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ESA SSA SWE Service Page Mockup: NSO/air

Non-Space Systems Operations – Service to airlines


Real-time foF2 index activity map
over Europe


Effective dose rate map due to
current cosmic radiation

A range of space weather phenomena can affect both aircrew and aviation technical infrastructure. The health of aircrew can be affected due to elevated radiation exposure mainly caused by Galactic Cosmic Rays (GCR) and by occasional solar eruptions of energetic charged particles (Solar Energetic Particles - SEP). Technical infrastructure can suffer from degradation or loss of communication and navigation signals, as well as avionics errors. Such disruptions can be caused by both electromagnetic and charged particle radiation, as well as changes in the ionospheric conditions.

The service "Non-Space Systems Operations – Service to airlines" aims at provision of access to global information, data, models and tools addressing these issues to help pilots and airline dispatchers in flight planning, especially for flights affected by space weather effects.

This service is implemented through a combination of products, tools and alerts which can be found through the following tabs along with expert support provided by the teams constituting the SWE 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.

A number of tools and products are available through this service, such as:

  • the Aviation Dosimetry (AVIDOS) tools providing a real-time assessment of cosmic radiation exposure at flight altitudes;
  • the Athens Neutron Monitoring Station (ANEMOS) providing tools like a real time GLE alerting system and access to multi-station neutron monitor data;
  • the RadSEP product providing an SEP post-event analysis for aviation radiation exposure;
  • the Ionosphere Monitoring and Prediction Center (IMPC) providing TEC maps and local scintillation indices;
  • the Real-Time Ionosphere Monitor (RTIM) providing VTEC, GIVE, S4 and σφ maps;
  • the European Ionosonde Service (EIS) providing TEC and foF2 maps, and ionospheric conditions at several locations;
  • the Ionosphere Monitoring Facility (IONMON) providing TEC maps;
  • the Space Weather Data Browsing and Analysis (SWE Data) provides access to space weather environment data.

This service page is curated by the ESC Space Radiation. For further information, please contact SSCC Help-desk.

The radiation environment at aviation altitudes is shaped mainly by Galactic Cosmic Radiation (GCR) that comes from outside of our solar system, is modulated by solar wind, and interacts with Earth's magnetosphere and atmosphere. As an effect, radiation exposure at aviation altitudes is slightly higher than that at ground level. Additionally, some solar events may lead to additional enhancements of radiation exposure not only in atmosphere but also even on the ground – so-called Ground Level Enhancements (GLEs). The elevated radiation at flight altitudes during a GLE, although temporal, can be notable especially for high latitude flights.

The user who is interested in the increased radiation levels during flights can use the Aviation Dosimetry (AVIDOS) tools, accessible from the Tools tab. AVIDOS is an informational and educational online software for the assessment of cosmic radiation exposure at flight altitudes during quiet and extraordinary solar conditions. It estimates route doses for flights between any two locations and calculates now-cast exposure during solar storms. It also provides a comparison of assessed exposure with natural background radiation on Earth. AVIDOS has four modes: "public", "aircrew", "waypoint" and "science". Public mode is designed for a user that demands quick assessment of cosmic radiation exposure for a selected flight without considering all technicalities. For calculations in public mode one needs to enter only date and time of the flight, departure and destination. In aircrew mode, the user can easily appreciate influence of flight route, altitude, duration and even flight date on the assessed radiation exposure by having the possibility to change all those parameters. Waypoints mode allows for dose assessment of a waypoint-by-waypoint designed flight including a complete set of parameters for each waypoint. Waypoints can be uploaded as batch file including: flight and waypoint identifications, altitude, date and time, and geographical latitude and longitude. Results can be downloaded for personal use. With science mode, researchers and experts can analyse dose dependency for different solar proton spectra or investigate different flight routes for the same extraordinary solar condition. Science mode offers: several implemented solar proton spectra, several implemented representative flights, all aspects of the spectra and flights are editable, results are displayed in terms of effective dose, and ambient dose equivalent and can be downloaded for personal use.

To protect aircrews' health, European legislation and various aviation authorities impose requirements concerning assessment and limitation of radiation exposure, as well as provision of information on cosmic radiation (see Auxiliary Info).

Space weather also affects airborne technical infrastructure especially for high latitude flights. Solar phenomena emit electromagnetic radiation and energetic particles that can ionise lower layers of the ionosphere (so-called Polar Cap Absorption - PCA). Disturbed ionospheric conditions influence very high frequency (VHF) signals of Global Navigation Satellite System (GNSS) often used for aircraft navigation and high frequency (HF) radio communication. Due to effects like attenuation, phase shifts, unexpected reflections, interferences and scintillations it may come to a disruption and even loss of navigation and communication signals (Radio Blackouts). Furthermore, aviation electronics and systems are exposed to atmospheric neutrons and protons created by cosmic rays interacting with atmospheric nuclei. This may lead to so-called Single Event Effects (SEE), mostly to a Single Event Upset (SEU) – non-destructive, soft error in electronics.

Information on the current and forecasted ionospheric conditions is provided through several monitoring centres and facilities, like the Ionosphere Monitoring and Prediction Center (IMPC), the Real-Time Ionosphere Monitor (RTIM), the European Ionosonde Service (EIS), the Ionosphere Monitoring Facility (IONMON) and the Service Supporting Resource Exploitation System Operators (RESOSS). The specific products provided can be accessed through in the Ionospheric, Thermospheric and Atmospheric Conditions section under the Products tab.

For further information, please contact SSCC Help-desk

Solar Activity

Solar X-ray Flux
  • Proba2/LYRA Rescaled latest data
  • GOES/SEM X-Ray Sensor datasets on SEDAT
     SEDAT

Interplanetary Medium at L1

High Energy >10 MeV Protons
  • Automated Multi Dataset Analysis (AMDA)
     AMDA
1-10 MeV Protons
  • Automated Multi Dataset Analysis (AMDA)
     AMDA
  • Raw ACE/SEPICA data in SEPEM

Ionospheric, Thermospheric and Atmospheric Conditions: (Near) Realtime Measurements and Data Archives

Atmospheric neutrons
  • Multi-station neutron monitor data
     ANeMoS

Ionospheric, Thermospheric and Atmospheric Conditions: Nowcasts

Vertical Total Electron Content Map
  • TEC map (Europe), current
     IMPC
  • TEC map (Global), current
     IMPC
  • VTEC maps (northern Europe)
     RTIM
  • IONMON TEC maps
     IONMON
  • Near real-time TEC maps for the European region
     EIS
  • TEC and Err(TEC) nowcast modelized maps
     ISM
  • TEC and Err(TEC) nowcast modelized values at a given location
     ISM
3D Electron Density Grids
    URSI Ionospheric Parameters
    • Nowcast European maps of foF2
       EIS
    Riometer Data
      Scintillation Indices and Parameters
      • Local scintillation indices S4 & σφ Kiruna
         IMPC
      • Local scintillation indices S4 & σφ Neustrelitz
         IMPC
      • Local scintillation indices S4 & σφ Svalbard
         IMPC
      • Local scintillation indices S4 & σφ Tenerife
         IMPC
      • Local scintillation indices S4 & σφ Toulouse
         IMPC
      • S4 maps (northern Europe)
         RTIM
      • σφ maps (northern Europe)
         RTIM
      • S4 and Err(S4) nowcast modelized maps
         ISM
      • SigmaPhi and Err(SigmaPhi) nowcast modelized maps
         ISM
      • S4 and Err(S4) nowcast modelized values at a given location
         ISM
      • SigmaPhi and Err(SigmaPhi) nowcast modelized values at a given location
         ISM
      • S4 observed map as quality data for ISM S4 nowcast modelized maps
      • SigmaPhi observed map as quality data for ISM SigmaPhi nowcast modelized maps

      Ionospheric, Thermospheric and Atmospheric Conditions: Forecasts

      Vertical Total Electron Content Map
      • TEC map (Europe), 1hr forecast
         IMPC
      • TEC map (Global), 1hr forecast
         IMPC
      • TEC and Err(TEC) 6-hour forecast modelized maps
         ISM
      • TEC and Err(TEC) 6h forecast modelized values at a given location
         ISM
      3D Electron Density Grids
        URSI Ionospheric Parameters
        • European maps of foF2 long term predictions
           EIS
        • Maps of forecasted foF2 over Europe for the next 24 hours
           EIS
        • Forecasted foF2 values for the next 24 hours over each ionosonde.
           EIS
        Riometer Data
          Scintillation Indices and Parameters
          • S4 and Err(S4) 6-hour forecast modelized maps
             ISM
          • SigmaPhi and Err(SigmaPhi) 6-hour forecast modelized maps
             ISM
          • S4 and Err(S4) 6h forecast modelized values at a given location
             ISM
          • SigmaPhi and Err(SigmaPhi) 6h forecast modelized values at a given location
             ISM

          Aircraft Effects and Radiation Exposure: Data Archives

          Dose at Aircraft Altitudes

          AVIDOS 2.0 is an online, informational and educational software for the assessment of cosmic radiation exposure at flight altitudes. AVIDOS 2.0 performs assessment of cosmic radiation due to galactic cosmic radiation and attempts to nowcast radiation exposure due to solar energetic particles. AVIDOS 2.0 uses real-time data from Oulu neutron monitor station and real-time alerts from GLE-alerting service ANeMoS.

          The Athens Neutron Monitor Station (ANeMoS) provides access to the following tools. GLE ALert plus provides alerts for ground level enhancement (GLE) events and produces every minute a General GLE Alert Graph and station alert graphs for all the stations participating in the network; The multi-station Neutron Monitor data provides continuous measurements of galactic cosmic rays from neutron monitors located around the world.

          SWE Data is a web application that provides access to a wide range of Space Weather related data sources covering the areas of the spacecraft, ionospheric, and ground effects. SWE Data allows the user to access all data contained in the repository providing analysis and visualisation tools from these disparate sources.

          Ground Level Enhancement Detection

          GLE alert+

           ANeMoS

          This section provides links to web pages or resources that are not part of the SSA Space Weather Network or esa.int domain. These sites are not under ESA control, and therefore ESA is not responsible for any of the information or links that you may find there.

          Reference documents