Effects of Non-Spherical Ice Crystal Shape on Modeled Properties of Thin Tropical Tropopause Layer Cirrus

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Rick Russotto
Dept. of
Atmospheric
Sciences,
Univ. of
Washington
With:
Tom Ackerman
Dale Durran
ATTREX
Science Team
Meeting
Boulder, CO
October 21,
2014
EFFECTS OF NON-
SPHERICAL ICE CRYSTAL
SHAPE ON MODELED
PROPERTIES OF THIN
TROPICAL TROPOPAUSE
LAYER CIRRUS
Support:
NSF grant ATM-0926996
Dept. of Defense NDSEG Fellowship
Cirrus in TTL important for:
Radiative absorption
Water vapor transport into stratosphere
Why use a cloud-resolving model?
Understand effects of mesoscale, radiatively induced circulations
Previous work 
(Dinh 
et al.
, 2010, 2012, 2014)
 assumed all
spheres
Observations 
(Lawson 
et al.
, 2008)
 suggest at least some plates and
columns
Existing code could not maintain largest crystals
INTRODUCTION
New simulations incorporate more realistic ice crystal shapes
Fall speed
Growth rate
Radiative absorption
How does this affect time evolution of clouds?
INTRODUCTION
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MODEL OVERVIEW
Dynamics:
System for Atmospheric Modeling (SAM)
(Khairoutdinov and Randall, 2003)
Microphysics:
Bin microphysics scheme 
(Dinh and Durran, 2012)
 
Radiation:
Lookup table of broadband ice crystal absorption cross sections
COMPONENTS OF MODEL
 
Domain:
2D (
x
 and 
z
)
432 km (
x
) by 3.25 km (
z
)
Δ
x 
= 100 m
Δ
z 
= 25 m
Δ
t
 = 6 s
 
 
 
SIMULATION SETUP
 
Initialization:
No large-scale flow
Pre-existing cloud
Ice crystals: 3 
μ
m radius
Sounding: Nauru,
 
           January average
 
 
For microphysics: oblate and
prolate spheroids
For radiation:
Collection of spheres
Conserve SA/Volume ratio
(Neshyba et al., 2003)
 
Aspect ratio of 6 for now
 
REPRESENTING PLATES AND COLUMNS
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FALL SPEED
Stokes regime:
Large enough that fluid is continuum
Small enough that fluid’s inertia is negligible
Analytical expression for terminal velocity
Corrections for spheroids: functions only of aspect ratio
(Fuchs, 
Mechanics of Aerosols
, 1964)
Orientation: maximize horizontal cross section
FALL SPEED: CALCULATION
FALL SPEED: EFFECT OF SHAPE
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GROWTH RATES
GROWTH RATE: CALCULATION
GROWTH RATE: EFFECT OF SHAPE
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RADIATIVE ABSORPTION
Single scattering
properties:
Extinction cross
section (
λ
)
Absorption 
 
cross
section (
λ
)
Asymmetry factor
(
λ
)
 
Mie
scattering
code
Cloud,
temperature,
gas profiles
SW and LW fluxes
at cloud
boundaries
 
1-D spectral
radiative
transfer model
Broadband
absorption cross
sections
Ice crystal properties:
Mass
Aspect ratio
 
Invert SAM
radiation
scheme
RADIATION: PARAMETERIZATION PROCESS
Bulk ice properties:
Complex  refractive
index (
λ
)
RADIATION: EFFECT OF SHAPE
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RESULTS AND
FUTURE WORK
CIRCULATION AT 6 HOURS
CLOUD AT 24 HOURS
LIFTING OF CLOUD
 
Preliminary: additional lifting due to
Fall speeds (2/3)
Radiation (1/3)
TOTAL CLOUD MASS
Distinguish effects of fall speed, growth rate, and radiation
Other ways to get single-scattering properties
T-Matrix method 
(Mishchenko & Travis, 1998)
Improved geometric optics method 
(Yang & Liou, 1996)
Use of ATTREX data:
Ice crystal size distributions (also habits)
Environmental water vapor distributions
Inertial-gravity waves?
FUTURE WORK
undefined
QUESTIONS?
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ADDITIONAL SLIDES
CIRCULATION AT 6 HOURS
Other ways to get single-scattering properties
T-Matrix method 
(Mishchenko & Travis, 1998)
Improved geometric optics method 
(Yang & Liou, 1996)
Existing databases 
(Fu et al., 1999; Yang et al., 2013)
Exact scattering solution for spheroids 
(Asano & Sato, 1980)
GROWTH RATE: CALCULATION
m 
= ice crystal mass
C
 = capacitance
S
ice
 = saturation ratio w.r.t. ice
R
v
 = gas constant for water vapor
T 
= temperature
e
sat,ice
 = sat. vapor pressure over plane surface
L
s
 
= latent heat of sublimation
k’
a
 
= modified thermal conductivity of air
D’
v
 
= modified diffusivity of water vapor in air
GROWTH RATE: CAPACITANCE METHOD
m 
= ice crystal mass
C
 = capacitance
S
ice
 = saturation ratio w.r.t. ice
R
v
 = gas constant for water vapor
T 
= temperature
e
sat,ice
 = saturation vapor pressure over plane surface
L
s
 
= latent heat of sublimation
k’
a
 
= modified thermal conductivity of air
D’
v
 
= modified diffusivity of water vapor in air
r 
= radius of sphere
a = semi-major axis of ellipse of revolution
b = semi-minor axis  “     “        “      “
e = eccentricity           “     “        “      “
A = linear eccentricity “     “        “      “
MORE ON GROWTH RATE
Field
discontinuity
corrections for
thermal
conductivity
and water
vapor
diffusivity (D
v
’,
k
a
’) depend on
particle size.
What measure
of size to use
for spheroids?
Makes a big
difference.
FALL SPEEDS
FALL SPEEDS
FALL SPEED: STOKES’ LAW METHOD
β
 
= aspect ratio
= (major axis)/
(minor axis)
FALL SPEED: STOKES’ LAW METHOD
MEAN ICE CRYSTAL MASS
PARTICLE SIZE DISTRIBUTIONS
Note: these
are earlier
simulations
that did not
consider
effects of
shape on
radiation,
and also had
a different
growth rate
calculation.
PARTICLE SIZE DISTRIBUTIONS
Starting Bin
PARTICLE SIZE DISTRIBUTIONS
Starting Bin
PARTICLE SIZE DISTRIBUTIONS
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This study explores the impact of non-spherical ice crystal shapes on the properties of cirrus clouds in the thin tropical tropopause layer. Incorporating realistic ice crystal shapes into models affects fall speed, growth rate, and radiative absorption, influencing the time evolution of clouds. The model overview includes dynamics, microphysics, and radiation components, with a focus on representing plates and columns. The calculation of fall speed considers the Stokes regime, analytical expressions for terminal velocity, and corrections for spheroids based on aspect ratio.

  • Ice crystal shape
  • Cirrus clouds
  • Tropical tropopause
  • Fall speed
  • Cloud modeling

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  1. EFFECTS OF NON- SPHERICAL ICE CRYSTAL SHAPE ON MODELED PROPERTIES OF THIN TROPICAL TROPOPAUSE LAYER CIRRUS Rick Russotto Dept. of Atmospheric Sciences, Univ. of Washington With: Tom Ackerman Dale Durran ATTREX Science Team Meeting Support: Boulder, CO NSF grant ATM-0926996 Dept. of Defense NDSEG Fellowship October 21, 2014

  2. INTRODUCTION Cirrus in TTL important for: Radiative absorption Water vapor transport into stratosphere Why use a cloud-resolving model? Understand effects of mesoscale, radiatively induced circulations Previous work (Dinh et al., 2010, 2012, 2014) assumed all spheres Observations (Lawson et al., 2008) suggest at least some plates and columns Existing code could not maintain largest crystals

  3. INTRODUCTION New simulations incorporate more realistic ice crystal shapes Fall speed Growth rate Radiative absorption How does this affect time evolution of clouds?

  4. MODEL OVERVIEW

  5. COMPONENTS OF MODEL Dynamics: System for Atmospheric Modeling (SAM) (Khairoutdinov and Randall, 2003) Microphysics: Bin microphysics scheme (Dinh and Durran, 2012) Radiation: Lookup table of broadband ice crystal absorption cross sections

  6. SIMULATION SETUP Initialization: No large-scale flow Pre-existing cloud Ice crystals: 3 m radius Sounding: Nauru, January average Domain: 2D (x and z) 432 km (x) by 3.25 km (z) x = 100 m z = 25 m t = 6 s

  7. REPRESENTING PLATES AND COLUMNS For microphysics: oblate and prolate spheroids For radiation: Collection of spheres Conserve SA/Volume ratio (Neshyba et al., 2003) Aspect ratio of 6 for now

  8. FALL SPEED

  9. FALL SPEED: CALCULATION Stokes regime: Large enough that fluid is continuum Small enough that fluid s inertia is negligible Analytical expression for terminal velocity Corrections for spheroids: functions only of aspect ratio (Fuchs, Mechanics of Aerosols, 1964) Orientation: maximize horizontal cross section

  10. FALL SPEED: EFFECT OF SHAPE

  11. GROWTH RATES

  12. GROWTH RATE: CALCULATION How to account for both size and shape? Electrostatic analogy: growth rate capacitance Equal to radiusfor spheres Spheroids: function of major and minor axes capacitance

  13. GROWTH RATE: EFFECT OF SHAPE

  14. RADIATIVE ABSORPTION

  15. RADIATION: PARAMETERIZATION PROCESS Ice crystal properties: Mass Aspect ratio Single scattering properties: Extinction cross section ( ) Absorption cross section ( ) Asymmetry factor ( ) Mie scattering code Cloud, temperature, gas profiles Bulk ice properties: Complex refractive index ( ) 1-D spectral radiative transfer model Broadband absorption cross sections SW and LW fluxes at cloud boundaries Invert SAM radiation scheme

  16. RADIATION: EFFECT OF SHAPE

  17. RESULTS AND FUTURE WORK

  18. CIRCULATION AT 6 HOURS u (m/s), 6 hours Z (km) Z (km) w (m/s), 6 hours Z (km) Z (km)

  19. CLOUD AT 24 HOURS

  20. LIFTING OF CLOUD Preliminary: additional lifting due to Fall speeds (2/3) Radiation (1/3)

  21. TOTAL CLOUD MASS

  22. FUTURE WORK Distinguish effects of fall speed, growth rate, and radiation Other ways to get single-scattering properties T-Matrix method (Mishchenko & Travis, 1998) Improved geometric optics method (Yang & Liou, 1996) Use of ATTREX data: Ice crystal size distributions (also habits) Environmental water vapor distributions Inertial-gravity waves?

  23. QUESTIONS?

  24. ADDITIONAL SLIDES

  25. CIRCULATION AT 6 HOURS u (m/s), 6 hours Z (km) Z (km) w (m/s), 6 hours Z (km) Z (km) (m/s), 6 hours Z (km) Z (km)

  26. Other ways to get single-scattering properties T-Matrix method (Mishchenko & Travis, 1998) Improved geometric optics method (Yang & Liou, 1996) Existing databases (Fu et al., 1999; Yang et al., 2013) Exact scattering solution for spheroids (Asano & Sato, 1980)

  27. GROWTH RATE: CALCULATION General growth rate equation: (Pruppacher and Klett, 1978) ?? ??= 4??(?ice 1) ?v? ?sat,ice? v + ?? ?? ?v? 1 ? a? m = ice crystal mass C = capacitance Sice = saturation ratio w.r.t. ice Rv = gas constant for water vapor T = temperature esat,ice = sat. vapor pressure over plane surface Ls= latent heat of sublimation k a= modified thermal conductivity of air D v= modified diffusivity of water vapor in air Shape dependence for: C D v k a

  28. GROWTH RATE: CAPACITANCE METHOD General growth rate equation (Pruppacher and Klett, 1978): ?? ??= 4??(?ice 1) ?v? ?sat,ice? v + ?v? 1 ?? ?? ? a? Expressions for capacitance, C: Spheres: C = r Oblate spheroids: m = ice crystal mass C = capacitance Sice = saturation ratio w.r.t. ice Rv = gas constant for water vapor T = temperature esat,ice = saturation vapor pressure over plane surface Ls= latent heat of sublimation k a= modified thermal conductivity of air D v= modified diffusivity of water vapor in air r = radius of sphere ?2 ?2 ?? sin 1 ?where ? = ? = 1 Prolate spheroids: ? ?+? ? ? = ?2 ?2 where ? = ln a = semi-major axis of ellipse of revolution b = semi-minor axis e = eccentricity A = linear eccentricity

  29. MORE ON GROWTH RATE Field discontinuity corrections for thermal conductivity and water vapor diffusivity (Dv , ka ) depend on particle size. What measure of size to use for spheroids? Makes a big difference.

  30. FALL SPEEDS Stokes regime: Large enough that fluid is a continuum Small enough that fluid s inertia is negligible Analytical expression for drag coefficient And therefore terminal velocity For spheres: ??=2 9 ????? ???? ?2

  31. FALL SPEEDS Corrections for spheroids from Fuchs, Mechanics of Aerosols (1964) Dynamic shape factor : rate of settling of equivalent mass sphere rate of settling of spheroid particle function only of aspect ratio =? ? Fall directions: maximize horizontal cross section

  32. FALL SPEED: STOKES LAW METHOD Corrections for spheroids from Fuchs, Mechanics of Aerosols (1964) Dynamic shape factor : rate of settling of equivalent mass sphere rate of settling of spheroid particle For oblate spheroids, falling along the polar axis: 4 3 ?1/3 ?2 1 = aspect ratio = (major axis)/ (minor axis) = ? ?2 2 ?2 1 tan 1 ?2 1 + ? For prolate spheroids, falling transverse to the polar axis: 8 3 ? 1/3 ?2 1 = 2?2 3 ?2 1 ?2 1 + ? ln ? +

  33. FALL SPEED: STOKES LAW METHOD Has been used before (Jensen et al., 2008) Only works for low Reynolds numbers, but that should be the case here: ??? ? Estimates: kg m3 Re = ? 1.2? 2= 0.162 (2 scale heights up) ? 10mm = 0.01m (based on updrafts in Dinh et al., 2010) s s ? 100 m = 0.0001 m(conservative estimate for particle size) ? 1.2 10 5kg (viscosity of air at about 180 K) m s Re 0.0135 1

  34. MEAN ICE CRYSTAL MASS

  35. PARTICLE SIZE DISTRIBUTIONS Note: these are earlier simulations that did not consider effects of shape on radiation, and also had a different growth rate calculation.

  36. PARTICLE SIZE DISTRIBUTIONS

  37. PARTICLE SIZE DISTRIBUTIONS Starting Bin

  38. PARTICLE SIZE DISTRIBUTIONS Starting Bin

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