weak. The
start of the 1997 El Niño event is marked by SSTs that are more than 1
standard deviation greater than the climatological mean for over 3
months. A stronger seasonal cycle occurs in the temperate zone, as seen in
the Gulf of Maine (Fig. 2b). The SSTs over the entire year 2012 exceed the
climatological mean plus 1 standard deviation. The daily progression shows
particularly elevated May–June temperatures, which initiated a season of
anomalous lobster catch (Mills et al., 2013). Of course, these atypical
events can also investigated by examining the anomalies.</p>
      <p>Long time series are ideal for computing multi-decadal trends. On an annual
scale, the 1982 to 2014 global linear trend using dOISST is <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.12 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
per decade. The wintertime trend is slightly smaller
(0.09 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per decade using only January monthly averages; Fig. 3a)
than in summertime (0.14 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C per decade using only July monthly
averages; Fig. 3b). The 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution data allow
trends to be computed on more local scales, but comparisons should always be
made with in situ measurements, if available. The daily SST information can
be used to generate other climate-relevant parameters. For example, the
number of days that SSTs are above a threshold, also known as degree days,
is an indicator of thermal stress for corals. In fact, many ecological
responses to a changing ocean can be modeled in terms of the cumulative
effect of daily temperatures on growth, reproduction, recruitment, and the
like.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Global OISST trends (1982–2014) using <bold>(a)</bold> January monthly means
only and <bold>(b)</bold> July monthly means only.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f03.pdf"/>

        </fig>

      <p>Global validation of the dOISST using buoy and ship data is not an
independent assessment because in situ data are used to make the product,
although the amount of satellite data incorporated is much greater.
Comparisons with other SST analyses would have the same issue since most
analyses also use in situ data. With that caveat, Reynolds and Chelton
(2010) showed that, relative to buoys, the dOISST.v2 and other analyses all
exhibit regional variability in performance, reflecting their methodological
differences. For the dOISST.v2, the root-mean-square error relative to the
buoys is about 0.3 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Reynolds and Chelton (2010) also found
that the product degrades in quality during prolonged periods of no data,
e.g., seasonally cloud-covered areas such as the Gulf Stream in winter.
Analyses that included microwave data had better results when infrared
retrievals were not available, because of the added data coverage. However, when
infrared data were available, the addition of microwave data reduced the
quality of the resulting analyses because microwave SSTs are less accurate.
In any case, an analysis is not necessarily the best source of SST for a
single point in space or time because it is a smoothed product. The
advantage is that where there are no observations, an analysis provides
interpolated values and, over time, a consistent long-term record. It should
be noted that the analysis is also useful as a reference field for
identifying bad data and is therefore used in several satellite algorithms
for quality control. It also serves as a first guess or as ancillary data
for computing parameters that require a known temperature field.</p>
      <p>Argo data, which are not used as an input to dOISST, can also be used for
validation. However, Argo observations are available only after 2000 and
are located deeper (<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4 m) than surface buoy measurements. As
agreed on by the GHRSST community, most SST analyses do not incorporate Argo
data in order to have a common independent validation data set.
Martin et al. (2012) used Argo data for the year 2010 to compare different near-real-time
SST data sets, including the preliminary dOISST (defined in Sect. 3.1), and
their collective median. All data sets had a standard deviation below 0.7 K
relative to Argo data. Most, including dOISST, had an overall bias between
0.2 to 0.4 K. Certainly, as the Argo data set grows, it might be possible to
withhold only a portion for validation and use the rest in the analysis.
For a future version of dOISST, Argo data could improve data coverage in
areas with sparse ship and buoy data such as the Tropical Pacific, where
moored buoy data were degraded for some years.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Power spectra of three analyzed SST fields from the first 2
months of 2016. See text for explanation of data sets used. At smaller
scales, the spectrum of the RSS product that ingests high-resolution inputs
(1 km MODIS SSTs) continues to display the same spectral slope into the
smaller-scale range. MODIS SSTs are available only from 1999.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f04.pdf"/>

        </fig>

      <p>In terms of feature resolution, i.e., the ability of an analysis to
reproduce mesoscale ocean features and capture SST gradients, Reynolds et
al. (2007) showed dOISST performs well. Reynolds and Chelton (2010) also
found that feature resolution of an analysis is not necessarily related to
the grid size. To illustrate this point here, the power spectral densities
of three SST data sets examined by Reynolds and Chelton (2010) are shown
(Fig. 4). The plot is similar to Reynolds and Chelton (2010) except that the
latest versions of the three data sets (from the first 2 months of 2016)
are used and the spectra are smoother because they are the average of
several areas rather than a single area, in order to provide a global
representation of each data set. The three products shown differ in grid
resolutions: dOISST is on a 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid, the Operational SST and Sea
Ice Analysis (OSTIA) is on a 1/20<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid
(<ext-link xlink:href="http://dx.doi.org/10.5067/GHOST-4FK01" ext-link-type="DOI">10.5067/GHOST-4FK01</ext-link>; UK Met Office, 2005), and the Remote Sensing Systems
(RSS) analysis is computed on a 1/11<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid
(<ext-link xlink:href="http://dx.doi.org/10.5067/GHMWI-4FR01" ext-link-type="DOI">10.5067/GHMWI-4FR01</ext-link>; Remote Sensing Systems, 2008). All spectra indicate identical
large-scale (and perhaps seasonal) SST patterns at wavelengths larger than
1500 km. All spectra also show similar slopes (of <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2) in the mesoscale
range down to about 300 km wavelength. At shorter scales (&lt; 200 km),
the power spectra for dOISST and OSTIA are nearly identical even when the
latter has a finer grid size. In comparison, the RSS product resolves
finer-scale features as indicated by the more gradual drop off.</p>
      <p>In general, the higher-resolution SST analyses combine higher-resolution
infrared data (with low spatial coverage due to inability to penetrate
clouds) and lower-resolution but more spatially complete microwave data,
which have quasi-all-weather coverage (e.g., Vázquez-Cuervo et al., 2013).
The ability to provide good feature resolution in a particular area is
constrained by the availability of finer resolution (<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 km)
infrared data and the use of a methodology that preserves that information.
Thus, even though the average spectra may show an ability to resolve fine
features, products tend to be smoother in areas where only microwave data are
available (Vázquez-Cuervo et al., 2013). High-resolution artifacts may also
be created due to insufficient data (Reynolds and Chelton, 2010).</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p>A long-term sea-surface temperature climate data record consisting of in
situ and satellite data blended daily on a 1/4<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid
is available for climate monitoring, modeling, validation, and a wide range
of other applications. The data set uses AVHRR data from 1981 to the present,
bias-adjusted relative to situ data. This produces a time series that is
more consistent than satellite infrared retrievals alone. This CDR is
produced, distributed, and generated by the NCEI, a newly formed entity that is a merger of
three NOAA data centers including the National Climatic Data Center (NCDC),
which originally produced this data set.</p>
      <p>Compared to the precursor weekly OISST at NCEP, the CDR has many updates
including higher spatial resolution, reprocessed inputs, and adjustment of
ship data to match buoys. The CDR is also used as an ancillary field in
reprocessed and operational satellite algorithms including the Pathfinder
AVHRR SST, Tropical Rainfall Measuring Mission (TRMM) rain rate, and
Aquarius salinity. The CDR version of the dOISST.v2 is available in netCDF
format <ext-link xlink:href="http://dx.doi.org/10.7289/V5SQ8XB5" ext-link-type="DOI">10.7289/V5SQ8XB5</ext-link> (Reynolds et al., 2008).</p>
<sec id="Ch1.S4.SSx1" specific-use="unnumbered">
  <title>Data availability</title>
      <p>The dOISST.v2 data set described in this paper is available at the National
Centers for Environmental Information, under the name “NOAA Optimum
Interpolation 1/4 Degree Daily Sea Surface Temperature (OISST) Analysis,
Version 2” with <ext-link xlink:href="http://dx.doi.org/10.7289/V5SQ8XB5" ext-link-type="DOI">10.7289/V5SQ8XB5</ext-link>. The data are also available in a
different format at the Physical Oceanography Distributed Active Archive
Center (PODAAC) at the Jet Propulsion Laboratory (JPL) under the name
“GHRSST Level 4 AVHRR_OI Global Blended Sea Surface Temperature Analysis”,
with <ext-link xlink:href="http://dx.doi.org/10.5067/GHAAO-4BC01" ext-link-type="DOI">10.5067/GHAAO-4BC01</ext-link>. The two other SST products used for
comparisons in Fig. 4 are also available at the PODAAC. The “GHRSST Level 4
mw_ir_OI Global Foundation Sea Surface Temperature analysis” has
<ext-link xlink:href="http://dx.doi.org/10.5067/GHMWI-4FR01" ext-link-type="DOI">10.5067/GHMWI-4FR01</ext-link>. The “GHRSST Level 4 OSTIA Global Foundation Sea
Surface Temperature Analysis” has <ext-link xlink:href="http://dx.doi.org/10.5067/GHOST-4FK01" ext-link-type="DOI">10.5067/GHOST-4FK01</ext-link>.</p><?xmltex \hack{\clearpage}?>
</sec>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <title>What's new in version 2</title>
      <p>By Richard W. Reynolds, 30 January 2009</p>
<sec id="App1.Ch1.S1.SS1">
  <title>Introduction</title>
      <p>The purpose of this note is to discuss the upgrade of the version 1 (v.1)
daily OI SST analysis
(Reynolds et al., 2007) to version 2 (v.2). These changes are relatively
small and mostly consist of additional temporal smoothing. In addition,
preliminary Pathfinder data (following Kilpatrick et al., 2001) have been
processed using NOAA-7. This allows the analysis to be extended backward in
time. The daily OI AVHRR-only v2 analysis now begins on 1 September 1981;
v1 began on 4 January 1985.</p>
</sec>
<sec id="App1.Ch1.S1.SS2">
  <title>Modifications version 2</title>
      <p>Other than the extension of v2 backward in time to September 1981, there are
seven analysis changes in v.2.</p>
<sec id="App1.Ch1.S1.SS2.SSS1">
  <title>Temporal smoothing of daily OI data</title>
      <p>Day-to-day analysis differences are discussed by Reynolds et al. (2007) on
page 5491 and illustrated there in Fig. 13 by four partial snap shots of the
Gulf Stream from the AMSR and the
AVHRR instruments during 1 day.
The day-to-day differences are due to a limited number of observations in
regions of high variability. Observations are limited by the spatial width
of the satellite swath as well as by cloud cover for AVHRR and by
precipitation and the vicinity of land for AMSR.</p>
      <p>In v.1 observations used in the daily OI were taken from the day analyzed.
To temporally smooth the analysis, 3 days of data were used where the off
days (the day before and after the analysis day) have doubled noise-to-signal
ratios (standard deviation) compared to the center day. The doubled
noise-to-signal ratio reduces the impact of the off days.</p>
      <p>See Reynolds et al. (2007) page 5480 for a discussion of noise-to-signal
ratios.</p>

<?xmltex \floatpos{t}?><table-wrap id="App1.Ch1.T1"><caption><p>The linear least squares fit of the ship and buoy data shown in
Fig. A2.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Period</oasis:entry>  
         <oasis:entry colname="col2">Slope</oasis:entry>  
         <oasis:entry colname="col3">Intercept</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">1989–1997</oasis:entry>  
         <oasis:entry colname="col2">0.988</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.136 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1998–2006</oasis:entry>  
         <oasis:entry colname="col2">0.924</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.118 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1989–2006</oasis:entry>  
         <oasis:entry colname="col2">0.965</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.133 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="App1.Ch1.T2"><caption><p>Comparison of different versions.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.90}[.90]?><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Feature</oasis:entry>  
         <oasis:entry colname="col2">V.1</oasis:entry>  
         <oasis:entry colname="col3">Interim V.2</oasis:entry>  
         <oasis:entry colname="col4">Final V.2</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Time delay</oasis:entry>  
         <oasis:entry colname="col2">1 day</oasis:entry>  
         <oasis:entry colname="col3">1 day</oasis:entry>  
         <oasis:entry colname="col4">14 days</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Days of data in OI</oasis:entry>  
         <oasis:entry colname="col2">1 day</oasis:entry>  
         <oasis:entry colname="col3">1 day</oasis:entry>  
         <oasis:entry colname="col4">3 days</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Ship bias correction</oasis:entry>  
         <oasis:entry colname="col2">No</oasis:entry>  
         <oasis:entry colname="col3">Yes</oasis:entry>  
         <oasis:entry colname="col4">Yes</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Preliminary zonal bias</oasis:entry>  
         <oasis:entry colname="col2">No</oasis:entry>  
         <oasis:entry colname="col3">Yes</oasis:entry>  
         <oasis:entry colname="col4">Yes</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Smoothing of EOT modes</oasis:entry>  
         <oasis:entry colname="col2">No</oasis:entry>  
         <oasis:entry colname="col3">No</oasis:entry>  
         <oasis:entry colname="col4">5 days</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Days of data in EOT bias</oasis:entry>  
         <oasis:entry colname="col2">7 days</oasis:entry>  
         <oasis:entry colname="col3">7 days</oasis:entry>  
         <oasis:entry colname="col4">15 days</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">AMSR data improved</oasis:entry>  
         <oasis:entry colname="col2">No</oasis:entry>  
         <oasis:entry colname="col3">Yes</oasis:entry>  
         <oasis:entry colname="col4">Yes</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Start AVHRR-only OI</oasis:entry>  
         <oasis:entry colname="col2">Jan 1985</oasis:entry>  
         <oasis:entry colname="col3">Replaced</oasis:entry>  
         <oasis:entry colname="col4">Sep 1981</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Start AMSR<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>AVHRR OI</oasis:entry>  
         <oasis:entry colname="col2">Jun 2002</oasis:entry>  
         <oasis:entry colname="col3">Replaced</oasis:entry>  
         <oasis:entry colname="col4">Jun 2002</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p>To verify the impact of this smoothing, 43 moored buoys were selected which
had daily data for at least 99 % of the days for the period 2003–2005. These
buoys were located off the coasts of North America and Europe and in the
tropical Pacific and Atlantic. Auto spectra were computed for the 2003–2005
period at each of buoy locations from the daily-averaged buoy data and from
four daily OI analyses: the OI using either only AVHRR or AMSR and AVHRR data
with 1 day or 3 days of data. The spatial averaged spectra are shown in Fig. A1. The low frequencies (&lt; 0.2 cycles per day) are nearly identical.
The buoy data and the 3-day OI analyses have similar variances at higher
frequencies although the buoy variance is being slightly higher. However,
the 1-day OI analyses have considerably larger variance at higher
frequencies than the others.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F1"><caption><p>Globally averaged daily spectra for 2003–2005 computed at 43 moored
buoy locations and averaged. “AVHRR-only” and “AMSR<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>AVHRR” indicate daily
OI spectra using either 1 day or 3 days of data. “Buoy” indicates spectra
using daily buoy data.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f05.pdf"/>

          </fig>

</sec>
<sec id="App1.Ch1.S1.SS2.SSS2">
  <title>Ship SST biases with respect to buoys</title>
      <p>As discussed in Reynolds et al. (2007), the random and bias errors of ship
SST data are larger than the random and bias errors of buoy SSTs.
Furthermore, as shown in Fig. A2 from Reynolds et al. (2002), the coverage of
buoys tends to increase with time while the coverage of ship tends to
decrease. To determine the variability of a globally averaged bias, monthly
averaged ship biases were computed with respect to buoys. However, even with
temporal smoothing, differences occurred at irregular intervals and did not
seem to be related to seasonal or El Niño–Southern Oscillation events.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F2"><caption><p>Scatter plot of global collocated average monthly ship vs. buoy
anomaly for January 1989–December 2006. The first 9 years are shown in the
black and the second 9 years in red. Least squares linear fits for the two
periods are also shown.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f06.pdf"/>

          </fig>

      <p>Monthly scatter plots of the collocated average global ship and buoy anomaly
SSTs are shown in Fig. A2 for two 9-year periods. The least squares linear
fit for the two periods is also shown with the slope and intercept given in
Table A1. These results strongly suggest that a spatial and temporal
constant bias correction is needed. However, finer space and time
corrections do not seem to be possible with the limited in situ data
available. The fit indicates that the average intercept is <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.13 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.
When the average global difference are computed directly, the average
buoy minus ship difference is found to <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.14 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. As differences of
0.01 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C are not significant, 0.14 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C was subtracted from
all ship data before they are used in the satellite bias correction and in
the OI analysis. No correction was made for the buoy data.</p>
</sec>
<sec id="App1.Ch1.S1.SS2.SSS3">
  <title>Zonal satellite bias correction</title>
      <p>As discussed on page 5482 of Reynolds et al. (2007), the daytime and
nighttime satellite observations are adjusted to the daily average of the in
situ (ship and buoy) data. This is done using EOTs which are similar to rotated empirical orthogonal
functions. The method produces an anomaly SST EOT for in situ data, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>I</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
and an anomaly SST EOT for satellite data, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> are the
longitude and latitude coordinates, respectively. The bias, <inline-formula><mml:math display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula>, is defined as
the difference: <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>I</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Only EOT modes which are
adequately sampled by both in situ and  satellite data are used. In
regions where there are no EOT modes, the anomalies and hence the biases are
0.</p>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F3"><caption><p>Average July 2006 difference between the daily AVHRR-only OI
using Pathfinder NOAA-17 data and operational Navy NOAA-17 data. All
versions use bias-corrected satellite data. In the top panel the Pathfinder
daily OI uses no preliminary zonal bias correction; in the bottom panel the
Pathfinder daily OI uses a preliminary zonal bias correction.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f07.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F4"><caption><p>Spatially averaged nighttime AVHRR bias correction spectra for
2000–2005. Binomial three-point, five-point, and seven-point temporal smoothing are
shown; an unsmoothed version is labeled “Nt 1 Fld”.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f08.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F5"><caption><p>Daily OI Nino-3 anomalies using EOT bias correction with 15 and 7
days of data. “N-7” indicates that NOAA-7 satellite SST data are used.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f09.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.F6"><caption><p>AMSR extra quality-controlled SST data anomalies for 9 February
2003. The black regions show where data have been rejected by the extra
quality control.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://essd.copernicus.org/articles/8/165/2016/essd-8-165-2016-f10.png"/>

          </fig>

      <p>Figure 12 from Reynolds et al. (2002) shows that Pathfinder AVHRR SSTs have
cold biases with respect to operational Navy AVHRR. If the bias correction
has a residual, long-term differences will indicate it. This is shown in the
upper panel of Fig. A3 for July 2006. The tropical differences suggest
possible cloud Pathfinder contamination in the Intertropical Convergence
Zone. However, there are also high latitude differences where in situ data
are sparse. To correct these differences smoothed zonal in situ minus
satellite differences, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, were computed directly from the data. These
differences were subtracted from the satellite data before the EOT
procedures and then added back onto the biases. This zonal correction has no
net impact on the bias correction unless there are no EOT modes. In that
case,  <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The lower panel shows the difference between the
two daily OI versions with the zonal correction. Here the zonal correction
reduces the difference between 60 and 40<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S. It has
little impact outside of the region even at high northern latitudes.
Although there are differences at high latitudes which are not corrected by
the EOT method, the biases are not zonal between 70 and
80<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N so <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is small there.</p>
</sec>
<sec id="App1.Ch1.S1.SS2.SSS4">
  <title>Temporal smoothing of satellite bias corrections</title>
      <p>The biases, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, use 7 days of in situ and satellite data. These biases tend
to be temporally noisy because the in situ data are sparse. In particular,
jumps in the biases can occur as time changes and data either appear or
disappear from the 7-day window.</p>
      <p>A binomial filter using 3, 5, and 7 days was then used on the mode weights of
the original 7-day bias corrections. To examine the impact, spectra were
computed over a 6-year period. The spectral results were very similar for
both day and night. The globally averaged nighttime bias spectrum is shown
in Fig. A4 for each binomial filter along with the original unsmoothed
spectrum. All spectra show some ringing which is roughly at frequency
multiples of roughly one-seventh cycles per day and due to the use of 7 days of
data.</p>
      <p>All the binomial filters reduce the variance at higher frequencies. It is
not clear which version of the binomial filter would be best. However, the
5-day binomial filter seemed to be a reasonable compromise and was selected.</p>
</sec>
<sec id="App1.Ch1.S1.SS2.SSS5">
  <title>Increased number of days and data used in the bias correction</title>
      <p>Comments from John Stark, UK Met Office, and preliminary processing of
NOAA-7 data indicated that the daily OI Niño-3 time series were noisy
with periods of about a week due to the EOT bias correction. The time series
was especially noisy in the earlier half of the record before 1990 when buoy
data were sparse. Additional filtering of the weights (medians, nine-point box
car, etc.) did not give much improvement. Thus, the EOT data period was
increased from 7 to 15 days. Figure A5 shows that the Niño-3 anomalies
using 7 and 15 days. In particular note the 7-day anomaly sign change
centered near 15 January 1982. It is clear that this type of variability is
reduced using 15 days.</p>
</sec>
<sec id="App1.Ch1.S1.SS2.SSS6">
  <title>Improved AMSR quality control</title>
      <p>Figure 12 from Reynolds et al. (2007) shows that the daily OI interpolates
the analysis across the region of missing AMSR data near 130<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W
and 35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. This region was missing AMSR data due to precipitation
contamination which results in extreme values on the edges of this region.
Chelle Gentemann (personal communication, 2007) used improved quality
control to flag AMSR data with questionable SST obs. The results for 9
February 2003 are shown in Fig. A6. The questionable SSTs (in black) are
only a small part of the total observations. The AMSR extra quality control
reduces the strong noise shown in Fig. 12 from Reynolds et al. (2007).</p>
</sec>
<sec id="App1.Ch1.S1.SS2.SSS7">
  <title>Improved AMSR quality control</title>
      <p>There were some errors in the quarter-degree land/sea mask. The major change
was to eliminate some inland fiords by setting these points to land. These
points occurred at the edge of the Arctic in Russia and Greenland, in the
Inside Passage area of Alaska south of Juneau, and in the Strait of
Magellan. In these regions winter sea ice was often the only data available
to the analysis and often lead to large anomalies in summer. In addition,
one badly represented small island in the Red Sea and one spurious island
off Antarctica near 75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and 0.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W were eliminated and
set to ocean.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
<sec id="App1.Ch1.S1.SS3">
  <title>Final comments</title>
      <p>The use of 3 days of data in the OI and smoothing of the modes in the bias
correction is not possible in near real time. Thus, two versions will be
run: a real-time interim version followed by a final version after a 2-week
delay. The interim version uses 1 day of in situ and satellite data in the
OI with a satellite bias correction using 7 days (one sided) of data and
without smoothing of the EOT modes. The final version uses 3 days (centered)
of in situ and satellite data in the OI with a satellite bias correction
using 15 days (centered) of data and smoothing of the EOT modes over 5 days
(centered). Both versions have a ship bias correction, a preliminary zonal
correction of satellite data, and improved quality control of the AMSR data.
The interim version is replaced by the final version when the final version
is computed. The daily OI using AVHRR only is available from September 1981
to present; the daily OI with AMSR <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> AVHRR is available from June 2002 to
present. Table A2 indicates the differences among version 1 and the interim
and final version 2.</p><?xmltex \hack{\clearpage}?>
</sec>
</app>
  </app-group><notes notes-type="authorcontribution">

      <p>All authors contributed to the text. V. Banzon wrote the draft, with
significant text added by T. Smith. M. T. Chin performed the spectral
analysis for Fig. 4 and provided accompanying text. Processing details were
provided by C. Liu and B. Hankins, who ran the operational production.</p>
  </notes><ack><title>Acknowledgements</title><p>The authors would like to thank R. W. Reynolds (retired), H.-M. Zhang, and
G. Peng for providing comments that greatly improved this paper. R. W. Reynolds
also authored the material presented in Appendix A and gave
permission to include it in this article. Members of the OISST Integrated
Products team, including C. Hutchins, P. Jones, R. McFadden, V. Toner, and D. Wunder,
helped meet CDR program requirements for transition and maintenance
of dOISST.v2.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: G. M. R. Manzella</p></ack><ref-list>
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    <!--<article-title-html>A long-term record of blended satellite and in situ sea-surface temperature for climate monitoring, modeling and environmental studies</article-title-html>
<abstract-html><p class="p">This paper describes a blended sea-surface temperature
(SST) data set that is part of the National Oceanic and Atmospheric
Administration (NOAA) Climate Data Record (CDR) program product suite. Using
optimum interpolation (OI), in situ and satellite observations are combined
on a daily and 0.25° spatial grid to form an SST analysis, i.e., a
spatially complete field. A large-scale bias adjustment of the input
infrared SSTs is made using buoy and ship observations as a reference. This
is particularly important for the time periods when volcanic aerosols from
the El Chichón and Mt. Pinatubo eruptions are widespread globally. The main
source of SSTs is the Advanced Very High Resolution Radiometer (AVHRR),
available from late 1981 to the present, which is also the temporal span of
this CDR. The input and processing choices made to ensure a consistent
data set that meets the CDR requirements are summarized. A brief history and
an explanation of the forward production schedule for the preliminary and
science-quality final product are also provided. The data set is produced and
archived at the newly formed National Centers for Environmental Information
(NCEI) in Network Common Data Form (netCDF) at <a href="http://dx.doi.org/10.7289/V5SQ8XB5" target="_blank">doi:10.7289/V5SQ8XB5</a>.</p></abstract-html>
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Vázquez-Cuervo, J., Armstrong, E., and Harris, A.: The effect of aerosols
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Vázquez-Cuervo, J., Armstrong, E. M., Casey, K. S., Evans, R., and
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The impact of going to higher resolution, Remote Sens. Environ.,
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</mixed-citation></ref-html>--></article>
