Exploiting SNPP VIIRS Day Night Band (DNB) for Tropical ... · Steve Miller2, Charles Sampson1,...

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Jeff Hawkins 1 , Jeremy Solbrig 1 , Mindy Surratt 1 , Kim Richardson 1 , Steve Miller 2 , Charles Sampson 1 , John Kent 3 , and Tom Lee 1 1 Naval Research Laboratory, Monterey, CA 2 Cooperative Institute for Research in the Atmosphere (CIRA), Ft. Collins, CO 3 Science Applications International Inc., Monterey, CA March 1, 2007 OFCM Interdepartmental Hurricane Conference March 5, 2014 Exploiting SNPP VIIRS Day Night Band (DNB) for Tropical Cyclone Monitoring 1

Transcript of Exploiting SNPP VIIRS Day Night Band (DNB) for Tropical ... · Steve Miller2, Charles Sampson1,...

Page 1: Exploiting SNPP VIIRS Day Night Band (DNB) for Tropical ... · Steve Miller2, Charles Sampson1, John Kent3, and Tom Lee1 1Naval Research Laboratory, Monterey, CA 2Cooperative Institute

Jeff Hawkins1, Jeremy Solbrig1, Mindy Surratt1, Kim Richardson1, Steve Miller2, Charles Sampson1, John Kent3, and Tom Lee1

1Naval Research Laboratory, Monterey, CA2Cooperative Institute for Research in the Atmosphere (CIRA), Ft.

Collins, CO3Science Applications International Inc., Monterey, CA

March 1, 2007OFCM Interdepartmental Hurricane ConferenceMarch 5, 2014

Exploiting SNPP VIIRS Day Night Band (DNB) for Tropical Cyclone Monitoring

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Naval Research Laboratory - MontereyNaval Research Laboratory - MontereyOFCM Interdepartmental Hurricane ConferenceOFCM Interdepartmental Hurricane Conference

Suomi NPP VIIRSSpacecraft: Suomi National Polar-orbiting Partnership (NPP)Sensor: Visible Infrared Imager Radiometer Suite (VIIRS)Launch Date: October 28, 2011Heritage: AVHRR, OLS, MODISChannels: 22 including day/night band (DNB) Swath Width: ~3000 kmApplication Enhancements: a) 22 channels b) 14-bit digitizationc) Wider swathd) DNB – night time visible (740 m)e) Retain resolution to scan edge

Courtesy of Raytheon Space and Airborne Systems

• .63 µm• .86 µm• 1.6 µm• 3.7 µm• 11.4 µm

Wavelength

1.1 km .25–1 km 0.37 km

AVHRR MODIS VIIRS

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Lunar Reflection

Lunar ReflectionLight Emission

Gray / Blue shading = Solar / Lunar illuminationRed / Blue lines = Solar / Lunar terminators

• ~40% of nighttime data offer lunar coverage > ¼ moon (annual average; 0930 orbit).

• Current low-light system: DMSP/OLS photomultiplier tube enables detection of light levels ~5 orders of magnitude lower than conventional VIS sensors.

• SNPP/VIIRS Day Night Band (DNB) has major advances to nighttime imagery capability (resolution, calibration, digitization.)

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Typhoon Jelawat, 9-25-12 17Z shown here…

Moon is setting in the west during this DNB nighttime overpass.

Faint lunar illumination on eastern eyewall

Lightning flash in outer band

Taiwan city lights

Manila city lights

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Miller and Turner, 2009. IEEE Trans. Geosci. Rem. Sens., 47(7), 2316-2329.

A lunar irradiance prediction model to allow conversion from DNB radiance to reflectance units

R = πI↑ / [cos(θm)Em]

Enables quantitative applications from measurements of reflected moonlight

Miller et al.. 2012. J. Atmos. Ocean. Tech., 29, 538-557.

A lunar availability assessment for the VIIRS/DNB to determine when and where nighttime lunar applications are possible for NPP and other polar orbits.

~45% all nights at mid-latitudes offer sufficient levels of moonlight

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Lunar model is used to produce a form of near constant contrast (NCC) imagery.

Not applicable to the day/night terminator where solar signal is present.

Moon phase: 80%

Manila city lights

Cut off line for lunar model

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Tropical Depression 30W, 11-12-13 19Z shown here…

DNB radiance image, overshooting tops near “apparent center”, but can’t view cloud field reliably on eastern ½ due to lack of illumination

Moon phase: 81%, but moon setting to the west

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Tropical Depression 30W, 11-12-13 19Z shown here…

DNB “reflectance”, using the NRL-MRY lunar model to convert the radiances + IR

Low clouds – yellowHigh clouds – white/cyan

Analyst now able to better comprehend the 3-D cloud structure

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Tropical Storm Flossie7-29-2013 1102Z

Longwave IR

Storm “heading” towards Big Island (Hawaii) landfall with future track WNW

Hawaii

Maui

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VIIRS DNB radiance image coincident with previous IR

Can see through thin cirrus to low level clouds below

740 m spatial resolution across the entire 3000 km swath (note edge of swath over Maui)

Hawaii

Maui

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VIIRS DNB reflectance image after correction via the NRL-MRY lunar model:

Takes into account:a) Lunar phaseb) Moon-satellite-storm

viewing geometry

Only done when sufficient lunar illumination available

Hawaii

Maui

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VIIRS DNB reflectance + IR reveals LLCC displaced ~60 nm from IR mid-level convection center, low clouds – yellow, high clouds white/cyan.

CPHC Warning :- Relocated TS Flossie

center fix well north- Landfall no longer on

island of Hawaii- Revised track now

impacts area along northern coasts

Hawaii

Maui

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Shear & Low-Level Circulation Centers

VIIRS DNB reflectance + IR excellent tool for detecting low-level circulation centers (LLCC) due to shear

05L Erin 08-18-13 09L Humberto 09-17-13

CIMSS Shear241/21 kts

CIMSS Shear279/24 kts

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Hot Towers & Overshooting Tops

VIIRS DNB reflectance products can isolate convective bursts (hot towers) associated with intensity changes

16E Priscilla 10-16-13 20W Twenty 09-26-13

97% 50%

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Tropical Cyclone Eyes

DNB night time visible can assist IR in determining eye structure, eye size, and tilt

04S Bruce 12-21-13 28W Lekima 10-23-1339% 98%

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Lightning

VIIRS DNB lightning detection captures a small % of total flashes due to scene scanning realities

91L Invest 07-30-13 09L Humberto 09-17-13

39% 98%

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Nighttime TC Monitoring Via DNB

Summary

VIIRS DNB has “unique” TC monitoring features DNB fills a visible data void at night Excellent tool for viewing low-level circulation centers

LLCC (sheared and genesis systems) Assists in detecting TC 3-D cloud structure Highlights overshooting tops (hot towers) Helps view TC “clear or open” eyes with IR data Identifies isolated lightning flashes Will add ~ 10 months of DNB data to NRL TC page shortly

[email protected]