ground flash fraction retrieval algorithm glm science meeting huntsville, al september 24, 2013

20
Ground Flash Fraction Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013 Dr. William Koshak, NASA-Marshall Space Flight Center Dr. Richard Solakiewicz, Chicago State University

Upload: megara

Post on 18-Mar-2016

20 views

Category:

Documents


0 download

DESCRIPTION

Ground Flash Fraction Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013 Dr. William Koshak, NASA-Marshall Space Flight Center Dr. Richard Solakiewicz, Chicago State University. Summary of Main Advances. Mathematical Advances to Analytic Perturbation Method - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

Ground Flash Fraction Retrieval Algorithm

GLM Science MeetingHuntsville, AL

September 24, 2013

Dr. William Koshak, NASA-Marshall Space Flight CenterDr. Richard Solakiewicz, Chicago State University

Page 2: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

Summary of Main Advances

Mathematical Advances to Analytic Perturbation Method Derived closed form solution for ground flash fraction … no

numerical scanning of H function. Derived explicit analytic forms for the perturbation vectors. Derived a way to determine flash type of specific flashes.

APM Error Analysis Completed Via Simulations

DEMO Completed

Journal Paper Completed & Ready for Submission (JTECH)

Page 3: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

MIX

(1 ) m g c

gNG g cNC c

NM m M G C

/gN N

Instrument ObservesN MGAs.

Invert this Distributionto Find Ground FlashFraction α

Page 4: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

APM SOLUTION PROCESS

(1 ) m g c

(1 )r r r r m g c

(truth)

(model)

Page 5: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

( )( )( ) (1 ) ( )

r rg

r r r r

g xP xg x c x

2

( ) ( )( )(1 )( )

( )

T

r

r r

r r

m b a ba b

g m a bc m a b

PROBABILITY FLASH, HAVING MGA = x, IS A GROUND FLASH:

( ) 0.5 Ground Flash

( ) 0.5 Cloud Flashg

g

P x

P x

APM SOLUTION SUMMARY

PERTURBATION GIVES:

Page 6: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

Simulate Population from OTD Data (Flash Type Categorized by NLDN)

Page 7: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

Simulate Population from LIS Data (Flash Type Categorized by NLDN)

Page 8: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013
Page 9: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF RANDOM ERROR (a = g, b = c)

NONE 8 km2 16 km2

32 km2 64 km2

Page 10: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF RANDOM ERROR (a and b from method)

NONE 8 km2 16 km2

32 km2 64 km2

Page 11: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF SYSTEMATIC ERROR (a = g, b = c)

NONE 8 km2 16 km2

-8 km2 -16 km2 DIGITAL(16 km2 finite footprint)

Page 12: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF SYSTEMATIC ERROR (a and b from method)

NONE 8 km2 16 km2

-8 km2 -16 km2 DIGITAL(16 km2 finite footprint)

Page 13: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF CLIMATOLOGY SAMPLE SIZE

Ng = 40,000Nc = 120,000

Ng = 10,000Nc = 30,000

Ng = 5,000Nc = 5,000

Ng = 1,000Nc = 1,000

Ng = 500Nc = 500

Ng = 200Nc = 200

Page 14: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

EFFECT OF OBSERVATION SAMPLE SIZE N

N = 5,000N = 7,500 N = 2,500

N = 1,000 N = 500

Page 15: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

NOMINAL (LIS data)

# Observations:N = 5000

# in Climate Sampling:Ng = 40,000Nc = 120,000

Instr. Measurement Error:Random = ±32 km2Systematic = 16 km2 digital

gpop mean = 465.4 km2cpop mean = 251.9 km2difference = 213.5 km2

Mean Error = 0.027Std = 0.022

Page 16: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

NOMINAL (OTD data)

# Observations:N = 5000

# in Climate Sampling:Ng = 40,000Nc = 120,000

Instr. Measurement Error:Random = ±128 km2Systematic = 64 km2 digital

gpop mean = 493.0 km2cpop mean = 215.6 km2difference = 277.4 km2

Mean Error = 0.018Std = 0.014

Page 17: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

CAN HANDLE ARBITRARY DISTRIBUTIONS (AS USUAL, CG & IC DISTRIBUTIONS NEED TO BE DISTINCT)

Page 18: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

PERFORMANCE OF SPECIFIC FLASH TYPING

Mean Fraction Correct = 0.780Std = 0.131

LIS data

Mean Fraction Correct = 0.797Std = 0.119

OTD data

Page 19: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

FUNCTIONAL DEMO NOW EXISTS

Page 20: Ground Flash Fraction  Retrieval Algorithm GLM Science Meeting Huntsville, AL September 24, 2013

Thank You