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GOES-16, GOES-17 and GOES-18 Data Status: L1b data are available for most instruments. Some L2 data are available.
GOES-R L2 data will be available on a rolling basis as products reach maturity. The L2 time series data are aggregated into daily and longer netCDF files, while the SUVI
files are in FITS format.
Real-time JSON files with partial data products for some GOES-R instruments are available from SWPC.
Consult the ReadMe files below before using the data.
Example codes to use these
data.
GOES-R Level 2 Data: Space Weather Instruments
| Instrument |
Product |
File Access |
Description |
| EUVS |
User Guide
Readme
|
|
| EUVS 1-min Averages |
|
Spectral line irradiances, the Mg II index, and proxy spectra from the EXIS Extreme Ultraviolet Sensor (EUVS) |
| EUVS Daily Averages |
|
Daily averages of spectral line irradiances, the Mg II index, and proxy spectra |
| EUVS Flare Summary |
|
List of solar flares with times |
| EUVS High Resolution |
|
High temporal and spectral resolution EUVS measurements |
| XRS |
User Guide
Readme
Responsivity
|
|
| XRS 1-minute Averages |
|
1-minute averages of XRS measurements |
| XRS 1-second Fluxes |
|
High cadence measurements from the EXIS X-Ray Sensor (XRS) |
| XRS Daily Background |
|
Daily averages and background |
| XRS Flare Location |
|
Based on XRS quad diode measurements |
| XRS Flare Summary |
|
List of solar flares with times, flare classes and integrated fluxes |
| Full Resolution |
|
Full resolution magnetic field readings in different coordinate systems |
| 1-min Averages |
|
Averages of 10 Hz magnetometer field readings |
| Quiet Fields |
|
Magnetic field deviation from quiescent state |
| Geo-magnetopause Crossing |
|
Location of magnetopause and identification of when geo-magnetopause crosses satellite paths (Demo)
|
| Averages |
|
1-min and 5-min averages for the Magnetospheric Particle Sensors (MPS-HI and MPS-LO) and for the Solar and Galactic Proton Sensor (SGPS) |
| MPS-HI Moments and Spacecraft Charging |
|
Density and temperature moments and spacecraft charging level |
| MPS-LO Moments and Spacecraft Charging |
|
Density and temperature moments and spacecraft charging level |
| Event Detection |
|
Proton event detection (SGPS) |
| Rate of Rise |
|
Rate at which integral flux is increasing |
| LET |
|
Linear Energy Transfer measurements (measurement of harmful radiation) |
| High Dynamic Range (HDR) Images |
|
HDR images of the solar disk assembled from six different SUVI wavelengths |
| Fixed Difference Images |
|
Differences between the current solar image and a fixed reference image |
| Running Difference Images |
|
Differences between current solar image and previous image |
| Thematic Maps |
|
Color-coded images that identify flares, bright regions, coronal holes, and other solar features |
| Bright Regions |
|
Reports on bright/active regions |
| Flare Locations |
|
Reports on solar flares |
| Coronal Hole Boundaries |
|
Shape files for coronal hole boundaries |
| Satellite Location |
|
Satellite location (ephemeris) in multiple coordinates |
Links to L1b data directories are available for most of the GOES-R space weather instruments. Consult the ReadMe files below before using the data. Time-series L1b data are provided in daily or longer netCDF files. SUVI L1b images are in FITS format. Granular L1b netCDF files, each containing from 3 seconds to 5 minutes of data depending on the product, are provided via
CLASS.
Example codes to
use these
data.
GOES-R Level 1b Data: Space Weather Instruments
| Instrument |
Product |
Observation Interval |
File Access |
Description |
| EXIS EUVS L1b Solar Flux: EUV |
≤ 30 seconds |
|
EUV lines, MG II index and EUV modeled spectra.
More details
|
| EXIS XRS L1b Solar Flux: X-Ray |
1 second |
|
Soft X-ray fluxes.
More details
|
| Magnetometer L1b Geomagnetic Field |
0.1 second (10 Hz) |
|
Estimated ambient magnetic field in four coordinate reference frames.
More details |
|
SEISS EHIS L1b Energetic Heavy Ions
|
5 minutes |
|
Heavy ion differential fluxes derived from in situ measurements of heavy ion count rates.
More details
|
| SEISS MPS-Lo L1b Magnetospheric Electrons and Protons: Low Energy |
1 second |
|
Fluxes of relatively low energy electrons and ions derived from in situ measurements of electron and ion count rates.
More details
|
|
SEISS MPS-HI L1b Magnetospheric Electrons and Protons: High Energy
|
1 second |
|
Fluxes of medium and high energy electrons and protons derived from in situ measurements of electron and proton count rates.
More details
|
| SEISS SGPS L1b Solar and Galactic Protons |
1 second |
|
Fluxes of very high energy protons derived from in situ measurements of proton count rates.
More details
|
|
SUVI L1b Solar Imagery: EUV
|
10 seconds |
|
Solar images at six wavelengths and multiple radiance level ranges in support of viewing the sun during different types of solar activity. Image exposures are 10 msec or 1 sec.
More details |
SUVI Extended Coronal Imaging Data
Mosaic images of the extended solar corona from GOES-17 SUVI special observing campaigns are available for August-September 2018, August-December 2019, and April 2021. GOES-18 data
is now also available for July-September 2022.
Access: GOES-17 Data, GOES-18 Data and the ReadMe.
Geomagnetic Storms
2017-05-27 to 2017-05-28: A geomagnetic storm created various types of Ultra-low Frequency (ULF) waves in the magnetosphere. These waves were observed in space and on the ground, and the
GOES-14 and
GOES-16 magnetometer data are provided in order to
compare to ground-based measurements and models of ULF waves during the event. Data were created as part of the Geospace Environment Modeling (GEM) ULF Wave Modeling, Effects, and
Applications (UMEA) Challenge. See the
ReadMe for caveats associated with these data.
Solar Flares
September 2017: The GOES-16 Solar Ultraviolet Imager (SUVI) captured images of a series of flares in Sept. 2017. At this time, the instrument was still in Beta status. NCEI reprocessed Level 0 data to create Level 1b images. These files are organized by SUVI wavelength, for instance
Fe195 images. See the
ReadMe for caveats associated with these data.
L2 composites were also generated for this solar flare event. These L2 data are provisional and will be replaced in the future.
Solar Proton Events
September 2017: GOES-16 Solar and Galactic Proton Sensor (SGPS) data and comparisons
with GOES-13 and -15 EPS/EPEAD: All Data and Comparison Plots, ReadMe
GOES-R Space Weather Publications
| Authors |
Year |
Title |
Source |
Link |
| Barani, M, WC Tu, T Sarris, K Pham and RJ Redmon |
2019 |
Estimating the Azimuthal Mode Structure of ULF Waves Based on Multiple GOES Satellite Observations |
J. Geophys. Res-Space Phys. |
doi:10.1029/2019JA026927 |
| Boudouridis, A, JV Rodriguez, BT Kress, BK Dichter and TG Onsager |
2020 |
Development of a Bowtie Inversion Technique for Real-Time Processing of the GOES-16/-17 SEISS MPS-HI Electron Channels |
Space Weather |
doi:10.1029/2019SW002403 |
| Califf, S, D Early, M Grotenhuis, TM Loto'aniu and J Kronenwetter |
2019 |
Correcting the Arcjet Thruster Disturbance in GOES-16 Magnetometer Data |
Space Weather ARTN e2019SW002347 |
doi:10.1029/2019SW002347 |
| Darnel, JM, DB Seaton, C Bethge, L Rachmeler, A Jarvis, SM Hill, et al. |
2022 |
The GOES-R Solar UltraViolet Imager |
Space Weather |
doi:10.1029/2022SW003044 |
| Goodman, SJ, TJ Schmit, J Daniels and RJ Redmon |
2019 |
Chapter 23 - GOES-R Series Summary and Look Ahead |
The GOES-R Series |
doi:10.1016/C2015-0-06249-9 |
| Kress, BT, JV Rodriguez and TG Onsager |
2019 |
Chapter 20 - The GOES-R Space Environment In Situ Suite (SEISS): Measurement of Energetic Particles in Geospace |
The GOES-R Series |
doi:10.1016/C2015-0-06249-9 |
| Loto'aniu, TM, RJ Redmon, S Califf, HJ Singer, W Rowland, S Macintyre, C Chastain, R Dence, R Bailey, E Shoemaker, FJ Rich, D Chu, D Early, J Kronenwetter and M Todirita |
2019 |
The GOES-16 Spacecraft Science Magnetometer |
Space Sci. Rev. |
doi:10.1007/s11214-019-0600-3 |
| Loto’aniu, PTM, S Califf, RJ Redmon and HJ Singer |
2019 |
Chapter 21 - Magnetic Field Observations from the GOES-R Series |
The GOES-R Series |
doi:10.1016/C2015-0-06249-9 |
| Machol, JL, FG Eparvier, RA Viereck, DL Woodraska, M Snow, E Thiemann, TN Woods, WE McClintock, S Mueller, TD Eden, R Meisner, S Codrescu, SD Bouwer and AA Reinard |
2019 |
Chapter 19 - GOES-R Series Solar X-ray and Ultraviolet Irradiance |
The GOES-R Series |
doi:10.1016/C2015-0-06249-9 |
| Redmon, RJ, DB Seaton, R Steenburgh, J He, and JV Rodriguez |
2018 |
September
2017's geoeffective space weather and impacts to the Caribbean radio communications during hurricane
response |
Space Weather |
doi:10.1029/2018SW001897 |
| Seaton, DB and JM Darnel |
2018 |
Observations of an Eruptive Solar Flare in the Extended EUV Solar Corona |
Astrophys J Lett. |
doi:10.3847/2041-8213/aaa28e |
| Seaton, DB, JM Darnel, V Hsu and JM Hughes |
2019 |
Chapter 18 - GOES-R Series Solar Dynamics |
The GOES-R Series |
doi:10.1016/C2015-0-06249-9 |
| Seaton, DB, JM Hughes, SK Tadikonda, A Caspi, CE DeForest, A Krimchansky, NE Hurlburt, R Seguin, and G Slater |
2021 |
The Sun's dynamic extended corona observed in extreme ultraviolet |
Nature Astronomy |
doi:10.1038/s41550-021-01427-8 |
| Thiemann, EMB, FG Eparvier, D Woodraska, PC Chamberlin, J Machol, T Eden, AR Jones, R Meisner, S Mueller, M Snow, R Viereck and TN Woods |
2019 |
The GOES-R EUVS model for EUV irradiance variability |
J. Space Weather Space Clim. |
doi:10.1051/swsc/2019041 |
The GOES XRS science quality data have been reprocessed to update calibrations, fill gaps and to revise algorithms. Data provided include daily, monthly and mission-length files, as well as plots.
The GOES MAG data are reprocessed high-resolution versions of the operational GOES 8-15 MAG data that had not been previously made available at full resolution (2 Hz). The data were converted into GOES-R NetCDF and include daily files and plots.
Operational (real time) GOES 1-15 data
Science Quality GOES 1-15 Data: Space Weather Instruments
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