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Dataset Title:  SPI - Iodine monoxide (IO) measurements made using a MAX-DOAS (Multi-AXis
Differential Optical Absorption Spectroscopy) instrument in the austral summer
of 2016/17 during the Antarctic Circumnavigation Expedition (ACE).
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Institution:  SPI   (Dataset ID: SPI_10_5281_zenodo_3843375)
Information:  Summary ? | License ? | Metadata | Background (external link) | Files | Make a graph
 
Variable ?   Optional
Constraint #1 ?
Optional
Constraint #2 ?
   Minimum ?
 
   Maximum ?
 
 datetime (Time, UTC) ?          2017-02-03T19:00:00Z    2017-04-08T17:00:00Z
 io_mixing_ratio (parts per trillion) ?          0.156    5.558
 io_mixing_ratio_unc (parts per trillion) ?          0.029    1.347
 io_vcd ?          1.73E11    2.23E13
 io_vcd_unc ?          2.78E11    3.16E12
 
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The Dataset Attribute Structure (.das) for this Dataset

Attributes {
 s {
  datetime {
    Int32 _ChunkSizes 512;
    String _CoordinateAxisType "Time";
    Float64 actual_range 1.4861484e+9, 1.4916708e+9;
    String axis "T";
    String description "time";
    String ioos_category "Time";
    String long_name "Time";
    String standard_name "time";
    String time_origin "01-JAN-1970 00:00:00";
    String units "seconds since 1970-01-01T00:00:00Z";
  }
  io_mixing_ratio {
    Int32 _ChunkSizes 512;
    Float64 actual_range 0.156, 5.558;
    String description "Quotient between the number density of iodine monoxide (IO) and the number density of the air or atmosphere at that same height, expressed in units of parts per trillion (1 out every 1e12 air molecules) or pptv [parts per trillion]";
    String spi_original_name "io_mixing_ratio (pptv)";
    String units "parts per trillion";
  }
  io_mixing_ratio_unc {
    Int32 _ChunkSizes 512;
    Float64 actual_range 0.029, 1.347;
    String description "Uncertainty in the iodine monoxide (IO) mixing ratio [parts per trillion]";
    String spi_original_name "io_mixing_ratio_unc (pptv)";
    String units "parts per trillion";
  }
  io_vcd {
    Int32 _ChunkSizes 512;
    Float64 actual_range 1.73e+11, 2.23e+13;
    String description "Vertical column density of iodine monoxide (IO) representing the vertical integration of the trace gas concentration profile [molecules per cm^2]";
    String spi_original_name "io_vcd (molec/cm^2)";
  }
  io_vcd_unc {
    Int32 _ChunkSizes 512;
    Float64 actual_range 2.78e+11, 3.16e+12;
    String description "Uncertainty in the vertical column density of iodine monoxide (IO) [molecules per cm^2]";
    String spi_original_name "io_vcd_unc (molec/cm^2)";
  }
 }
  NC_GLOBAL {
    String _NCProperties "version=2,netcdf=4.7.2,hdf5=1.10.5";
    String cdm_data_type "Other";
    String citation "Benavent, N., Garcia-Nieto, D., Cuevas, C.A. and Saiz-Lopez, A. (2020). Iodine monoxide (IO) measurements made using a MAX-DOAS (Multi-Axis Differential Optical Absorption Spectroscopy) instrument in the austral summer of 2016/17 during the Antarctic Circumnavigation Expedition (ACE). (Version 1.0) [Data set]. Zenodo. https://doi.org/10.5281/zenodo.3843376";
    String contributors "[{'title': 'Nuria Benavent', 'path': 'https://orcid.org/0000-0003-3473-0629', 'role': 'author', 'organisation': 'Department of Atmospheric Chemistry and Climate, Institute of Physical Chemistry Rocasolano, Consejo Superior de Investigaciones Científicas, Spain'}, {'title': 'David Garcia-Nieto', 'path': 'https://orcid.org/0000-0002-0884-5978', 'role': 'author', 'organisation': 'Department of Atmospheric Chemistry and Climate, Institute of Physical Chemistry Rocasolano, Consejo Superior de Investigaciones Científicas, Spain'}, {'title': 'Carlos Alberto Cuevas', 'path': 'https://orcid.org/0000-0002-9251-5460', 'role': 'author', 'organisation': 'Department of Atmospheric Chemistry and Climate, Institute of Physical Chemistry Rocasolano, Consejo Superior de Investigaciones Científicas, Spain'}, {'title': 'Alfonso Saiz-Lopez', 'path': 'https://orcid.org/0000-0002-0060-1581', 'email': 'a.saiz@csic.es', 'role': 'author', 'organisation': 'Department of Atmospheric Chemistry and Climate, Institute of Physical Chemistry Rocasolano, Consejo Superior de Investigaciones Científicas, Spain'}]";
    String Conventions "COARDS, CF-1.6, ACDD-1.3";
    String creator_name "Nuria Benavent";
    String creator_type "institution";
    String creator_url "https://orcid.org/0000-0003-3473-0629";
    String DOI "https://doi.org/10.5281/zenodo.3843376";
    String history 
"2024-04-19T08:45:51Z (local files)
2024-04-19T08:45:51Z https://erddap.emodnet-physics.eu/erddap/tabledap/SPI_10_5281_zenodo_3843375.html";
    String infoUrl "https://doi.org/10.5281/zenodo.3843376";
    String institution "SPI";
    String keywords "ACE, Antarctic Circumnavigation Expedition, Antarctica, atmosphere, halogens, IO, iodine monoxide, MAX-DOAS";
    String license "CC-BY-4.0";
    String platform_code "UBXH3_ACE_3843375";
    String platform_name "R/V Akademik Tryoshnikov";
    String sourceUrl "(local files)";
    String standard_name_vocabulary "CF Standard Name Table v55";
    String summary "To achieve the objectives of the project, we installed a MAX-DOAS (Multi-AXis Differential Optical Absorption Spectroscopy) instrument on the vessel “Akademik Tryoshnikov”. This instrument is based on the DOAS technique, which is used to measure trace gas concentrations in the atmosphere. The method consists of the analysis of the spectral absorption lines that each trace gas produces in the solar spectra. The DOAS technique uses the narrowband features that every trace gas has in their spectral absorption coefficients. This differential cross section is unique and acts like a fingerprint for the trace gases, allowing to differentiate between them and to estimate their concentrations (for further details see Platt and Stutz, 2008). In the past decades, atmospheric chemists have come to realize that halogen species (like Cl, Br or I and their oxides ClO, BrO and IO) exert a powerful influence on the chemical composition of the troposphere and through that influence affect the evolution of pollutants, hence having a significant impact on climate. These reactive halogen species are potent oxidizers for organic and inorganic compounds throughout the troposphere. In particular, halogen cycles can act on several compounds (such as methane, ozone, particles…), all of which are climate forcing agents through direct and indirect radiative effects. Dynamic exchange of halogens between ocean, sea ice, snowpack and atmosphere is the main driver for the frequent occurrence of Ozone Depletion Events (ODEs) and Atmospheric Mercury Depletion Events (AMDEs) (Saiz-Lopez and von Glasow, 2012). In this dataset we present the mixing ratio and vertical column density of iodine monoxide (IO) recorded in the austral summer of 2016/2017 in the Southern Ocean and Atlantic Ocean, averaged over one-hour time periods.";
    String title "SPI - Iodine monoxide (IO) measurements made using a MAX-DOAS (Multi-AXis Differential Optical Absorption Spectroscopy) instrument in the austral summer of 2016/17 during the Antarctic Circumnavigation Expedition (ACE).";
    String type "ferrybox/ship";
  }
}

 

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