Skip to main content
Have a personal or library account? Click to login
Comparison of Traditional and Hybrid Forms of Optimal Localisation for Mitigation of Sampling Error in Ensemble Kalman Filters Cover

Comparison of Traditional and Hybrid Forms of Optimal Localisation for Mitigation of Sampling Error in Ensemble Kalman Filters

Open Access
|Apr 2024

Figures & Tables

Table 1

Types of Localisations. Bottom 3 rows show localisation application novel to this paper. Cost functions are given in terms of the parameter θ which represents the parameters of the distribution.

LOCALISATIONCOST FUNCTIONFORMBASED ON
GaussianNAexpdij22 γ2
Damps sample covariance towards 0.
Tuned width parameter γ. The distance between 2 points dij.
Optimal for a single covariance (OSTC)(α b^b)2P(b^|θ)db^α=bij2bij2+σbij^2
Damps sample sparse gain towards 0.
Signal: (mean) sparse gain.
Noise: mean variance in sample sparse gain.
Optimal for a variable covariance (OVTC)P(θ)(α b^b)2P(b^|θ)db^dθα=b¯2+σb2b¯2+σb2+σb^2
Damps sample sparse gain towards 0.
Signal: mean and variance in sparse gain.
Noise: mean variance in sample sparse gain.
hybrid Optimal for a variable covariance (HOVTC)P(θ)(b¯+α(b^b¯)b)2P(b^|θ)db^dθα=σb2σb2+σb^2
Damps sample sparse gain towards mean sparse gain.
Signal: variance in sparse gain.
Noise: mean variance in sample sparse gain.
hybrid tuned double Gaussian (HTDG)NAexpdij22 γ12expdij22 γ22
Damps sample covariance towards mean covariance.
Tuned width parameters γ1 and γ2. The distance between 2 points dij.
Figure 1

Schematic of a single DA process using the EnKF.

Figure 2

Schematic showing the ensemble and observation generation, assimilation and error production for a single DA cycle.

Figure 3

The flow diagram of the experiments performed and reported in this paper.

Figure 4

Plot showing the shape of each localisation and the statistics used to compute the localisation for Scenario 1. The form of the localisations is shown for observation variance 0.1, 1.0 and 10.0. The shown tuned widths are tuned from assimilating a single observation.

Figure 5

Plot showing the shape of each localisation and the statistics used to compute the localisation for Scenario 2. The form of the localisations is shown for observation variance 0.1,1.0 and 10.0. The shown tuned widths are tuned from assimilating a single observation.

Table 2

RMS error results for Scenario 1.

SCENARIO 1 OBSERVATION ERROR VARIANCE 0.1
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob0.86330.86560.86470.86560.86340.86310.86330.85220.85570.85760.85581.0466
Spacing 330.53680.55250.53760.53660.55230.54020.53750.58042.418614.78180.52331.0462
Spacing 90.24400.28520.24680.42890.28550.26130.24491.8869212.249538.6260.25731.0461
SCENARIO 1 OBSERVATION ERROR VARIANCE 1.0
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob0.94800.95020.95230.94980.94900.95060.94870.93980.94100.94110.94171.0466
Spacing 330.78480.79470.79110.78600.79270.79010.78540.76980.76680.76820.76691.0462
Spacing 90.56330.58860.57010.56410.58700.57090.56421.14600.59314.64810.54931.0461
SCENARIO 1 OBSERVATION ERROR VARIANCE 10.0
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob1.02771.02831.02851.02831.02801.02821.02801.02521.02531.02531.02531.0466
Spacing 330.99770.99920.99930.99880.99850.99870.99820.99030.99060.99060.99111.0462
Spacing 90.91520.92200.91970.91840.92030.91840.91730.90310.89890.89890.89921.0461
Table 3

RMS error results for Scenario 2.

SCENARIO 2 OBSERVATION ERROR VARIANCE 0.1
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob0.83110.82960.82950.82950.82950.82950.82940.80680.80680.80680.80701.0469
Spacing 330.37010.38580.37630.37450.38560.37580.37390.58560.34950.34600.34591.0464
Spacing 90.19950.2175152.6382136.75480.217416.2293109.3813.49720.19470.19470.19401.0463
SCENARIO 2 OBSERVATION ERROR VARIANCE 1.0
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob0.93240.93290.93500.93260.93290.23490.93260.91610.91610.91610.91611.0469
Spacing 330.72790.73700.73520.72890.73700.73520.72880.72150.69710.69710.69711.0464
Spacing 90.50890.52800.51730.51190.52800.51700.51131.82820.48460.48460.48471.0463
SCENARIO 2 OBSERVATION ERROR VARIANCE 10.0
OSTCOVTCHOVTC
GAUSSIAN(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)(SG;G)(C;C)(SG;C)HTDGBACKGROUND ERROR
Single ob1.02531.02520.02541.02521.02521.02541.02521.02071.02071.02071.02071.0469
Spacing 330.98970.99040.99070.99020.99040.99070.99010.97800.97820.97820.97821.0464
Spacing 90.89410.89980.89820.89690.89970.89820.89680.88820.87060.87060.87071.0463
Figure 6

RMS errors resulting from DA with each kind of localisation in Gaussian Scenario 1. Columns show results for a range of observation spacing and rows show a range of observation error variance.

Figure 7

RMS errors resulting from DA with each kind of localisation in Gaussian Scenario 2. Columns show results for a range of observation spacing and rows show a range of observation error variance.

DOI: https://doi.org/10.16993/tellusa.35 | Journal eISSN: 3035-9554
Language: English
Page range: 57 - 73
Submitted on: Feb 17, 2022
Accepted on: Mar 19, 2024
Published on: Apr 29, 2024
Published by: Stockholm University Press
In partnership with: Paradigm Publishing Services

© 2024 Rebecca Susanne Atkinson, Jonathan Flowerdew, Sue Hughes, Ian Roulstone, published by Stockholm University Press
This work is licensed under the Creative Commons Attribution 4.0 License.