| 1 | # $Id: $
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| 2 |
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| 3 | #****c* Configuration Files/romsaf_invert.cf *
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| 4 | #
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| 5 | # NAME
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| 6 | # romsaf_invert.cf - ROM SAF inversion default parameter settings
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| 7 | #
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| 8 | # SYNOPSIS
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| 9 | # <pp_program> ... -c romsaf_invert.cf ...
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| 10 | #
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| 11 | # DESCRIPTION
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| 12 | # This file reflects the configuration for the PP
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| 13 | # implementations within ROPP consistent with ROM SAF inversion data.
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| 14 | #
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| 15 | # NOTES
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| 16 | #
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| 17 | # AUTHOR
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| 18 | # Met Office, Exeter, UK.
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| 19 | # Any comments on this software should be given via the ROM SAF
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| 20 | # Helpdesk at http://www.romsaf.org
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| 21 | #
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| 22 | # COPYRIGHT
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| 23 | # (c) EUMETSAT. All rights reserved.
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| 24 | # For further details please refer to the file COPYRIGHT
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| 25 | # which you should have received as part of this distribution.
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| 26 | #
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| 27 | #****
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| 28 |
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| 29 | #-------------------------------------------------------------------------------
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| 30 | # 0. Output options
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| 31 | #-------------------------------------------------------------------------------
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| 32 | output_tdry = .true. ! Flag to output dry temperature
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| 33 |
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| 34 | output_diag = .false. ! Flag to output additional diagnostics
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| 35 |
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| 36 | #-------------------------------------------------------------------------------
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| 37 | # 1. Excess phase to bending angle processing
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| 38 | #-------------------------------------------------------------------------------
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| 39 |
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| 40 | # 1.1 Occultation processing method
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| 41 | # ---------------------------------
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| 42 |
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| 43 | # GO - use GEOMETRIC OPTICS processing to derive bending angle as a function of
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| 44 | # impact parameter from excess phase as a function of time.
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| 45 | # WO - use WAVE OPTICS (CT2 algorithm) processing to derive bending angle as a
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| 46 | # function of impact parameter from excess phase as a function of time.
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| 47 |
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| 48 | occ_method = WO
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| 49 |
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| 50 | # 1.2 Filtering method
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| 51 | # --------------------
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| 52 |
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| 53 | # optest - use OPTIMAL ESTIMATION: solution of integral equation
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| 54 | # slpoly - use SLIDING POLYNOMIAL
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| 55 |
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| 56 | filter_method = optest
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| 57 |
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| 58 | # 1.3 Smoothing bending angle profile
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| 59 | # -----------------------------------
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| 60 |
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| 61 |
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| 62 | fw_go_smooth = 3000.0 # Filter width for smoothed GO bending angles (m)
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| 63 |
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| 64 | fw_go_full = 3000.0 # Filter width for full resolution GO bending angles (m)
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| 65 |
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| 66 | fw_wo = 2000.0 # Filter width for wave optics bending angle above 7 km(m)
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| 67 |
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| 68 | fw_low = -1000.0 # Filter width for wave optics bending angle below 7 km (m)
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| 69 |
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| 70 | # 1.4 Maximum height for wave optics processing
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| 71 | # ---------------------------------------------
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| 72 |
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| 73 | hmax_wo = 25000.0 # Maximum height for wave optics processing (m)
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| 74 |
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| 75 | # 1.5 Data cut-off limits
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| 76 | # -----------------------
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| 77 |
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| 78 | Acut = 0.0 # Fractional cut-off limit for amplitude
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| 79 |
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| 80 | Pcut = 0.0 # Cut-off limit for impact height
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| 81 |
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| 82 | Bcut = 0.2 # Cut-off limit for bending angle
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| 83 |
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| 84 | Hcut = -999000.0 # Cut-off limit for straight-line tangent altitude
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| 85 |
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| 86 | # 1.6 CT2 options
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| 87 | # ---------------
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| 88 |
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| 89 | CFF = 2 # Complex field filter flag (CFF = 'P')
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| 90 |
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| 91 | dsh = 100.0 # Shadow border width (m)
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| 92 |
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| 93 | # 1.7 Degraded L2 data flag
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| 94 | # -------------------------
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| 95 |
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| 96 | opt_DL2 = .true.
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| 97 |
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| 98 | # 1.8 Compute and output spectra flag
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| 99 | # -----------------------------------
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| 100 |
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| 101 | opt_spectra = .false.
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| 102 |
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| 103 | # 1.9 Paths to EGM96 geoid model coefficients and corrections file
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| 104 | # ----------------------------------------------------------------
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| 105 |
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| 106 | egm96 = ../data/egm96.dat # EGM96 coefficients file
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| 107 |
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| 108 | corr_egm96 = ../data/corrcoef.dat # Correction coefficients file
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| 109 |
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| 110 | #-------------------------------------------------------------------------------
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| 111 | # 1. Ionospheric correction processing
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| 112 | #-------------------------------------------------------------------------------
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| 113 |
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| 114 | # 1.1 Ionospheric correction method
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| 115 | # ---------------------------------
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| 116 |
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| 117 | # GMSIS - use MSIS climatology bending angle (searching global MSIS profiles
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| 118 | # for best fit profile to obs) in ionospheric correction,
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| 119 | # statistical optimization and bending angle to refractivity inversion.
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| 120 | #
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| 121 | # MSIS - use MSIS climatology bending angle in ionospheric correction,
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| 122 | # statistical optimization and bending angle to refractivity inversion.
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| 123 | #
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| 124 | # GBARO - use BAROCLIM bending angle (searching global BAROCLIM profiles
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| 125 | # for best fit profile to obs) in ionospheric correction,
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| 126 | # statistical optimization and bending angle to refractivity inversion.
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| 127 | #
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| 128 | # BARO - use BAROCLIM bending angle in ionospheric correction,
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| 129 | # statistical optimization and bending angle to refractivity inversion.
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| 130 | #
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| 131 | # BG - use climatology from a specified input file containing
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| 132 | # background temperature, pressure and humidity
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| 133 | # (e.g. from an NWP analysis). The input filename can be specified
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| 134 | # using the '-bfile' command line argument or setting 'bfile' (see 1.5).
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| 135 | #
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| 136 | # NONE - linear combination of L1 and L2 bending angles in ionospheric
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| 137 | # correction, no additional information above observed profile top
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| 138 | # in the inverse Abel to compute refractivity.
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| 139 |
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| 140 | method = GBARO # Ionospheric correction method
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| 141 |
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| 142 | # 1.2 Abel integral method
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| 143 | # ------------------------
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| 144 |
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| 145 | # LIN - assume linear variation of bending angle and ln(n) between
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| 146 | # observation levels. This algorithm is used in ROM SAF NRT processing
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| 147 | #
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| 148 | # EXP - assume exponential variation of bending angle and ln(n) between
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| 149 | # observation levels. This algorithm is used in ropp_fm module.
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| 150 |
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| 151 | abel = LIN
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| 152 |
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| 153 | # 1.3 Statistical optimisation method
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| 154 | # -----------------------------------
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| 155 |
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| 156 | # SO - statistical optimisation.
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| 157 | # LCSO - linear combination plus statistical optimisation.
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| 158 |
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| 159 | so_method = so
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| 160 |
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| 161 | # 1.4 Climatology model coefficients files
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| 162 | # --------------------------------
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| 163 |
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| 164 | msisfile = MSIS_coeff.nc # MSIS model coefficients file
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| 165 | mfile = BAROCLIM_coeff.nc # Model coefficients file for stat.opt.
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| 166 |
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| 167 | # 1.5 Background model temperature, humidity, pressure file
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| 168 | # ---------------------------------------------------------
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| 169 |
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| 170 | bfile = BG_file.nc # Background meteorology profile file (method=BG)
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| 171 |
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| 172 | #-------------------------------------------------------------------------------
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| 173 | # 2. Impact parameter grid
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| 174 | #-------------------------------------------------------------------------------
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| 175 |
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| 176 | # The ionospheric correction interpolates L1 and L2 bending angle profiles onto a
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| 177 | # standard grid.
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| 178 |
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| 179 | dpi = 100.0 # Step of standard impact parameter grid (m)
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| 180 |
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| 181 | #-------------------------------------------------------------------------------
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| 182 | # 3. Smoothing bending angle profile
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| 183 | #-------------------------------------------------------------------------------
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| 184 |
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| 185 | # A smoothed bending angle profile is derived compute the fit of observed bending
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| 186 | # angles to the model bending angle profile.
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| 187 |
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| 188 | np_smooth = 3 # Polynomial degree for smoothing regression
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| 189 |
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| 190 | fw_smooth = 1000.0 # Filter width for smoothing profile
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| 191 |
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| 192 | #-------------------------------------------------------------------------------
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| 193 | # 4. Model bending angle profile fit to observations
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| 194 | #-------------------------------------------------------------------------------
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| 195 |
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| 196 | # To avoid systematic deviations from the observed profile with climatology,
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| 197 | # the model profile is scaled to the observed profile by a fitting method.
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| 198 |
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| 199 | sf_method = regular # Search and fit method (convoluted or regular)
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| 200 |
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| 201 | nparm_fit = 2 # Number of parameters for model fit regression
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| 202 |
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| 203 | hmin_fit = 40000.0 # Lower limit for model fit regression
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| 204 |
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| 205 | hmax_fit = 60000.0 # Upper limit for model fit regression
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| 206 |
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| 207 | omega_fit = 0.3 # A priori standard deviation of regression factor
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| 208 |
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| 209 | #-------------------------------------------------------------------------------
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| 210 | # 5. Ionospheric correction and statistical optimization
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| 211 | #-------------------------------------------------------------------------------
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| 212 |
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| 213 | # The method described by Gorbunov (2002) is implemented to perform ionospheric
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| 214 | # correction with statistical optimization.
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| 215 |
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| 216 | f_width = 250.0 # Ionospheric correction filter width
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| 217 |
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| 218 | delta_p = 100.0 # Step of homogeneous impact parameter grid
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| 219 |
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| 220 | s_smooth = 2000.0 # External ionospheric smoothing scale
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| 221 |
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| 222 | z_ion = 50000.0 # Lower height limit of ionospheric signal
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| 223 |
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| 224 | z_str = 35000.0 # Lower height limit of stratospheric signal
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| 225 |
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| 226 | z_ltr = 12000.0 # Lower height limit of tropospheric signal
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| 227 |
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| 228 | n_smooth = 11 # Number of points for smoothing (must be odd)
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| 229 |
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| 230 | model_err = -0.5 # A priori model error std.dev. (dyn.est. if negative)
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| 231 |
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| 232 | #-------------------------------------------------------------------------------
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| 233 | # 6. Bending angle inversion to refractivity
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| 234 | #-------------------------------------------------------------------------------
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| 235 |
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| 236 | # The Abel inversion is computed to retrieve refractivity from corrected
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| 237 | # bending angles. The corrected bending angle profile is extended
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| 238 | # using MSIS or BAROCLIM data above the observed profile top.
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| 239 |
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| 240 | ztop_invert = 150000.0 # Height of atmosphere top for inversion
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| 241 |
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| 242 | dzh_invert = 50.0 # Step of inversion grid above observation top
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| 243 |
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| 244 | dzr_invert = 20000.0 # Interval for regression in inversion
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| 245 |
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