Split Window Difference (10.3mm – 12.3mm): Quick Guide
The Split Window Difference (SWD) is a Brightness Temperature Difference (BTD) field that highlights low-level moisture and dust. Moisture can be detected because there is more absorption by water vapor of energy at wavelengths in the ‘Dirty Window’ Channel (12.3 µm) than in the ‘Clean Window’ (10.3...
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| Corporate Authors: | , |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
[Washington, D.C.,]
NASA
2017
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| Subjects: | |
| Online Access: | Volltext |
| Summary: | The Split Window Difference (SWD) is a Brightness Temperature Difference (BTD) field that highlights low-level moisture and dust. Moisture can be detected because there is more absorption by water vapor of energy at wavelengths in the ‘Dirty Window’ Channel (12.3 µm) than in the ‘Clean Window’ (10.3 µm). Dust can be detected because airborne silicates absorb more 10.3 µm energy than 12.3 µm energy. More absorption of energy leads to colder brightness temperatures. In the image at right, lighter grays highlight a greater SWD, i.e., more moisture in the atmosphere. Convection later forms on the moist axis |
| Physical Description: | 1 Online-Ressource (2 Seiten) |
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| 520 | 3 | |a The Split Window Difference (SWD) is a Brightness Temperature Difference (BTD) field that highlights low-level moisture and dust. Moisture can be detected because there is more absorption by water vapor of energy at wavelengths in the ‘Dirty Window’ Channel (12.3 µm) than in the ‘Clean Window’ (10.3 µm). Dust can be detected because airborne silicates absorb more 10.3 µm energy than 12.3 µm energy. More absorption of energy leads to colder brightness temperatures. In the image at right, lighter grays highlight a greater SWD, i.e., more moisture in the atmosphere. Convection later forms on the moist axis | |
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| spelling | USA National Oceanic and Atmospheric Administration Verfasser (DE-588)18185-7 aut Split Window Difference (10.3mm – 12.3mm) Quick Guide Contributor: Scott Lindstrom, Jordan Gerth, Tim Schmit [Washington, D.C.,] NASA 2017 1 Online-Ressource (2 Seiten) txt rdacontent c rdamedia cr rdacarrier The Split Window Difference (SWD) is a Brightness Temperature Difference (BTD) field that highlights low-level moisture and dust. Moisture can be detected because there is more absorption by water vapor of energy at wavelengths in the ‘Dirty Window’ Channel (12.3 µm) than in the ‘Clean Window’ (10.3 µm). Dust can be detected because airborne silicates absorb more 10.3 µm energy than 12.3 µm energy. More absorption of energy leads to colder brightness temperatures. In the image at right, lighter grays highlight a greater SWD, i.e., more moisture in the atmosphere. Convection later forms on the moist axis Satellitenmeteorologie (DE-588)4140530-4 gnd rswk-swf Meteorologie (DE-588)4038953-4 gnd rswk-swf Fernerkundung (DE-588)4016796-3 gnd rswk-swf Split Window Difference Geostationary Operational Environmental Satellites (GOES-R) Satellitenmeteorologie (DE-588)4140530-4 s Fernerkundung (DE-588)4016796-3 s DE-604 Meteorologie (DE-588)4038953-4 s Lindstrom, Scott Sonstige oth Gerth, Jordan Sonstige oth Schmit, Tim Sonstige oth USA National Aeronautics and Space Administration Verfasser (DE-588)2294-9 aut https://cimss.ssec.wisc.edu/goes/OCLOFactSheetPDFs/ABIQuickGuide_SplitWindowDifference.pdf Archivierung kostenfrei Volltext |
| spellingShingle | Split Window Difference (10.3mm – 12.3mm) Quick Guide Satellitenmeteorologie (DE-588)4140530-4 gnd Meteorologie (DE-588)4038953-4 gnd Fernerkundung (DE-588)4016796-3 gnd |
| subject_GND | (DE-588)4140530-4 (DE-588)4038953-4 (DE-588)4016796-3 |
| title | Split Window Difference (10.3mm – 12.3mm) Quick Guide |
| title_auth | Split Window Difference (10.3mm – 12.3mm) Quick Guide |
| title_exact_search | Split Window Difference (10.3mm – 12.3mm) Quick Guide |
| title_full | Split Window Difference (10.3mm – 12.3mm) Quick Guide Contributor: Scott Lindstrom, Jordan Gerth, Tim Schmit |
| title_fullStr | Split Window Difference (10.3mm – 12.3mm) Quick Guide Contributor: Scott Lindstrom, Jordan Gerth, Tim Schmit |
| title_full_unstemmed | Split Window Difference (10.3mm – 12.3mm) Quick Guide Contributor: Scott Lindstrom, Jordan Gerth, Tim Schmit |
| title_short | Split Window Difference (10.3mm – 12.3mm) |
| title_sort | split window difference 10 3mm 12 3mm quick guide |
| title_sub | Quick Guide |
| topic | Satellitenmeteorologie (DE-588)4140530-4 gnd Meteorologie (DE-588)4038953-4 gnd Fernerkundung (DE-588)4016796-3 gnd |
| topic_facet | Satellitenmeteorologie Meteorologie Fernerkundung |
| url | https://cimss.ssec.wisc.edu/goes/OCLOFactSheetPDFs/ABIQuickGuide_SplitWindowDifference.pdf |
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