Environment Specification: Data Archive
Welcome to the Spacecraft Design - Environment specification: data archive service
Overview
The service "Spacecraft Design - Environment specification: data archive" aims to provide, for past or future spacecraft, statistical information on the space environment (i.e. ionising radiation, plasma, microparticles, atmosphere, and UV) and its effects (e.g. dose, single event upset, sensor background, cumulated charge, spacecraft anomalies, microparticle impacts), as well as long-term solar cycle prediction since several spacecraft effects exhibit solar cycle variation. Such information is needed for tailored design of space systems especially in relation to radiation protection, electromagnetic compatibility and microparticle impacts. The service is intended for personnel involved in generating space environment specifications for the design of spacecraft.
This service is implemented through a combination of products and tools which can be found in the sections below along with expert support provided by the teams constituting the ESA Space Weather Service Network. Should you require further guidance in the use of this service, or have specific questions about any aspects of the service presented here, don’t hesitate to contact the Helpdesk.
Highlights
Announcements
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Products and Alerts
Products
Solar Activity: Data Archives
Solar Flares
- FLARECAST Solar flare forecast
- UGraz/KSO Solar flare detection archive
- UGraz/KSO Halpha light curves archive
- A-EFFort Solar flare forecast archive
- SIDC Solarmap
- SIDC Solar flare forecast archive
- SIDC Solar EUV flare detection archive
- SIDC Moderated Solar Weather Event list archive
- ASUCAS/SPS Solar flare forecast archive
- ASUCAS/SPS Daily space weather bulletin archive
Smoothed Sunspot Number (SSN, R12)
10.7cm Solar Radio Flux (F10.7)
Solar X-ray Flux
- UGraz/KSO Halpha light curves archive
- Proba2/LYRA Rescaled data archive
- GOES/SEM X-Ray Sensor datasets on SEDAT
Solar EUV Integrated Flux
Solar UV Flux
Solar Activity: Models and Reconstruction
Solar Flares
No product available in this category yet
Smoothed Sunspot Number (SSN, R12)
10.7cm Solar Radio Flux (F10.7)
Solar X-ray Flux
No product available in this category yet
Solar EUV Integrated Flux
No product available in this category yet
Solar UV Flux
No product available in this category yet
Solar Activity: Forecasts
Solar Flares
Smoothed Sunspot Number (SSN, R12)
10.7cm Solar Radio Flux (F10.7)
- CLS F10.7 and F30 nowcast & forecast
- UGraz/KSO Latest F10.7 and F30 forecasts
- SIDC Latest 10.7cm Solar radio flux (F10.7) forecast
- F10.7 Index Forecast 27-day/BGS
- F10.7 Index Forecast multi-year
- F10.7 Index Forecast 27-day/SWPC
- F10.7 Index Forecast 45-day
- F10.7 Index Forecast 30-day Absolute
- F10.7 Index Forecast 30-day Adjusted
Solar EUV Integrated Flux
No product available in this category yet
Solar UV Flux
No product available in this category yet
Interplanetary Medium at L1: Data Archives
High Energy >10 MeV Protons
- Automated Multi Dataset Analysis (AMDA)
- Herschel/SREM dataset on SEDAT
- Planck/SREM dataset on SEDAT
- HESPERIA RELeASE
- HESPERIA UMASEP-500
- Herschel/SREM radiation rates
- Planck/SREM radiation rates
- EDRS-C/NGRM L2 Proton differential fluxes
High Energy >10 MeV/nuc Ions
1-10 MeV Protons
1-10 MeV/nuc Ions
0.03-1 MeV/nuc Ions
2-50 MeV Solar Electrons
30 keV-8 MeV Electrons
Interplanetary Magnetic Field (IMF)
Solar Wind Bulk Velocity
- Archive - Solar wind model for Earth [WSA-Enlil]
- Archive - Solar wind model for Earth [ESWF]
- Archive - Solar wind model for Earth [STA+CH]
- Archive - Solar Wind Forecast Speed Comparison [SWFSC/E]
- Archive - Solar wind model for Earth 24 hour optimised [ESWF24]
- Archive - Enhanced 24 hour solar wind forecast [AWR_NXT]
- Automated Multi Dataset Analysis (AMDA)
Solar Wind Bulk Density
Solar Wind Temperature
Interplanetary Medium at L1: Models and Reconstruction
High Energy >10 MeV Protons
- Statistical long-term plasma products - L1 p>10MeV
- Automated Multi Dataset Analysis (AMDA)
- SPENVIS Short-term solar particle models
- SPENVIS Long-term solar particle models
- SPENVIS Galactic cosmic ray models
- Very high-energy solar energetic proton fluence
- Very high-energy solar energetic proton peak flux
- Solar very high-energy particle event catalogue
- Very high-energy solar proton event database
High Energy >10 MeV/nuc Ions
1-10 MeV/nuc Ions
0.03-1 MeV/nuc Ions
2-50 MeV Solar Electrons
30 keV-8 MeV Electrons
Interplanetary Magnetic Field (IMF)
Solar Wind Bulk Velocity
Solar Wind Bulk Density
Solar Wind Temperature
Interplanetary Medium at L1: Forecasts
High Energy >10 MeV Protons
High Energy >10 MeV/nuc Ions
No product available in this category yet
1-10 MeV Protons
No product available in this category yet
1-10 MeV/nuc Ions
No product available in this category yet
0.03-1 MeV/nuc Ions
No product available in this category yet
2-50 MeV Solar Electrons
No product available in this category yet
30 keV-8 MeV Electrons
No product available in this category yet
Interplanetary Magnetic Field (IMF)
Solar Wind Bulk Velocity
- SIDC Latest daily space weather bulletin
- Solar Wind Forecast Speed Comparison
- Near-Earth solar wind forecasts (WSA-Enlil + Ensemble)
- Empirical solar wind speed forecast
- Empirical solar wind speed forecast
- Solar wind speed forecast (STEREO-A persistence model)
- AWARE_NEXT Enhanced 24 hour solar wind forecast
- SWiFT
Solar Wind Bulk Density
Solar Wind Temperature
Magnetospheric Environment: Data Archives
High Energy >10 MeV Protons
- PROBA-V/EPT Proton flux spectra time series
- PROBA-V/EPT High-latitude/polar proton flux survey
- AZUR/EI-88 dataset on SEDAT
- GOES/SEM-EPS datasets on SEDAT
- UARS/PEM-HEPS dataset on SEDAT
- PROBA-1/SREM dataset on SEDAT
- Integral/SREM dataset on SEDAT
- IMP-8/CPME and CRNC datasets on SEDAT
- MIR/REM dataset on SEDAT
- STRV1B/REM dataset on SEDAT
- XMM/ERMD dataset on SEDAT
- SEPEM Reference proton data set
- Raw and cleaned GOES/SEM proton channels in SEPEM
- Raw IMP8/CPME proton channels in SEPEM
- Raw and cleaned IMP8/GME proton channels in SEPEM
- HESPERIA UMASEP-500
- PROBA-1/SREM radiation rates
- Integral/SREM radiation rates
- EDRS-C/NGRM L2 Proton differential fluxes
High Energy >10 MeV/nuc Ions
- PROBA-V/EPT Helium flux spectra time series
- PROBA-V/EPT High-latitude/polar helium flux survey
- AZUR/EI-88 dataset on SEDAT
- GOES/SEM-EPS datasets on SEDAT
- METOP02/SEM2 dataset on SEDAT
- IMP-8/CPME and CRNC datasets on SEDAT
- POES/SEM-2 datasets on SEDAT
- SEPEM Reference helium data set
- Raw and cleaned GOES/SEM helium channels in SEPEM
- Raw IMP8/CPME ion channels in SEPEM
- Raw IMP8/CPME helium channels in SEPEM
- Raw and cleaned IMP8/GME helium channels in SEPEM
1-10 MeV Protons
- Automated Multi Dataset Analysis (AMDA)
- AZUR/EI-88 dataset on SEDAT
- GOES/SEM-EPS datasets on SEDAT
- UARS/PEM-HEPS dataset on SEDAT
- IMP-8/CPME and CRNC datasets on SEDAT
- XMM/ERMD dataset on SEDAT
- SEPEM Reference proton data set
- Raw and cleaned GOES/SEM proton channels in SEPEM
- Raw IMP8/CPME proton channels in SEPEM
- Raw and cleaned IMP8/GME proton channels in SEPEM
- EDRS-C/NGRM L2 Proton differential fluxes
1-10 MeV/nuc Ions
- AZUR/EI-88 dataset on SEDAT
- GOES/SEM-EPS datasets on SEDAT
- IMP-8/CPME and CRNC datasets on SEDAT
- SEPEM Reference helium data set
- Raw and cleaned GOES/SEM helium channels in SEPEM
- Raw IMP8/CPME ion channels in SEPEM
- Raw IMP8/CPME helium channels in SEPEM
- Raw and cleaned IMP8/GME helium channels in SEPEM
0.03-1 MeV/nuc Ions
- Automated Multi Dataset Analysis (AMDA)
- METOP02/SEM2 dataset on SEDAT
- Equator_S/EPI dataset on SEDAT
- ISEE1/MEPI dataset on SEDAT
- POES/SEM-2 datasets on SEDAT
30 keV-8 MeV Electrons
- Automated Multi Dataset Analysis (AMDA)
- GOES-16 Radiation Environment
- GOES-15 Radiation Environment
- GOES-14 Radiation Environment
- GIOVE-A Radiation Environment
- Slot Region Radiation Environment
- MOSWOC Forecast
- Forecaster Summary
- Best Reconstruction of the Radiation Environment (GOES-15)
- Best Reconstruction of the Radiation Environment (GOES-14)
- Best Reconstruction of the Radiation Environment (GIOVE-A)
- Best Reconstruction of the Radiation Environment (slot)
- Best Reconstruction of the Radiation Environment (GOES-16)
- PROBA-V/EPT Electron flux spectra time series
- PROBA-V/EPT High-latitude/polar electron flux survey
- GOES/SEM-EPS datasets on SEDAT
- Meteosat-3/SEM2 dataset on SEDAT
- METOP02/SEM2 dataset on SEDAT
- CRRES/MEA dataset on SEDAT
- Equator_S/EPI dataset on SEDAT
- PROBA-1/SREM dataset on SEDAT
- Integral/SREM dataset on SEDAT
- IMP-8/CPME and CRNC datasets on SEDAT
- ISEE1/MEPI dataset on SEDAT
- ISEE1/KED dataset on SEDAT
- MIR/REM dataset on SEDAT
- STRV1B/REM dataset on SEDAT
- POES/SEM-2 datasets on SEDAT
- XMM/ERMD dataset on SEDAT
- Raw GOES/SEM >2 MeV electron channel in SEPEM
- Raw IMP8/CPME electron channels in SEPEM
- Raw IMP8/GME electron channels in SEPEM
- PROBA-1/SREM radiation rates
- Integral/SREM radiation rates
- EDRS-C/NGRM L2 Electron Fluxes
Thermal and Supra-thermal Electron and Ion Energy Spectra
Thermal Ions Density and Temperature
Magnetospheric Environment: (Near-) Real-time Measurements
Plasma Drift Velocity
No product available in this category yet
Magnetospheric Environment: Models and Reconstruction
High Energy >10 MeV Protons
- PROBA-V/EPT Proton flux geographical maps
- PROBA-V/EPT SAA proton energy spectrum characterisation
- Static radiation model of energetic protons at LEO
- SEPEM Reference event list
- SPENVIS Standard radiation belt models
- SPENVIS IRENE Radiation belt models
- SPENVIS Short-term solar particle models
- SPENVIS Long-term solar particle models
- SPENVIS Galactic cosmic ray models
- Very high-energy solar energetic proton fluence
- Very high-energy solar energetic proton peak flux
- Very high-energy solar proton event database
High Energy >10 MeV/nuc Ions
- PROBA-V/EPT Helium flux geographical maps
- PROBA-V/EPT SAA helium energy spectrum characterisation
- Static radiation model of energetic helium ions at LEO
- SPENVIS Short-term solar particle models
- SPENVIS Long-term solar particle models
- SPENVIS Galactic cosmic ray models
- High-energy solar heavy ion fluence model
- High-energy solar heavy ion peak flux model
1-10 MeV Protons
1-10 MeV/nuc Ions
0.03-1 MeV/nuc Ions
30 keV-8 MeV Electrons
- Automated Multi Dataset Analysis (AMDA)
- PROBA-V/EPT Electron flux geographical maps
- PROBA-V/EPT Auroral electron energy spectrum characterisation
- Static radiation model of energetic electrons at LEO
- SPENVIS Standard radiation belt models
- SPENVIS IRENE Radiation belt models
- SPENVIS Internal deep dielectric charging
- EDRS-C/NGRM Electron daily fluences
Thermal and Supra-thermal Electron and Ion Energy Spectra
Thermal Ions Density and Temperature
Magnetospheric Environment: Forecasts
High Energy >10 MeV Protons
High Energy >10 MeV/nuc Ions
No product available in this category yet
1-10 MeV Protons
No product available in this category yet
1-10 MeV/nuc Ions
No product available in this category yet
0.03-1 MeV/nuc Ions
No product available in this category yet
30 keV-8 MeV Electrons
Thermal and Supra-thermal Electron and Ion Energy Spectra
Thermal Ions Density and Temperature
No product available in this category yet
Thermospheric and Atmospheric Conditions: Data Archives
Atomic Oxygen Density
No product available in this category yet
Neutral Density and Wind
No product available in this category yet
Thermospheric and Atmospheric Conditions: Models and Reconstruction
Atomic Oxygen Density
Neutral Density and Wind
Thermospheric and Atmospheric Conditions: Forecasts
Atomic Oxygen Density
No product available in this category yet
Neutral Density and Wind
Microparticle Environment: Data Archives
Micro Particle Flux
Known Periods/events of Increased Microparticle Flux
No product available in this category yet
Microparticle Environment: Models and Reconstruction
Micro Particle Flux
Known Periods/events of Increased Microparticle Flux
Microparticle Environment: Forecasts
Micro Particle Flux
No product available in this category yet
Spacecraft Effects and Anomalies: Data Archives
Anomalies on Spacecraft Equipment
No product available in this category yet
Spacecraft Radiation Monitors
- Radiation environment outside the ISS
- Radiation environment inside ISS
- Accumulated dose in human phantoms on ISS
- PROBA-1/SREM dataset on SEDAT
- Integral/SREM dataset on SEDAT
- Rosetta/SREM dataset on SEDAT
- Herschel/SREM dataset on SEDAT
- Planck/SREM dataset on SEDAT
- MIR/REM dataset on SEDAT
- STRV1B/REM dataset on SEDAT
- PROBA-1/SREM radiation rates
- Integral/SREM radiation rates
- Rosetta/SREM radiation rates
- Herschel/SREM radiation rates
- Planck/SREM radiation rates
- EDRS-C/NGRM L2 Electron Fluxes
- EDRS-C/NGRM L2 Proton differential fluxes
Dose
- GOES-16 Total Ionising Dose and Dose Rate
- GOES-15 Total Ionising Dose and Dose Rate
- GOES-14 Total Ionising Dose and Dose Rate
- GIOVE-A Total Ionising Dose and Dose Rate
- Slot Region Total Ionising Dose and Dose Rate
- PROBA-V/EPT Total ionizing dose estimation at LEO
- PROBA-V/EPT Total non-ionizing dose estimation at LEO
- Radiation environment outside the ISS
- Radiation environment inside ISS
- Accumulated dose in human phantoms on ISS
Deep Dielectric Charging
Spacecraft Effects and Anomalies: Models and Reconstruction
Anomalies on Spacecraft Equipment
Spacecraft Radiation Monitors
Dose
Deep Dielectric Charging
Long-term Solar Cycle Prediction
Long-term Solar Activity
No product available in this category yet
Activity at L1
No product available in this category yet
Tools
User Manual
The space environments considered include energetic particle radiation, plasmas, atmospheres, micro-particles, and contamination. They can all cause serious problems for space systems that need to be carefully taken into account during the development of spacecraft. The radiation environment, consisting of radiation belts, cosmic rays, and solar energetic particles causes effects such as radiation damage, single-event upsets in electronics, background in detectors, and health hazards to astronauts. The plasma environment increases electrostatic charging of spacecraft parts or affects scientific instruments. The residual upper atmosphere causes surface erosion by atomic oxygen. Finally the micro-meteoroids and space debris environments introduce significant risks for manned and unmanned spacecraft.
MoreInterruptions
None