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Sea ice 2

Lecture, exercises and practical by Jun.-Prof. Dr. Lars Kaleschke

Monday 13:30-15:00
Room ZMAW 022

Description of the course

The lecture will cover the thermodynamic coupling between the sea ice, the ocean, and the atmosphere. It is designed for master-level students with moderate knowledge in numerics, scientific programming, and sea ice physics. A conceptual model of the Arctic will be derived and simulation results will be analysed. For didactical reasons the model will be developed from scratch and kept as simple as possible, but complex enough to learn about the basic principles of the thermodynamic interaction between the ocean, the ice and the atmosphere for climatic, oceanographic and meteorological studies.

Acknowledgments

This lecture is based on content taken from a lecture Sea ice modeling by Aike Beckmann (Univ. Hamburg, Summer 2009) and a short course on Ice-Ocean Modeling and Data Assimilation which was conducted by Frank Kauker and Michael Karcher (Univ. Bremen, 6-7 December 2006).

Project work: source code, results

/Gruppe1 /Gruppe2 /Gruppe3 /Gruppe4 /Gruppe5

Lesson 1 - Ocean mixed layer and radiative forcing without sea ice and atmosphere

Scenario 1

Ocean mixed layer forced by shortwave radiation only
No atmosphere
No exchange with deeper ocean layers, immediate mixing
Heat balance at the sea surface: Short wave incoming radiation + long wave outgoing radiation
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Numerics: forward-in-time integration, finite differences

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Research questions

Compute the time evolution of the ocean mixed layer temperature T_ml(t) for different h_ml, initial temperatures T_ml(t=0), and short wave insolation Q_SW.

Estimate the typical time scale for stationarity and select appropriate time step delta_t for model integration.

Change insolation after the model has reached stationarity.

Lesson 2: Incoming shortwave radiation

Top of the atmosphere

A rough approximation for the flux of solar irradiance at the top of the atmosphere (TOA) can be derived from geometric considerations

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with the solar constant S=1360 W/m², the solar zenith angle Z. The cosine of the zenith angle is given by

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where

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are latitude, declination, and hour angle, respectively. The declination and hour angle are calculated as

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Research questions

Calculate and plot the diurnal cycle of solar irradiance for the latitude of Hamburg on April 19.
Calculate and plot the daily averaged solar irradiance for three latitudes (0, 50, 90) as a function of time
Calculate and plot the zonal averaged solar irradiance for different months (e.g. January and July)
Compare with the calculated irradiance with CERES measurements
Calculate and plot the oceanic mixed layer temperature (h_ml=30m, T(0)=10^° C) forced with the solar irradiance (lat=30^°). Integration time shall be 3000 days. Explain the relation of temperature and irradiance.
Change the time step to one hour and calculate the diurnal cycle of the oceanic mixed layer temperature. Vary the mixed layer depth and latitude.

Validation

Radiative flux measurements are available from the Clouds and the Earth s Radiant Energy System (CERES) sensor. Climatology products from the NASA Langley Research Center Atmospheric Science Data Center can be used to validate flux parameterizations. The CERES-Terra 5-year TOA global product has an easy to use browse interface.

Lesson 3: Energy fluxes at the ocean surface

In this lesson we look at the energy fluxes at the ocean surface in polar latitudes. We will analyse the importance (magnitudes) of the different fluxes.

Scenario 3

Ocean surface kept constant at the freezing point
Prescribed atmospheric temperature
Energy fluxes based on empirical formulations given in Parkinson and Washington (1979)
Energy fluxes at the sea surface: Incoming short wave radiation + incoming and outgoing long wave radiation + sensible heat fluxes
Zonal average 60N-90N

Research questions

Calculate and plot the daily and zonally averaged solar irradiance as a function of time (day of the year)
Modify the irradiance by a cloud factor [Laevastu, 1960].
Calculate the incoming longwave radiation with Idso and Jackson's (1969) formula.
Calculate the sensible heat flux as a function of typical temperature differences and wind speed

Literature

References for download

Maykut, G.A. & N. Untersteiner, 1971: Some results from a time-dependent thermodynamic model of sea ice. J. Geophys. Res.,76, 1550-1575.

Semtner, A., 1976: A model for the thermodynamic growth of sea ice in numerical investigations of climate, J. Phys. Oceanogr, 6, 379-389.

Hibler III, W.D., 1979: A dynamic-thermodynamic sea ice model. J. Phys. Oceanogr., 9, 815-846.

Parkinson, C.L. & W.M. Washington, 1979: A large-scale numerical model of sea ice., J. Geophys. Res., 84, 311-337.

Sellers, W.D., 1969: A Global Climatic Model Based on the Energy Balance of the Earth-Atmosphere System, J. Appl. Met., 8(3), 392-400.

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+Lecture, exercises and practical by  [[LarsKaleschke|Jun.-Prof. Dr. Lars Kaleschke]]
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-Lecture, exercises and practical by  [[LarsKaleschke| Jun.-Prof. Dr. Lars Kaleschke]]

 * Monday 13:30-15:00
+ * Monday 13:30-15:00
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 The lecture will cover the thermodynamic coupling between the sea ice, the ocean, and the atmosphere. It is designed for master-level students with moderate knowledge in numerics, scientific programming, and sea ice physics. A conceptual model of the Arctic will be derived and simulation results will be analysed. For didactical reasons the model will be developed from scratch and kept as simple as possible, but complex enough to learn about the basic principles of the thermodynamic interaction between the ocean, the ice and the atmosphere for climatic, oceanographic and meteorological studies.
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 This lecture is based on content taken from a lecture ''Sea ice modeling'' by Aike Beckmann (Univ. Hamburg, Summer 2009) and a short course on ''Ice-Ocean Modeling and Data Assimilation'' which was conducted by Frank Kauker and Michael Karcher (Univ. Bremen, 6-7 December 2006).
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- * No atmosphere  
 * No exchange with deeper ocean layers, immediate mixing 
 * Heat balance at the sea surface: Short wave incoming radiation + long wave outgoing radiation {{{#!latex 
   $ Q_{SW}^{\downarrow}  + Q_{LW}^{\uparrow} = Q_{srf} $    }}}
+ * No atmosphere
 * No exchange with deeper ocean layers, immediate mixing
 * Heat balance at the sea surface: Short wave incoming radiation + long wave outgoing radiation
 {{{#!latex
   $ Q_{SW}^{\downarrow}  + Q_{LW}^{\uparrow} = Q_{srf} $
}}}
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- * {{{#!latex 
   $\frac{\partial T_{ml}}{\partial t}\rho_w c_w h_{ml}=Q_{srf}$ 
   }}}
+ * {{{#!latex
   $\frac{\partial T_{ml}}{\partial t}\rho_w c_w h_{ml}=Q_{srf}$
}}}
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-= Lesson 2: Radiative fluxes =
+= Lesson 2: Incoming shortwave radiation =
== Top of the atmosphere ==
A rough approximation for the flux of solar irradiance at the top of the atmosphere (TOA) can be derived from geometric considerations
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-== Top of the atmosphere ==

A rough approximation for the flux of solar irradiance at the top of the atmosphere (TOA) can be derived from geometric considerations
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-where {{{#!latex 
 $\phi, \delta, HA, $ }}} are latitude, declination, and [[http://en.wikipedia.org/wiki/Hour_angle|hour angle]], respectively. The declination and hour angle are calculated as
+where

{{{#!latex
 $\phi, \delta, HA, $
}}}
are latitude, declination, and [[http://en.wikipedia.org/wiki/Hour_angle|hour angle]], respectively. The declination and hour angle are calculated as
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-Radiative flux measurements are available from the [[http://science.larc.nasa.gov/ceres/index.html| Clouds and the Earth s Radiant Energy System (CERES) sensor]]. Climatology products from the NASA Langley Research Center Atmospheric Science Data Center can be used to validate flux parameterizations. The [[http://lposun.larc.nasa.gov/cgi-bin/cgiwrap/ceresdm/browse/browse.pl|CERES-Terra 5-year TOA global product]] has an easy to use browse interface.
+Radiative flux measurements are available from the [[http://science.larc.nasa.gov/ceres/index.html|Clouds and the Earth s Radiant Energy System (CERES) sensor]]. Climatology products from the NASA Langley Research Center Atmospheric Science Data Center can be used to validate flux parameterizations. The [[http://lposun.larc.nasa.gov/cgi-bin/cgiwrap/ceresdm/browse/browse.pl|CERES-Terra 5-year TOA global product]] has an easy to use browse interface.
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+= Lesson 3: Energy fluxes at the ocean surface =
In this lesson we look at the energy fluxes at the ocean surface in polar latitudes. We will analyse the importance (magnitudes) of the different fluxes.
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+== Scenario 3 ==
 * Ocean surface kept constant at the freezing point
 * Prescribed atmospheric temperature
 * Energy fluxes based on empirical formulations given in Parkinson and Washington (1979)
 * Energy fluxes at the sea surface: Incoming short wave  radiation + incoming and outgoing long wave radiation + sensible  heat fluxes
 * Zonal average 60N-90N

== Research questions ==
 * Calculate and plot the daily and zonally averaged solar irradiance as a function of time (day of the year)
 * Modify the irradiance by a cloud factor [Laevastu, 1960].
 * Calculate the incoming longwave radiation with Idso and Jackson's (1969) formula.
 * Calculate the sensible heat flux as a function of typical temperature differences and wind speed
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+Line 94:
-[[/Lesson1|References for download]]
+[[SeaIce2/Lesson1|References for download]]