EMODnet Physics ERDDAP Installation EMODnet Physics ERDDAP
Easier access to scientific data
log in    
Brought to you by EMODnet Physics    

ERDDAP > info > SPI_10_5281_zenodo_3843375

Grid
DAP
Data
Sub-
set
Table
DAP
Data
Make
A
Graph
W
M
S
Source
Data
Files
Acces-
sible
?
Title Sum-
mary
FGDC,
ISO,
Metadata
Back-
ground
Info
RSS E
mail
Institution Dataset ID
     data   graph     public 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).
   ?            M   background (external link) RSS Subscribe SPI SPI_10_5281_zenodo_3843375

The Dataset's Variables and Attributes

Row Type Variable Name Attribute Name Data Type Value
attribute NC_GLOBAL cdm_data_type String Other
attribute NC_GLOBAL citation String 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
attribute NC_GLOBAL contributors String [{'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'}]
attribute NC_GLOBAL Conventions String COARDS, CF-1.6, ACDD-1.3
attribute NC_GLOBAL creator_name String Nuria Benavent
attribute NC_GLOBAL creator_type String institution
attribute NC_GLOBAL creator_url String https://orcid.org/0000-0003-3473-0629 (external link)
attribute NC_GLOBAL DOI String https://doi.org/10.5281/zenodo.3843376 (external link)
attribute NC_GLOBAL infoUrl String https://doi.org/10.5281/zenodo.3843376 (external link)
attribute NC_GLOBAL institution String SPI
attribute NC_GLOBAL keywords String ACE, Antarctic Circumnavigation Expedition, Antarctica, atmosphere, halogens, IO, iodine monoxide, MAX-DOAS
attribute NC_GLOBAL license String CC-BY-4.0
attribute NC_GLOBAL platform_code String UBXH3_ACE_3843375
attribute NC_GLOBAL platform_name String R/V Akademik Tryoshnikov
attribute NC_GLOBAL sourceUrl String (local files)
attribute NC_GLOBAL standard_name_vocabulary String CF Standard Name Table v55
attribute NC_GLOBAL summary String 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.
attribute NC_GLOBAL title String 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).
attribute NC_GLOBAL type String ferrybox/ship
variable datetime   double  
attribute datetime _ChunkSizes int 512
attribute datetime _CoordinateAxisType String Time
attribute datetime actual_range double 1.4861484E9, 1.4916708E9
attribute datetime axis String T
attribute datetime description String time
attribute datetime ioos_category String Time
attribute datetime long_name String Time
attribute datetime standard_name String time
attribute datetime time_origin String 01-JAN-1970 00:00:00
attribute datetime units String seconds since 1970-01-01T00:00:00Z
variable io_mixing_ratio   double  
attribute io_mixing_ratio _ChunkSizes int 512
attribute io_mixing_ratio actual_range double 0.156, 5.558
attribute io_mixing_ratio description String 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]
attribute io_mixing_ratio spi_original_name String io_mixing_ratio (pptv)
attribute io_mixing_ratio units String parts per trillion
variable io_mixing_ratio_unc   double  
attribute io_mixing_ratio_unc _ChunkSizes int 512
attribute io_mixing_ratio_unc actual_range double 0.029, 1.347
attribute io_mixing_ratio_unc description String Uncertainty in the iodine monoxide (IO) mixing ratio [parts per trillion]
attribute io_mixing_ratio_unc spi_original_name String io_mixing_ratio_unc (pptv)
attribute io_mixing_ratio_unc units String parts per trillion
variable io_vcd   double  
attribute io_vcd _ChunkSizes int 512
attribute io_vcd actual_range double 1.73E11, 2.23E13
attribute io_vcd description String Vertical column density of iodine monoxide (IO) representing the vertical integration of the trace gas concentration profile [molecules per cm^2]
attribute io_vcd spi_original_name String io_vcd (molec/cm^2)
variable io_vcd_unc   double  
attribute io_vcd_unc _ChunkSizes int 512
attribute io_vcd_unc actual_range double 2.78E11, 3.16E12
attribute io_vcd_unc description String Uncertainty in the vertical column density of iodine monoxide (IO) [molecules per cm^2]
attribute io_vcd_unc spi_original_name String io_vcd_unc (molec/cm^2)

The information in the table above is also available in other file formats (.csv, .htmlTable, .itx, .json, .jsonlCSV1, .jsonlCSV, .jsonlKVP, .mat, .nc, .nccsv, .tsv, .xhtml) via a RESTful web service.


 
ERDDAP, Version 2.02
Disclaimers | Privacy Policy | Contact