The GOES‐R Solar UltraViolet Imager
Abstract The four Solar Ultraviolet Imagers (SUVI) on board the Geostationary Operational Environmental Satellite (GOES)‐16 and GOES‐17 and the upcoming GOES‐T and GOES‐U weather satellites serve as National Oceanic and Atmospheric Administration's operational solar coronal imagers. These four...
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Format: | Article |
Language: | English |
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Wiley
2022-04-01
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Series: | Space Weather |
Online Access: | https://doi.org/10.1029/2022SW003044 |
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author | Jonathan M. Darnel Daniel B. Seaton Christian Bethge Laurel Rachmeler Alison Jarvis Steven M. Hill Courtney L. Peck J. Marcus Hughes Jason Shapiro Allyssa Riley Gopal Vasudevan Lawrence Shing George Koener Chris Edwards Dnyanesh Mathur Shelbe Timothy |
author_facet | Jonathan M. Darnel Daniel B. Seaton Christian Bethge Laurel Rachmeler Alison Jarvis Steven M. Hill Courtney L. Peck J. Marcus Hughes Jason Shapiro Allyssa Riley Gopal Vasudevan Lawrence Shing George Koener Chris Edwards Dnyanesh Mathur Shelbe Timothy |
author_sort | Jonathan M. Darnel |
collection | DOAJ |
description | Abstract The four Solar Ultraviolet Imagers (SUVI) on board the Geostationary Operational Environmental Satellite (GOES)‐16 and GOES‐17 and the upcoming GOES‐T and GOES‐U weather satellites serve as National Oceanic and Atmospheric Administration's operational solar coronal imagers. These four identically designed solar Extreme UltraViolet instruments are similar in design and capability to the Solar Dynamics Observatory‐Atmospheric Imaging Assembly suite of solar telescopes, and are planned to operationally span two solar cycles or more, from 2017 through 2040. We present the concept of operations for the SUVI instruments, operational requirements, and constraints. The reader is also introduced to the instrument design, testing, and performance characteristics. Finally, the various data products are described along with their potential utility to the operational user or researcher. |
format | Article |
id | doaj-art-6530187210594aed9a13bcd60541f6de |
institution | Kabale University |
issn | 1542-7390 |
language | English |
publishDate | 2022-04-01 |
publisher | Wiley |
record_format | Article |
series | Space Weather |
spelling | doaj-art-6530187210594aed9a13bcd60541f6de2025-01-14T16:27:24ZengWileySpace Weather1542-73902022-04-01204n/an/a10.1029/2022SW003044The GOES‐R Solar UltraViolet ImagerJonathan M. Darnel0Daniel B. Seaton1Christian Bethge2Laurel Rachmeler3Alison Jarvis4Steven M. Hill5Courtney L. Peck6J. Marcus Hughes7Jason Shapiro8Allyssa Riley9Gopal Vasudevan10Lawrence Shing11George Koener12Chris Edwards13Dnyanesh Mathur14Shelbe Timothy15Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USANational Centers for Environmental Information National Oceanic and Atmospheric Administration Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USASpace Weather Prediction Center National Oceanic and Atmospheric Administration Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USASouthwest Research Institute Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USACooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USALockheed Martin Advanced Technology Center Palo Alto CA USALockheed Martin Advanced Technology Center Palo Alto CA USALockheed Martin Advanced Technology Center Palo Alto CA USALockheed Martin Advanced Technology Center Palo Alto CA USALockheed Martin Advanced Technology Center Palo Alto CA USALockheed Martin Advanced Technology Center Palo Alto CA USAAbstract The four Solar Ultraviolet Imagers (SUVI) on board the Geostationary Operational Environmental Satellite (GOES)‐16 and GOES‐17 and the upcoming GOES‐T and GOES‐U weather satellites serve as National Oceanic and Atmospheric Administration's operational solar coronal imagers. These four identically designed solar Extreme UltraViolet instruments are similar in design and capability to the Solar Dynamics Observatory‐Atmospheric Imaging Assembly suite of solar telescopes, and are planned to operationally span two solar cycles or more, from 2017 through 2040. We present the concept of operations for the SUVI instruments, operational requirements, and constraints. The reader is also introduced to the instrument design, testing, and performance characteristics. Finally, the various data products are described along with their potential utility to the operational user or researcher.https://doi.org/10.1029/2022SW003044 |
spellingShingle | Jonathan M. Darnel Daniel B. Seaton Christian Bethge Laurel Rachmeler Alison Jarvis Steven M. Hill Courtney L. Peck J. Marcus Hughes Jason Shapiro Allyssa Riley Gopal Vasudevan Lawrence Shing George Koener Chris Edwards Dnyanesh Mathur Shelbe Timothy The GOES‐R Solar UltraViolet Imager Space Weather |
title | The GOES‐R Solar UltraViolet Imager |
title_full | The GOES‐R Solar UltraViolet Imager |
title_fullStr | The GOES‐R Solar UltraViolet Imager |
title_full_unstemmed | The GOES‐R Solar UltraViolet Imager |
title_short | The GOES‐R Solar UltraViolet Imager |
title_sort | goes r solar ultraviolet imager |
url | https://doi.org/10.1029/2022SW003044 |
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