1 / 23

Improvement of Land Surface Parameters and States: Diagnosing Forecast and Model Deficiencies

Improvement of Land Surface Parameters and States: Diagnosing Forecast and Model Deficiencies. Michael Barlage (NCAR) Xubin Zeng (UA), Patrick Broxton ( UA) , Fei Chen (NCAR). 12 th JCSDA Science Meeting – 22 May 2014. Introduction.

yamin
Download Presentation

Improvement of Land Surface Parameters and States: Diagnosing Forecast and Model Deficiencies

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Improvement of Land Surface Parameters and States: Diagnosing Forecast and Model Deficiencies Michael Barlage (NCAR) XubinZeng (UA), Patrick Broxton (UA), Fei Chen (NCAR) 12th JCSDA Science Meeting – 22 May 2014

  2. Introduction Temperature biases in the Noah model can reduce the number of satellite observations that are assimilated In addition, snow melts too quickly and to correct for this, water is added during data assimilation, which results in too much melt This presentation documents deficiencies in the current forecast system and attributes part of them to model structural deficiencies Advances in model structure aim to improve surface temperature and snow simulation, increase atmospheric assimilation, and increase land surface assimilation

  3. Noah LSM Deficiencies Challenges with Noah LSM Structure Flagstaff WRF/Noah v3.2 T2m simulation (green) compared to METAR observations(black) Forecast Hour (Initialized at 12Z daily) • Cold bias during the day results from capped surface temperature at freezing • Bias recovers during the night • When snow is gone, bias is low FEB1 FEB13 FEB20 FEB27 Days in Feb KFLG Forecast Bias (ºC)

  4. Challenges with Noah LSM Structure • May 2007 temperature time series for a single location in Arctic System Reanalysis (3D-Var, land assimilation of vegetation, snow and albedo) • Observations in blue, analysis in red and model forecast in green • Pre-snowmelt period cold bias exists, assimilation helps • Significant cold bias exists during melt period (up to 15°C) • Post-melt period performance is quite good

  5. Challenges with Noah LSM Structure • Simultaneously with low temperature biases, snow continuously gets assimilated during spring • Due to model structure, this snow melts during the 24 hours until the next assimilation cycle • This reinforces the cold bias and inserts more water into the system, potentially causing adverse effects to hydrology prediction NCEP operational NAM model 24-hour forecasted snow minus analysis snow shows excessive melting during the entire month of March

  6. Snow Water Equivalent in GFS • SWE (kg/m^2) (Forecast – Analysis) *White areas: SWE <10 kg/m^2 in forecast and analysis For GFS, compare the forecast with a lead time of 4 days with the coincident analysis for each day in 2013 75 50 25 0 -25 -50 -75

  7. Challenges with Noah LSM Structure Noah LSM in NCEP Eta, MM5 and WRF Models(Pan and Mahrt 1987, Chen et al. 1996, Chen and Dudhia 2001, Ek et al., 2003) Noah-MP LSM in WRF and NCEP CFS (Yang et al., 2011; Niu et al., 2011) Reality Noah Noah-MP Multiple surface temperatures and distinct canopy Tcan(x,y,z) Single surface temperature Tcan Tskin Tsnow(x,y,z) Tsnow(z) Tbc(x,y,z) Tbc Tg Snow (x,y) Tg(x,y) Snow Snow

  8. Noah and Noah-MP LSM Structure Comparison • Six-month simulations using coupled atmosphere-land model from March – June 2010 • Compare only grids with 100% snow cover and evergreen needleleaf trees • When temperatures are below freezing, Noah-MP is warmer but consistent with Noah • When temperature approaches freezing, Noah temperature cannot get much above freezing

  9. Noah and Noah-MP LSM Structure Comparison • Compare to daily MODIS/Aqua land surface temperature at 13:30 overpass • Noah peaks near-freezing • Noah-MP is warmer than MODIS by 2-4K but distribution is much better than Noah

  10. Noah and Noah-MP LSM Structure Comparison Snow Water Equivalent simulated by six LSMs Noah and Noah-MP can produce similar snow through a modified snow albedo formulation Chen, et al. 2014

  11. Noah and Noah-MP LSM Structure Comparison Diurnal cycle of surface albedo: Niwot Ridge Jan, Mar, and Jul 2007 • Large variation among modeled winter albedo • Noah: larger seasonal variations • Noah-MP: drop during March spring melt AmeriFluxObs, MODIS, Noah, VIC, SAST, LEAF, CLM, Noah-MP Chen, et al. 2014 Albedo: 0.66 (Cline, 1997) over snow, 0.34 (MODIS, Jin et al., 2002),

  12. Noah and Noah-MP LSM Structure Comparison Monthly daytime min, max and mean absorbed SW and sensible heat (W/m2) for Jan, Mar, May and Jul O • Comparison of observed (O), Noah (N), and Noah-MP (M). • Noah has less absorbed solar radiation resulting in colder surface and lower (or negative) sensible heat flux 500 M O 400 300 M N 200 N 100 Jan 2007 Mar 2007 M O 300 O M 200 N 100 N 0 -100 Chen, et al. 2014

  13. Advantages with Noah-MP LSM Structure SWdn Noah-MP uses a two-stream radiative transfer treatment through the canopy based on Dickinson (1983) and Sellers (1985) • Canopy parameters: • Canopy top and bottom • Crown radius, vertical and horizontal • Vegetation element density, i.e., trees/grass leaves per unit area • Leaf and stem area per unit area • Leaf orientation • Leaf reflectance and transmittance for direct/diffuse and visible/NIR radiation • Multiple options for spatial distribution • Full grid coverage • Vegetation cover equals prescribed fractional vegetation • Random distribution with slant shading shaded fraction

  14. Advantages with Noah-MP LSM Structure • Over a Noah-MP grid, individual tree elements can be randomly distributed and have overlapping shadows • Noah-MP albedo is calculated based on canopy parameters • Noah prescribes snow-free and snow-covered albedo from satellite climatology SE Minnesota in Google Maps

  15. Advantages with Noah-MP LSM Structure • Using prescribed vegetation fraction varying from 5% to 100% as radiation fraction • Increasing vegetation fraction increases snow, decreases albedo

  16. Advantages with Noah-MP LSM Structure • Using randomly distributed shadows as radiation-active fraction through use of sun angle and canopy morphology • Complex interaction between vegetated and shadowed fraction and canopy/snow radiation absorption

  17. Continue to Develop Satellite Land Datasets MODIS 500m land cover climatology delivered to WRF v3.6 (Broxton et al., 2014) Deciduous Needleleaf Evergreen Needleleaf Deciduous Broadleaf Mixed Forest Closed Shrubland Open Shrubland Woody Savanna Savanna Grassland Permanent Wetland Cropland Urban Cropland/Natural Snow/Ice Barren Not Land Wooded Tundra Mixed Tundra Bare Ground Tundra Deciduous Broadleaf

  18. Continue to Develop Satellite Land Datasets Original Pixel Data Final Smooth Climatology Remove suspect data Fill missing data Smooth Marks -Individual value of year 2001 2002 2003 2004 2005 2006 2007 2008 Lines -black: median -yellow: tile climo (Savanna)

  19. Continue to Develop Satellite Land Datasets • WRF satellite-derived input datasets tend to produce too little vegetation outside of the tropics • Using fraction of photosynthetic absorbed radiation as a vegetation proxy May

  20. Can’t always blame the LSM • Monthly mean WRF radiation June 2010 (Dudhia scheme) • ERA-Interim monthly mean radiation June 2010 • Up to 100 W/m2 difference • 20 – 40% too high

  21. Continue to Develop Satellite Land Datasets D1 D3

  22. Relationship to Land Data Assimilation • Noah model land data assimilation • Favorable to directly assimilate (use) “bulk” land surface properties • Albedo • Green vegetation fraction (via NDVI or EVI) • Leaf Area Index (LAI) • Bulk surface treatment causes problems when heterogeneity is necessary (e.g., snow and vegetation) • Noah-MP model land data assimilation • Increased prognostic states for assimilation • LAI through dynamic vegetation model • Albedo needs to be treated differently (parameter estimation) • Vegetation fraction: what does it mean in the model? • More available states that can inform surface emissivity models • Prognostic LAI, partition of canopy water into ice/liquid • Both models use similar soil moisture treatment for soil moisture assimilation

  23. Conclusions Temperatures: significant biases can occur in the current Noah model, many of these are due to structural limitations when heterogeneities exist at the surface. Snow: In Noah, generally there is too little snow during the spring. Assimilation replaces this snow, it immediately melts and gets added to the soil or surface runoff. Are we reaching a structural limit in the Noah model? Do we need to move toward a more process-based model to capture important states that can informed satellite assimilation? Before the eventual (hopefully) update of the operational LSM, can we exploit the benefits of a more complex model, e.g., in a system such as LIS?

More Related