KABI KABI 291852Z 36011KT 7SM UP OVC007 M01/M03 A3014 RMK AO2 UPB44 SLP207 P0000 T10111028
KACT KACT 291907Z 36014KT 9SM OVC010 07/05 A3005 RMK AO2 T00720050
KADM KADM 291850Z 01013G20KT 10SM OVC009 M01/M04 A3016
KADS KADS 291847Z 32013G19KT 10SM OVC006 03/01 A3011
KAFW KAFW 291853Z 34016G23KT 7SM OVC007 01/M01 A3013 RMK AO2 SLP206 T00061011
KBAD KBAD 291855Z AUTO 16008KT 10SM -RA BKN008 OVC013 18/17 A2996 RMK AO2 RAB28E37RAB51 CIG 008V014 BKN V SCT SLPNO P0000 T01840167
KCNW KCNW 291855Z 33013KT 5SM -RA OVC007 08/06 A3007
KCSM KCSM 291853Z AUTO 01019G22KT 10SM OVC013 M07/M11 A3018 RMK AO2 SLP239 T10671106
KDAL KDAL 291853Z 33020G28KT 8SM OVC008 03/01 A3009 RMK AO2 PK WND 33028/1851 SLP188 T00330006 $
KDFW KDFW 291853Z 32020KT 7SM OVC007 02/M01 A3009 RMK AO2 SLP190 T00221006 $
KDTN KDTN 291853Z AUTO 14008KT 10SM OVC007 18/17 A2997 RMK AO2 RAB34E46 SLP146 P0000 T01830167
KDTO KDTO 291853Z 33013G18KT 9SM OVC006 00/M01 A3015 RMK AO2 SLP210 T00001011
KDYS KDYS 291855Z AUTO 36013KT 10SM OVC008 M01/M05 A3012 RMK AO2 PRESFR SLPNO T10121052
KFSI KFSI 291856Z AUTO 02017KT 10SM OVC012 M04/M08 A3016 RMK AO2 FZDZE56 SLPNO
KFTW KFTW 291853Z 32017G23KT 7SM OVC007 01/M01 A3011 RMK AO2 SLP196 T00061006
KFWS KFWS 291850Z 32017G21KT 6SM BR OVC007 02/00 A3011
KGGG KGGG 291900Z 36006KT 10SM BKN005 OVC036 18/17 A2996 RMK AO2 T01830172 $
KGKY KGKY 291853Z 31017G24KT 10SM OVC009 03/00 A3008 RMK AO2 PK WND 32028/1837 RAE03 SLP186 P0000 T00280000
KGPM KGPM 291850Z 33008G16KT 10SM OVC009 03/00 A3010
KGVT KGVT 291855Z AUTO 34016KT 7SM OVC004 03/02 A3008 RMK AO2 TSNO T00250017
KGYI KGYI 291850Z 35013KT 7SM OVC005 00/M01 A3013
KLAW KLAW 291753Z 35017G22KT 10SM OVC011 M04/M08 A3022 RMK AO2 SLP240 T10391083 11022 21044 50008
KLBB KLBB 291853Z 01007KT 10SM OVC010 M03/M06 A3009 RMK AO2 SLP202 T10281061
KLTS KLTS 291855Z AUTO 01014KT 10SM OVC017 M04/M09 A3018 RMK AO2 CIG 016 RWY18L CIG 016 RWY36R SLPNO T10391088 $
KMAF KMAF 291902Z 05014KT 6SM HZ SCT013 06/01 A3004 RMK AO2 T00560006
KMLU KMLU 291910Z 14004KT 3SM RA BR BKN048 OVC060 16/15 A3002 RMK AO2 P0005 T01610150
KNFW KNFW 291852Z 33018KT 6SM BR OVC009 01/M02 A3012 RMK AO2 PRESFR SLP182 T00061017 CHINO S VISNO S $
KOKC KOKC 291852Z 35017KT 10SM OVC008 M06/M08 A3019 RMK AO2 SLP237 T10611083
KOUN KOUN 291847Z 33015KT 10SM OVC007 M06/M08 A3018
KPWA KPWA 291853Z 35016KT 10SM OVC010 M06/M09 A3021 RMK AO2 SLP244 T10611094
KRBD KRBD 291853Z 33017G25KT 8SM OVC006 03/01 A3005 RMK AO2 PK WND 33028/1816 SLP176 T00280011
KSHV KSHV 291856Z 16007KT 9SM -RA OVC007 19/18 A2996 RMK RAB30 SLPNO
KSJT KSJT 291851Z 06008KT 9SM OVC010 07/03 A3007 RMK AO2 SLP184 T00670033
KSPS KSPS 291852Z 36015KT 10SM OVC014 M02/M06 A3020 RMK AO2 SLP228 T10221061
KTIK KTIK 291855Z 35017KT 10SM OVC007 M06/M07 A3016 RMK CIG 005 RWY13 SLPNO T10631068 $
KTKI KTKI 291853Z 34015KT 10SM OVC005 02/01 A3010 RMK AO2 SLP201 T00220011 $
KTXK KTXK 291853Z 34003KT 7SM -RA BKN007 BKN080 OVC100 18/15 A3001 RMK AO2 RAB22 SLP159 P0001 T01780150
KTYR KTYR 291903Z 32011KT 9SM SCT007 BKN011 OVC090 16/14 A2998 RMK AO2 T01610144

NEXRAD Radar For Dallas/Fort Worth
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This is a composite plot of the radar summary, echo tops, storm movement, TVS and MESO signatures and watch boxes. The radar summary is color coded by precip type. Greens, yellows and reds are rain. Pinks are mixed precipitation (freezing rain, sleet). Blues are snow. NOTE: Radar data is susceptible to a phenomena called anomalous propagation. This generally happens at night and appears as a area of 20 dBZ echos (darkest green) which is centered around each radar site and expands with time. To try and reduce the problem, low echo values near the radar sites have been removed.

GOES-16, formerly known as GOES-R before reaching geostationary orbit, is the first of the GOES-R series of Geostationary Operational Environmental Satellite (GOES) operated by NASA and the National Oceanic and Atmospheric Administration (NOAA). GOES-16 serves as the operational geostationary weather satellite in the GOES East position at 75.2°W, providing a view centered on the Americas. GOES-16 provides high spatial and temporal resolution imagery of the Earth through 16 spectral bands at visible and infrared wavelengths using its Advanced Baseline Imager (ABI). GOES-16's Geostationary Lightning Mapper (GLM) is the first operational lightning mapper flown in geostationary orbit. The spacecraft also includes four other scientific instruments for monitoring space weather and the Sun.
The Geostationary Operational Environmental Satellite (GOES) program began as a joint effort between the National Aeronautics and Space Administration (NASA) and the National Oceanic and Atmospheric Administration (NOAA) in 1975 to develop geostationary weather satellites following the success of the Applications Technology Satellite (ATS) and Synchronous Meteorological Satellite programs beginning in 1966. In the 1999 Operational Requirements Document (ORD) for the Evolution of Future NOAA Operational Geostationary Satellites, NOAA listed instrument requirements for the next generation of GOES imager and sounder. Top priorities included continuous observation capabilities, the ability to observe weather phenomena at all spatial scales, and improved spatial and temporal resolution for both the imager and sounder. These specifications laid the conceptual foundations for the instruments that would eventually be included with GOES-16.
Images updated every 5 minutes. NOAA GEOS-16
GOES 16 Visible Radar

The 0.47 micrometer (µm), or “blue” band, one of the two visible bands on the ABI, provides data for monitoring aerosols. The geostationary 0.47 µm band provides nearly continuous daytime observations of dust, haze, smoke and clouds. Measurements of aerosol optical depths (AOD) will help air quality monitoring and tracking, respectively. This blue band, combined with a “green” band and a “red” band (0.64 µm), can provide “simulated natural color” imagery of the Earth. The 0.47 µm band is also useful for air pollution studies and improving numerous products that rely on clear-sky radiances (such as land and sea surface products).
GOES 16 Longwave Infrared

The traditional longwave infrared window (11.2 micrometer (μm)) band enables operational meteorologists to diagnose discrete clouds and organized features for general weather forecasting, analysis, and broadcasting applications. Observations from this infrared window channel can characterize atmospheric processes associated with extratropical cyclones and also in single thunderstorms and convective complexes. The window channel also contributes to many satellite derived products, such as precipitation estimates, cloud-drift winds, hurricane intensity and track analyses, cloud-top heights, volcanic ash detection, as well as fog detection, cloud phase, and cloud particle size estimates.
GOES 16 Shortwave IR 4 Hour Loop

The shortwave IR window (3.9 micrometer (μm)) band (on the current GOES imagers) has been demonstrated to be useful in many applications, including fog/low cloud identification at night, fire/hot-spot identification, volcanic eruption and ash detection, and daytime snow and ice detection. Low-level atmospheric vector winds can also be estimated using this band. The shortwave IR window is also useful for studying urban heat islands and clouds. Compared to nighttime, there will be overall warmer temperatures in this shortwave window band during the day, due to the additional reflected solar component

Surface Data
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This is a composite map contain the following analyses: radar summary (color filled areas), surface data plot (composite station model), frontal locations (in various bold lines) and pressure contours (in thin blue lines).