Proton Event products are issued for several thresholds and for two particle energy levels. The ≥10 MeV products match the NOAA Solar Radiation Storm (S-scale) thresholds (10, 100, 1000, 10000, 100000 pfu), based upon values observed or expected on the primary GOES satellite. The ≥100 MeV products are based on a single flux threshold of 1 proton flux unit (pfu).
Proton Event WARNINGS are forecasts of a proton event and are issued by SWPC under two conditions: warning of the expected ONSET of a Proton Event, and warning of the expected PERSISTENCE of a Proton Event that is already in progress. The ≥10 MeV Integral Flux WARNING is issued based upon the expectation of reaching or exceeding flux levels of 10 pfu. The ≥100 MeV Integral Flux WARNING is issued based on the expectation of reaching or exceeding flux levels of 1 pfu. Proton Event WARNINGS include a specific indication of what condition - Onset or Persistence - applies to the WARNING. The WARNING period is expressed in terms of “Valid From” and “Valid To” times. If needed, the warning period may be extended by means of an EXTENDED WARNING. EXTENDED WARNINGS always have the same “Valid From” time as the original WARNING, with a revised “Now Valid Until” time specified in the message. The ≥10 MeV Integral Flux WARNING includes the predicted level of activity based on the NOAA S-scale.
Proton Event ALERTS are issued upon confirmation of ≥10 Mev or ≥100 MeV Integral Flux exceeding certain thresholds. Initial ALERTS for ≥10 MeV and ≥100 MeV energies are issued for integral flux reaching or exceeding 10 pfu and 1 pfu, respectively. Higher threshold ≥10 MeV ALERTS are also issued for threshold exceedance of 100, 1,000, 10,000, and 100,000 pfu, matching the thresholds described in the NOAA S-scale. Once the Proton Flux has dropped below a given threshold, a Proton Event SUMMARY is issued, specifying the start, maximum, end times, and maximum flux observed for the event, along with the corresponding NOAA S-scale. Because flux levels can drop slowly, the time of a "confirmed" drop below threshold can sometimes take several hours to determine.
Higher threshold products for ≥100 MeV flux levels, such as 100 pfu, are being considered for future implementation. Solar Proton Events at Earth can occur throughout the solar cycle but are most frequent in solar maximum years. SPEs result from fast coronal mass ejections. During an SPE, satellites experience dramatically increased bombardment by high-energy particles. Fluxes of particles with energies ≥ 10 MeV can reach 43,500 protons/cm2/sec/ster. Single Event Upset rates in spacecraft electronics increase with high fluxes since there is a higher likelihood of impact on a sensitive location. In addition, these high energy particles can access the polar ionosphere and create an enhanced region of ionization (called the ‘D-Region’) which interferes with HF radio communication in these areas.
High-energy particles can reach Earth anywhere from 20 minutes to many hours following the initiating solar event. The particle energy spectrum and arrival time seen by satellites varies with the location and nature of the event on the solar disk.
SWPC has high-energy proton detectors on the GOES geostationary and NOAA polar-orbiting satellites. GOES 5-minute averaged integral proton flux (protons/cm2-s-sr), as measured by the SWPC primary GOES satellite for energy thresholds of >=10, >=50, >=100, and >=500 MeV, are provided. SWPC's proton event threshold is 10 protons/cm2-s-sr at >=10 MeV.
Solar proton event observations and predictions have been made from the early 1960's to the present time; the National Centers for Environmental Information and SWPC have daily forecast reports going back to 1966, and data back to 1996.
The dynamic plot above can be downloaded in multiple image formats using the menu at the upper right. The menu also offers the ability to download the displayed numerical data in JSON format.
Numerical data are also available directly from SWPC's data service at:
https://services.swpc.noaa.gov/json/goes/
In that directory the file instrument-sources.json provides the mapping of primary and secondary measurements from each instrument to the satellite from which that measurement is made. The file satellite-longitudes.json provides the longitudes of the satellites. Observation data are found under the primary and secondary subdirectories.
NOTE: After January 31, 2020 other JSON/GOES data files and subdirectories will be removed. This is due to discontinuation of GOES-14 and GOES-15 observations on that date.
Historical 3-day plots and text files from 1996 through January 2020 are available at:
ftp://ftp.swpc.noaa.gov/pub/warehouse/
or by following the archive link under “Data Access." Daily forecast reports are also available beginning in 1966.
The official archive for GOES data, can be found at:
https://www.ngdc.noaa.gov/stp/satellite/goes-r.html
Data prior to GOES-16 can be found at: