The GOES-R Series 2020
DOI: 10.1016/b978-0-12-814327-8.00018-4
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GOES-R Series Solar Dynamics

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Cited by 7 publications
(4 citation statements)
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“…Level‐2 SUVI products are created and available through SWPC as forecast products in PNG format with latency less than 5 minutes, or from the National Centers for Environmental Information (NCEI) as science products with a latency of a few hours. A detailed discussion of SUVI observations and data products appears in (Seaton et al., 2020). Figure 14 shows an overview of different SUVI data products and the flow from data level to data level.…”
Section: Suvi Productsmentioning
confidence: 99%
“…Level‐2 SUVI products are created and available through SWPC as forecast products in PNG format with latency less than 5 minutes, or from the National Centers for Environmental Information (NCEI) as science products with a latency of a few hours. A detailed discussion of SUVI observations and data products appears in (Seaton et al., 2020). Figure 14 shows an overview of different SUVI data products and the flow from data level to data level.…”
Section: Suvi Productsmentioning
confidence: 99%
“…Level-2 SUVI products are created and available through SWPC as forecast products in PNG format with latency less than five minutes, or from the National Centers for Environmental Information (NCEI) as science products with a latency of a few hours. A detailed discussion of SUVI observations and data products appears in (Seaton et al, 2020). Figure 13 shows an overview of different SUVI data products and the flow from data level to data level.…”
Section: Suvi Productsmentioning
confidence: 99%
“…A host of real‐time observational data are available to SWPC forecasters to support adjustments to the proton event climatological probabilities described in step 3. Examples include solar active region magnetogram data from GONG (Hill, 2018), products from the Solar Dynamic Observatory (SDO: Pesnell et al., 2012) Helioseismic and Magnetic Imager (HMI: Schou et al., 2012), imagery from the SDO Atmospheric Imaging Assembly (Lemen et al., 2012) and the GOES Solar UltraViolet Imager (Seaton et al., 2020; Vasudevan et al., 2019), as well as GOES X‐ray and proton data. Input from the United States Air Force solar region and activity reports, containing plain text information remarking on active region characteristics, is also considered.…”
Section: Probabilistic Proton Event Productsmentioning
confidence: 99%