Data
MEDOC provides different types of data to the solar and heliospheric physics community: observation data from space missions, data products derived from observational data, and results from numerical simulations. The corresponding data sets are listed below, with links to data access.
Observation data
Data access is mainly provided through a unifed web interface (web app and API), which includes the following data sets:
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SOHO (1996-)
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| CDS | UV spectra | LASCO | White-light corona images |
| CELIAS | Particle fluxes | MDI | Disk Dopplergrams and magnetograms |
| COSTEP | Particle fluxes | SUMER | UV spectra |
| EIT | EUV disk images | SWAN | UV images of the heliosphere |
| ERNE | Particle fluxes | UVCS | Coronal UV spectra |
| GOLF | Time series of integrrated disk velocities | VIRGO | Disk-integrated photometry |
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TRACE (1998-2010)
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| TRACE | EUV and white-light disk images | ||
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CORONAS-F (2001-2005)
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| Spirit | EUV disk and corona images, XUV spectra | ||
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STEREO (2006-)
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| SECCHI/EUVI | EUV disk images | SECCHI/HI | White-light heliospheric images |
| SECCHI/COR | White-light corona images | ||
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SDO (2010-)
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| AIA | UV and EUV disk images | HMI | Visible disk images, Dopplergrams, and magnetograms |
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PICARD (2010-2014)
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| SODISM | Visible disk and limb images | SOVAP/BOS | Total irradiance |
| PREMOS | Total and spectral irradiance | PICARD-SOL/SODISM2 | Visible disk and limb images |
Furthermore, the following data sets are available through specific interfaces:
- PICARD (including mission timeline and documents)
- SOHO/LASCO/C2 legacy archive (including calibrated and derived data, CME catalogues, 3D electron density from coronal tomography).
Data derived from observational data
The unified web interface includes the following data, which are computed from observational data:
- SOHO/EIT synchronous synoptic maps.
- SDO/AIA Differential Emission Measure (DEM) maps. The maps are also provided through a Virtual Observatory interface.
Furthermore, MEDOC provides:
- An instance of the HELIO Heliophysics Events Catalogue (with active regions, filaments, filaments/prominences, sunspots, type III events).
- The H2020 FLARECAST processed data for machine learning of flares (API for active region properties, for predictions).
- ICME catalogues.
- A prominence and quiet Sun spectral atlas.
Simulation results data
The following pages provide data from numerical simulations results:
- 1D solar wind hydrodynamical code (from the VP code)
- 3D MHD simulation of an eruption (from the OHM code)
- Cosmic rays in MHD simulations of the solar wind (from the PLUTO code)
Contact: medoc-contact /at/ ias.u-psud.fr
