NCAR · climbfuji · Mar 22, 2019 · Mar 22, 2019
diff --git a/physics/docs/img/GFS_gwdc.eps b/physics/docs/img/GFS_gwdc.eps
diff --git a/physics/docs/img/GFS_sice_wonton2000_fig1.eps b/physics/docs/img/GFS_sice_wonton2000_fig1.eps
diff --git a/physics/docs/img/NSST.eps b/physics/docs/img/NSST.eps
diff --git a/physics/docs/img/Noah_LA_interaction.eps b/physics/docs/img/Noah_LA_interaction.eps
diff --git a/physics/docs/img/gfdl_cloud_mp_diagram.eps b/physics/docs/img/gfdl_cloud_mp_diagram.eps
diff --git a/physics/docs/img/land_dataset.eps b/physics/docs/img/land_dataset.eps
diff --git a/physics/docs/img/precpd-micop.eps b/physics/docs/img/precpd-micop.eps
diff --git a/physics/docs/img/roughness_length_fig1.eps b/physics/docs/img/roughness_length_fig1.eps
diff --git a/physics/docs/img/roughness_length_fig2.eps b/physics/docs/img/roughness_length_fig2.eps
diff --git a/physics/docs/img/schematic_Rad_mod.eps b/physics/docs/img/schematic_Rad_mod.eps
diff --git a/physics/docs/img/schematic_sice.eps b/physics/docs/img/schematic_sice.eps
diff --git a/physics/docs/pdftxt/GFDL_cloud.txt b/physics/docs/pdftxt/GFDL_cloud.txt
@@ -9,7 +9,6 @@ Krueger et al.(1995) \cite krueger_et_al_1995, Chen and Lin (2011) \cite chen_an
 Physics processes of GFDL cloud MP are described in Figure 1 (also see warm_rain() and icloud()) and are feature with time-split between warm-rain (faster) and ice-phase (slower) processes (see 'conversion time scale' in gfdl_cloud_microphys.F90 for default values). 
 
 \image  html  gfdl_cloud_mp_diagram.png "Figure 1: GFDL MP at a glance (Courtesy of S.J. Lin at GFDL)" width=10cm
-\image  latex  gfdl_cloud_mp_diagram.eps "Figure 1: GFDL MP at a glance (Courtesy of S.J. Lin at GFDL)" width=10cm
 
 Some unique attributes of GFDL cloud microphysics include:
 

diff --git a/physics/docs/pdftxt/GFS_GWDC.txt b/physics/docs/pdftxt/GFS_GWDC.txt
@@ -30,7 +30,6 @@
  the large-scale flow.
 
  \image html  GFS_gwdc.png "Figure 1: Gravity waves generated by penetrative convection in the presence of background wind. (Based on Hooke(1986); and Kim et al. (2003))" width=10cm
- \image latex  GFS_gwdc.eps "Gravity waves generated by penetrative convection in the presence of background wind. (Based on Hooke(1986); and Kim et al. (2003))" width=10cm
 
  Compared with orographic gravitity waves, it has proven more difficult to model the way in which
  gravity waves are generated by various convective sources; The simplest situation is depicted in 

diff --git a/physics/docs/pdftxt/GFS_NOAH.txt b/physics/docs/pdftxt/GFS_NOAH.txt
@@ -27,7 +27,6 @@
  gay-dotted line (no arrows) indicates the top of the PBL, and the seven
  small vertical dashed lines (no arrows) represent precipitation
  \image html Noah_LA_interaction.png "Figure 1: Local Land-atmosphere Interaction (courtesy of Michael Ek, Ek and Mahrt (1994), Ek and Holtslag (2004))" width=10cm
- \image latex Noah_LA_interaction.eps "Local Land-atmosphere Interaction (courtesy of Michael Ek, Ek and Mahrt (1994), Ek and Holtslag (2004))" width=10cm
 Recently, the land surface updates in 2017 GFS operational physics includes:
  - IGBP 20-type 1-km land classification
  - STASGO 19-type 1-km soil classification
@@ -38,7 +37,6 @@ Recently, the land surface updates in 2017 GFS operational physics includes:
  - Increase ground heat flux under deep snow
  - Upgrade surface layer parameterization scheme \ref GFS_SFCLYR to modify the roughness-length formulation and introduce a stability parameter constraint in the Monin-Obukhov similarity theory to prevent the land-atmosphere system from fully decoupling leading to excessive cooling of 2m temperature during sunset
  \image html land_dataset.png "Figure 2: Land Data Sets Used in NCEP Modeling Systems" width=10cm
- \image latex land_dataset.eps "Land Data Sets Used in NCEP Modeling Systems" width=10cm
 
 \section intra_noah Intraphysics Communication
  +  GFS Noah LSM Driver (\ref arg_table_lsm_noah_run)

diff --git a/physics/docs/pdftxt/GFS_RRTMG.txt b/physics/docs/pdftxt/GFS_RRTMG.txt
@@ -11,7 +11,6 @@
 
  The schematic radiation module structure is shown in Figure 1.
  \image html schematic_Rad_mod.png "Figure 1: Schematic Radiation Module Structure" width=10cm
- \image latex schematic_Rad_mod.eps "Schematic Radiation Module Structure" width=10cm
 
  GFS radiation package is intended to provide a fast and accurate
  method of determining the total radiative flux at any given

diff --git a/physics/docs/pdftxt/GFS_ZHAOC.txt b/physics/docs/pdftxt/GFS_ZHAOC.txt
@@ -18,7 +18,6 @@
  prognostically produced, enabling this scheme to predict precipitation type.
 
  \image  html  GFS_zhaocarr_schematic.png "Figure 1: Schematic illustration of the precipitation scheme" width=10cm
- \image  latex  GFS_zhaocarr_schematic.eps "Schematic illustration of the precipitation scheme" width=10cm
 
  The parameterization of precipitation is required in order to remove
  water from the atmosphere and transport it to the ground.
@@ -30,7 +29,6 @@
  + Melting of snow to form rain below the freezing level (\f$P_{sm1}\f$, \f$P_{sm2}\f$)
  + Evaporation of precipitation (\f$E_{rr}\f$, \f$E_{rs}\f$)
 \image html precpd-micop.png "Figure 2: Microphysical processes simulated in the precipitation scheme " width=10cm
-\image latex precpd-micop.eps "Microphysical processes simulated in the precipitation scheme " width=10cm
  Some processes, such as the freezing of raindrops and the interaction between rain drops and cloud ice, have been ignored
  since the upward motion on the synoptic scale is too weak to advect the raindrops upward. Additionally, precipitation is
  diagnostically calculated directly from the cloud mixing ratio.