File:Gassendi crater rendering 1 1.png

   LOLA Team and Kaguya Team 

Originators

   Planetary Data System 

Publisher

   USGS Astrogeology Science Center 

Publication Date

   2015-02-04

References:

Barker, M. K., Mazarico, E., Neumann, G. A., Zuber, M. T., Haruyama, J., & Smith, D. E. (2016). A new lunar digital elevation model from the Lunar Orbiter Laser Altimeter and SELENE Terrain Camera. Icarus, 273, 346–355. https://doi.org/10.1016/j.icarus.2015.07.039Earth Planets Space, 60, 243-255. https://doi.org/10.1186/BF03352788

Kato, M., Takizawa, Y., Sasaki, S., & SELENE Project Team (2006). The SELENE Mission: Present status and science goals. Paper presented at the 38th Lunar and Planetary Science Conference, Lunar and Planetary Institute, Houston, TX. https://www.lpi.usra.edu/meetings/lpsc2007/pdf/1211.pdf

Matsunaga, T., Ohtake, M., Haruyama, J., Ogawa, Y., Nakamura, R., Yokota, Y., Morota, T., et al. (2008). Discoveries on the lithology of lunar crater central peaks by SELENE Spectral Profiler. Geophysical Research Letters, 35(L23201). https://doi.org/10.1029/2008GL035868

Mazarico, E., Rowlands, D. D., Neumann, G. A., Smith, D. E., Torrence, M. H., Lemoine, F. G., & Zuber, M. T. (2012). Orbit determination of the Lunar Reconnaissance Orbiter. Journal of Geodesy, 86(3), 193-207. https://doi.org/10.1007/s00190-011-0509-4

Ohtake, M., Haruyama, J., Matsunaga, T., Yokota, Y., Morota, T., Honda, C., & LISM Team (2008). Performance and scientific objectives of the SELENE (KAGUYA) Multiband Imager. Earth Planets Space, 60, 257-264. https://doi.org/10.1186/BF03352789

Petro, N. E., Keller, J. W., Cohen, B. A., & McClanahan, T. P. (2019). Ten years of the Lunar Reconnaissance Orbiter: Advancing lunar science and context for future lunar exploration. Paper presented at the 50th Lunar and Planetary Science Conference, Lunar and Planetary Institute, Houston, TX. https://www.hou.usra.edu/meetings/lpsc2019/pdf/2780.pdf

Tooley, C. R., Houghton, M. B., Saylor Jr., S. S., Peddie, C., Everett, D. F., Baker, C. L., & Safdie, K. N. (2010). Lunar Reconnaissance Orbiter mission and spacecraft design. Space Science Reviews, 150(1), 23–62. https://doi.org/10.1007/s11214-009-9624-4

https://astrogeology.usgs.gov/search/map/moon_lro_lola_selene_kaguya_tc_dem_merge_60n60s_59m

1. /usr/bin/gmt

1. gdalwarp -te -45 -21 -35 -12 ../../alunardata1/Lunar_LRO_LOLAKaguya_DEMmerge_60N60S_512ppd2.tif dem1.tif
2. gdalwarp -te -45 -21 -35 -12 ../../alunardata1/Lunar_LRO_LROC-WAC_Mosaic_global_100m_June20132.tif mosaic1.tif
3. gdalwarp -te -45 -21 -35 -12 ../../alunardata1/Lunar_LRO_LOLAKaguya_Shade_60N60S_512ppd2.tif shade1.tif

1. gdal_translate dem1.tif dem1.nc

1. 1. test
2. gmt makecpt -Chaxby -T-10000/10000/1 -Z > palette1.cpt

1. gmt grdimage dem1.nc -Cpalette1.cpt -JX10c -R-45/-35/-21/-12 -B2 -pdf

1. exit(-1)

1. gmt grdgradient dem1.nc -Ghillshade-grad.nc -A270 -Ne0.6 -V
2. gmt grdhisteq hillshade-grad.nc -Ghillshade-hist.nc -N -V
3. gmt grdmath hillshade-hist.nc 5 DIV = hillshade-int.nc

1. gmt grdgradient dem1.nc -Ghillshade-grad2.nc -A90 -Ne0.6 -V
2. gmt grdhisteq hillshade-grad2.nc -Ghillshade-hist2.nc -N -V
3. gmt grdmath hillshade-hist2.nc 5 DIV = hillshade-int2.nc

1. gdal_translate mosaic1.tif mosaic1.nc
2. gdal_translate shade1.tif shade1.nc

1. cdo remapbil,dem1.nc mosaic1.nc mosaic1s.nc
2. cdo remapbil,dem1.nc shade1.nc shade1s.nc

1. gdaldem dem1.tif hillshade1.tif -az 90 -alt 15
2. gdaldem hillshade dem1.tif hillshade1.tif -of GTiff -b 1 -z 1.0 -s 1.0 -az 90.0 -alt 45.0
3. gdal_translate hillshade1.tif hillshade1.nc

1. exit(-1)

gmt makecpt -Cgray -T-100000/100000/1 -Z > palette1.cpt

1. gmt makecpt -Cbilbao -T-500/500/1 -Z > palette3.cpt

gmt makecpt -Chaxby -T-1000/1000/10 -Z > palette2.cpt

1. gmt makecpt -Ccopper -T-8000/3000/10 > palette2.cpt
2. gmt makecpt -Cbilbao -T-8000/3000/10 > palette2.cpt

gmt begin out png -C

1. gmt grdimage dem1.tif -Ihillshade-grad2.nc -Cpalette1.cpt -JX10c -R-45/-35/-21/-13 -B1

gmt grdimage dem1.tif -Ihillshade-grad2.nc -Cwysiwyg -JX10c -R-45/-35/-21/-13 -B1

1. gmt grdimage dem1.nc -Ishade1s.nc -Chaxby -JX10c -R-45/-35/-21/-13 -B1

1. gmt grdimage mosaic1.tif -JX10c -R-45/-35/-21/-12 -B1
2. gmt grdcontour dem1.nc -JX10c -R-45/-35/-21/-12 -C500 -A1000 -W1,blue, -t75

1. 1. some tlp event
2. echo -48.0 23.3 | gmt psxy -JX10c -R-R-45/-35/-21/-12 -Sc1.6c -W02p,55/0/0,--

gmt end

1. exit(-1)

1. include "colors.inc"

1. include "functions.inc"
2. include "rand.inc"

1. include "colors.inc"
2. include "stones.inc"

global_settings {

 max_trace_level 5

}

1. declare seed1=seed(123);

1. declare Color=rgb <1,1/2,0.0>*1;

 camera{
   location <0, 150, 3>
   look_at <0,0,3>
   up <0,1,0>
   right <1,0,0>
   angle 10
 }

 light_source{ <1000,150,0>*1000*1000 White*2 }

1. declare surfobj1= height_field {

   png "dem1.png"
   smooth
   pigment { color rgb <1,1,1> }

finish {ambient 0.1 phong 0.1 specular 0.5 diffuse 0.7 } normal { wrinkles scale 1/1000 bump_size -0.1 }

   translate <-.5, -.5, -.5>
   scale <20, 1., 20>
 //  rotate z*180
  // rotate x*180
 }

1. declare smouk1=sphere{ <0,0,0>, 2

       pigment { rgbt 1 }
       hollow

interior{ //---------------------
   media{ method 3
          emission 0.6
         
          scattering{ 4, 
                      <1,1,1>*3.00   
                      extinction  1.50  
          } 

          density{ spherical // or: boxed

octaves 16

                   turbulence 1
                   color_map {
                   [0.00 rgb 0] 
                   [0.05 rgb 0]
                   [0.20 rgb 0.2]
                   [0.30 rgb 0.6]
                   [0.40 rgb 1]
                   [1.00 rgb 1] 
                              } 
          } 

          samples 10,20     // 3,3 for adaptive sampling
          intervals 3     //
          confidence 0.9  //
    } // end of media
 } 
scale 1
rotate<0,0,0>

// translate < -0.5, 1.50 + 0.20,0> }

object {surfobj1 scale 2 rotate y*0 scale y*3}

//object {smouk1 scale 8 scale y/4 translate y*0.3}