4 datasets found
  1. SPICE, Spectral Imaging of the Coronal Environment

    • esdcdoi.esac.esa.int
    Updated Jun 30, 2020
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    Frédéric Auchère (2020). SPICE, Spectral Imaging of the Coronal Environment [Dataset]. http://doi.org/10.5270/esa-lbmdy7c
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    Dataset updated
    Jun 30, 2020
    Dataset provided by
    European Space Agencyhttp://www.esa.int/
    Authors
    Frédéric Auchère
    Time period covered
    Apr 1, 2020 - Present
    Description

    The SPICE instrument is a high-resolution slit-scanning imaging spectrometer operating at extreme ultraviolet wavelengths from 70.4 nm to 79.0 nm and 97.3 nm to 104.9 nm. It is a facility instrument on the Solar Orbiter mission, funded by ESA member states and ESA. SPICE provides diagnostics of the temperature, density and chemical composition of the solar plasma from the chromosphere to the corona. The spatial resolution of about 6 arcseconds and the spectral resolution is of the order of 0.07 nm. SPICE can raster a maximum field of view of 14x16 arcminutes. Three 11' long narrow slits (2”, 4", 6"), plus a long 14'x30’’ wide slit are available. SPICE produces three types of data: full spectra (full detector images), sit and stare observations (fixed slit), and scanned observations (the slit scanning the field of view). In scanned observations, up to 8 windows of 32 spectral pixels wide can be included. All Solar Orbiter SPICE data are available from the public Solar Orbiter data archive at http://soar.esac.esa.int/

  2. MEX-E-M-SPICE-6

    • esdcdoi.esac.esa.int
    Updated Feb 1, 2024
    + more versions
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    European Space Agency (2024). MEX-E-M-SPICE-6 [Dataset]. http://doi.org/10.57780/esa-dvhwrm0
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    Dataset updated
    Feb 1, 2024
    Dataset provided by
    European Space Agencyhttp://www.esa.int/
    Time period covered
    Jun 2, 2003 - Dec 31, 2023
    Description
    1. SPICE System Overview SPICE data contain geometric and other ancillary information needed to recover the full value of science instrument data. In particular, SPICE kernels provide spacecraft and planetary ephemerides, instrument mounting alignments and spacecraft orientation. Data needed for r^ant time conversions is also included. SPICE was designed by the Navigation and Ancillary Information Facility (NAIF) to aid scientists and engineers with ancillary and engineering data. This data comes from a wide range of sources such as the spacecraft, the mission control center and the designers of the spacecraft and its instruments. The ancillary data comprises information on data acquisition; position and orientation of the spacecraft at the time of acquisition; information on the target, such as location, shape and orientation; reference frame specifications and time conversion data. The primary SPICE data sets are often called 'kernels' or 'kernel files'. These kernels are composed of ancillary information, which has been created in such a way as to allow easy access and correct usage by the space science and engineering communities. In addition to the kernels, there is software provided, known as the SPICE Toolkit, along with standards, documentation and software support. The SPICE Toolkit and documentation can be found at: https://naif.jpl.nasa.gov/naif/ The SPICE Toolkit was freely offered to the worldwide space science and space mission engineering communities at the time this data set was released. The few rules governing its use are posted on the ''Rules'' page of the NAIF website: https://naif.jpl.nasa.gov/naif/rules.html SPICE is used on a number of space missions, such as ESA's Mars Express, SMART1, Venus Express, ExoMars2016, BepiColombo, Solar Orbiter and Rosetta missions, and all of NASA's solar system exploration missions. The SPICE system has been produced and is maintained by Ca [truncated!, Please s [truncated!, Please see actual data for full text]
  3. h

    3DView Website

    • hpde.io
    Updated Jul 11, 2014
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    (2014). 3DView Website [Dataset]. https://hpde.io/SMWG/Service/CDPP/3DView.html
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    Dataset updated
    Jul 11, 2014
    License

    https://cdla.io/permissive-1-0/https://cdla.io/permissive-1-0/

    Description

    3DView is a science tool that offers immediate 3D visualization of spacecraft position and attitude, planetary ephemerides, as well as scientific data representation (observations and models). A large number of mission trajectories are included (via Spice Kernels) : Cluster, Themis, Solar Orbiter, Juice, Juno, Maven, Mars Express, Venus Express, ... 3DView can access observational database (AMDA, CDAWeb, CLweb, ...) as well as simulation and model databases (from FMI, LATMOS, SINP, ...)

  4. RO-RL-E-M-A-C-SPICE-6

    • esdcdoi.esac.esa.int
    Updated Jan 10, 2017
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    European Space Agency (2017). RO-RL-E-M-A-C-SPICE-6 [Dataset]. http://doi.org/10.57780/esa-3dwqlgp
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    Dataset updated
    Jan 10, 2017
    Dataset provided by
    European Space Agencyhttp://www.esa.int/
    Time period covered
    Mar 2, 2004 - Jan 1, 2017
    Description
    1. SPICE System Overview SPICE data contain geometric and other ancillary information needed to recover the full value of science instrument data. In particular, SPICE kernels provide spacecraft and planetary ephemerides, instrument mounting alignments and spacecraft orientation. Data needed for r^ant time conversions is also included. SPICE was designed by the Navigation and Ancillary Information Facility (NAIF) to aid scientists and engineers with ancillary and engineering data. This data comes from a wide range of sources such as the spacecraft, the mission control center and the designers of the spacecraft and its instruments. The ancillary data comprises information on data acquisition; position and orientation of the spacecraft at the time of acquisition; information on the target, such as location, shape and orientation; reference frame specifications and time conversion data. The primary SPICE data sets are often called 'kernels' or 'kernel files'. These kernels are composed of ancillary information, which has been created in such a way as to allow easy access and correct usage by the space science and engineering communities. In addition to the kernels, there is software provided, known as the SPICE Toolkit, along with standards, documentation and software support. The SPICE Toolkit and documentation can be found at: http://naif.jpl.nasa.gov/naif/ The SPICE Toolkit was freely offered to the worldwide space science and space mission engineering communities at the time this data set was released. The few rules governing its use are posted on the ''Rules'' page of the NAIF website: https://naif.jpl.nasa.gov/naif/rules.html SPICE is used on a number of space missions, such as ESA's Mars Express, SMART1, Venus Express, ExoMars2016, BepiColombo, Solar Orbiter and Rosetta missions, and all of NASA's solar system exploration missions. The SPICE system has been produced and is maintained by Cal [truncated!, Please s [truncated!, Please see actual data for full text]
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Frédéric Auchère (2020). SPICE, Spectral Imaging of the Coronal Environment [Dataset]. http://doi.org/10.5270/esa-lbmdy7c
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SPICE, Spectral Imaging of the Coronal Environment

Experiment onboard the ESA/NASA Solar Orbiter mission

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31 scholarly articles cite this dataset (View in Google Scholar)
Dataset updated
Jun 30, 2020
Dataset provided by
European Space Agencyhttp://www.esa.int/
Authors
Frédéric Auchère
Time period covered
Apr 1, 2020 - Present
Description

The SPICE instrument is a high-resolution slit-scanning imaging spectrometer operating at extreme ultraviolet wavelengths from 70.4 nm to 79.0 nm and 97.3 nm to 104.9 nm. It is a facility instrument on the Solar Orbiter mission, funded by ESA member states and ESA. SPICE provides diagnostics of the temperature, density and chemical composition of the solar plasma from the chromosphere to the corona. The spatial resolution of about 6 arcseconds and the spectral resolution is of the order of 0.07 nm. SPICE can raster a maximum field of view of 14x16 arcminutes. Three 11' long narrow slits (2”, 4", 6"), plus a long 14'x30’’ wide slit are available. SPICE produces three types of data: full spectra (full detector images), sit and stare observations (fixed slit), and scanned observations (the slit scanning the field of view). In scanned observations, up to 8 windows of 32 spectral pixels wide can be included. All Solar Orbiter SPICE data are available from the public Solar Orbiter data archive at http://soar.esac.esa.int/

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