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Resolve spatial rest + swath vs focal trade
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@stephanieyflu
stephanieyflu committed Nov 30, 2023
1 parent 362b3a5 commit c0c6fde
Showing 1 changed file with 78 additions and 38 deletions.
116 changes: 78 additions & 38 deletions tradebooks/spatial_resolution_&_swath_vs_focal_length_trade.ipynb
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Original file line number Diff line number Diff line change
Expand Up @@ -10,9 +10,21 @@
},
{
"cell_type": "code",
"execution_count": 1,
"execution_count": 40,
"metadata": {},
"outputs": [],
"outputs": [
{
"ename": "ImportError",
"evalue": "cannot import name 'orient_and_broadcast' from 'architect.libs.utillib' (C:\\Users\\Optics\\Documents\\GitHub\\architect\\architect\\libs\\utillib.py)",
"output_type": "error",
"traceback": [
"\u001b[1;31m---------------------------------------------------------------------------\u001b[0m",
"\u001b[1;31mImportError\u001b[0m Traceback (most recent call last)",
"\u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\tradebooks\\spatial_resolution_&_swath_vs_focal_length_trade.ipynb Cell 2\u001b[0m line \u001b[0;36m<cell line: 12>\u001b[1;34m()\u001b[0m\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X65sZmlsZQ%3D%3D?line=8'>9</a>\u001b[0m \u001b[39mfrom\u001b[39;00m \u001b[39mIPython\u001b[39;00m\u001b[39m.\u001b[39;00m\u001b[39mdisplay\u001b[39;00m \u001b[39mimport\u001b[39;00m display\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X65sZmlsZQ%3D%3D?line=10'>11</a>\u001b[0m \u001b[39m# project\u001b[39;00m\n\u001b[1;32m---> <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X65sZmlsZQ%3D%3D?line=11'>12</a>\u001b[0m \u001b[39mfrom\u001b[39;00m \u001b[39marchitect\u001b[39;00m\u001b[39m.\u001b[39;00m\u001b[39mlibs\u001b[39;00m\u001b[39m.\u001b[39;00m\u001b[39mutillib\u001b[39;00m \u001b[39mimport\u001b[39;00m orient_and_broadcast\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X65sZmlsZQ%3D%3D?line=12'>13</a>\u001b[0m \u001b[39mfrom\u001b[39;00m \u001b[39marchitect\u001b[39;00m\u001b[39m.\u001b[39;00m\u001b[39msystems\u001b[39;00m\u001b[39m.\u001b[39;00m\u001b[39moptical\u001b[39;00m \u001b[39mimport\u001b[39;00m foreoptics, masks, sensors, spectrometers\n",
"\u001b[1;31mImportError\u001b[0m: cannot import name 'orient_and_broadcast' from 'architect.libs.utillib' (C:\\Users\\Optics\\Documents\\GitHub\\architect\\architect\\libs\\utillib.py)"
]
}
],
"source": [
"# stdlib\n",
"from pathlib import Path\n",
Expand All @@ -25,7 +37,7 @@
"from IPython.display import display\n",
"\n",
"# project\n",
"from architect.libs import utillib\n",
"from architect.libs.utillib import orient_and_broadcast\n",
"from architect.systems.optical import foreoptics, masks, sensors, spectrometers"
]
},
Expand All @@ -39,7 +51,7 @@
},
{
"cell_type": "code",
"execution_count": 2,
"execution_count": 12,
"metadata": {},
"outputs": [],
"source": [
Expand All @@ -56,7 +68,7 @@
},
{
"cell_type": "code",
"execution_count": 5,
"execution_count": 36,
"metadata": {},
"outputs": [],
"source": [
Expand All @@ -74,9 +86,7 @@
"\n",
"# region vectorization\n",
"parameter_space_shape = (focal_length.size, slit_size.size)\n",
"focal_length = utillib.orient_and_broadcast(\n",
" a=focal_length, dim=0, shape=parameter_space_shape\n",
")\n",
"focal_length = orient_and_broadcast(a=focal_length, dim=0, shape=parameter_space_shape)\n",
"# endregion"
]
},
Expand All @@ -89,7 +99,7 @@
},
{
"cell_type": "code",
"execution_count": 6,
"execution_count": 37,
"metadata": {},
"outputs": [],
"source": [
Expand All @@ -115,31 +125,26 @@
},
{
"cell_type": "code",
"execution_count": 7,
"execution_count": 38,
"metadata": {},
"outputs": [
{
"ename": "UnitConversionError",
"evalue": "Can only apply 'maximum' function to quantities with compatible dimensions",
"output_type": "error",
"traceback": [
"\u001b[1;31m---------------------------------------------------------------------------\u001b[0m",
"\u001b[1;31mUnitConversionError\u001b[0m Traceback (most recent call last)",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\quantity_helper\\helpers.py:68\u001b[0m, in \u001b[0;36mget_converters_and_unit\u001b[1;34m(f, unit1, unit2)\u001b[0m\n\u001b[0;32m 67\u001b[0m \u001b[39mtry\u001b[39;00m:\n\u001b[1;32m---> 68\u001b[0m converters[changeable] \u001b[39m=\u001b[39m get_converter(unit2, unit1)\n\u001b[0;32m 69\u001b[0m \u001b[39mexcept\u001b[39;00m UnitsError:\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\quantity_helper\\helpers.py:32\u001b[0m, in \u001b[0;36mget_converter\u001b[1;34m(from_unit, to_unit)\u001b[0m\n\u001b[0;32m 30\u001b[0m \u001b[39m\"\"\"Like Unit._get_converter, except returns None if no scaling is needed,\u001b[39;00m\n\u001b[0;32m 31\u001b[0m \u001b[39mi.e., if the inferred scale is unity.\"\"\"\u001b[39;00m\n\u001b[1;32m---> 32\u001b[0m converter \u001b[39m=\u001b[39m from_unit\u001b[39m.\u001b[39;49m_get_converter(to_unit)\n\u001b[0;32m 33\u001b[0m \u001b[39mreturn\u001b[39;00m \u001b[39mNone\u001b[39;00m \u001b[39mif\u001b[39;00m converter \u001b[39mis\u001b[39;00m unit_scale_converter \u001b[39melse\u001b[39;00m converter\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\core.py:1061\u001b[0m, in \u001b[0;36mUnitBase._get_converter\u001b[1;34m(self, other, equivalencies)\u001b[0m\n\u001b[0;32m 1059\u001b[0m \u001b[39mpass\u001b[39;00m\n\u001b[1;32m-> 1061\u001b[0m \u001b[39mraise\u001b[39;00m exc\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\core.py:1046\u001b[0m, in \u001b[0;36mUnitBase._get_converter\u001b[1;34m(self, other, equivalencies)\u001b[0m\n\u001b[0;32m 1045\u001b[0m \u001b[39mtry\u001b[39;00m:\n\u001b[1;32m-> 1046\u001b[0m \u001b[39mreturn\u001b[39;00m \u001b[39mself\u001b[39;49m\u001b[39m.\u001b[39;49m_apply_equivalencies(\n\u001b[0;32m 1047\u001b[0m \u001b[39mself\u001b[39;49m, other, \u001b[39mself\u001b[39;49m\u001b[39m.\u001b[39;49m_normalize_equivalencies(equivalencies))\n\u001b[0;32m 1048\u001b[0m \u001b[39mexcept\u001b[39;00m UnitsError \u001b[39mas\u001b[39;00m exc:\n\u001b[0;32m 1049\u001b[0m \u001b[39m# Last hope: maybe other knows how to do it?\u001b[39;00m\n\u001b[0;32m 1050\u001b[0m \u001b[39m# We assume the equivalencies have the unit itself as first item.\u001b[39;00m\n\u001b[0;32m 1051\u001b[0m \u001b[39m# TODO: maybe better for other to have a `_back_converter` method?\u001b[39;00m\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\core.py:1022\u001b[0m, in \u001b[0;36mUnitBase._apply_equivalencies\u001b[1;34m(self, unit, other, equivalencies)\u001b[0m\n\u001b[0;32m 1020\u001b[0m other_str \u001b[39m=\u001b[39m get_err_str(other)\n\u001b[1;32m-> 1022\u001b[0m \u001b[39mraise\u001b[39;00m UnitConversionError(\n\u001b[0;32m 1023\u001b[0m \u001b[39mf\u001b[39m\u001b[39m\"\u001b[39m\u001b[39m{\u001b[39;00munit_str\u001b[39m}\u001b[39;00m\u001b[39m and \u001b[39m\u001b[39m{\u001b[39;00mother_str\u001b[39m}\u001b[39;00m\u001b[39m are not convertible\u001b[39m\u001b[39m\"\u001b[39m)\n",
"\u001b[1;31mUnitConversionError\u001b[0m: 'km nm / mm' (length) and 'km um' (area) are not convertible",
"\nDuring handling of the above exception, another exception occurred:\n",
"\u001b[1;31mUnitConversionError\u001b[0m Traceback (most recent call last)",
"\u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\tradebooks\\spatial_resolution_&_swath_vs_focal_length_trade.ipynb Cell 10\u001b[0m line \u001b[0;36m<cell line: 1>\u001b[1;34m()\u001b[0m\n\u001b[1;32m----> <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=0'>1</a>\u001b[0m sensor_spatial_resolution \u001b[39m=\u001b[39m payload\u001b[39m.\u001b[39;49mget_spatial_resolution(\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=1'>2</a>\u001b[0m wavelength\u001b[39m=\u001b[39;49mtarget_wavelength,\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=2'>3</a>\u001b[0m target_distance\u001b[39m=\u001b[39;49morbital_altitude,\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=3'>4</a>\u001b[0m skew_angle\u001b[39m=\u001b[39;49mskew_angle[\u001b[39m0\u001b[39;49m],\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=4'>5</a>\u001b[0m )\u001b[39m.\u001b[39mto(unit\u001b[39m.\u001b[39mm)\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=6'>7</a>\u001b[0m display(\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=7'>8</a>\u001b[0m \u001b[39mf\u001b[39m\u001b[39m\"\u001b[39m\u001b[39mSensor-limited spatial resolution test shape: \u001b[39m\u001b[39m{\u001b[39;00msensor_spatial_resolution\u001b[39m.\u001b[39mshape\u001b[39m}\u001b[39;00m\u001b[39m\"\u001b[39m\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=8'>9</a>\u001b[0m )\n\u001b[0;32m <a href='vscode-notebook-cell:/c%3A/Users/Optics/Documents/GitHub/architect/tradebooks/spatial_resolution_%26_swath_vs_focal_length_trade.ipynb#X12sZmlsZQ%3D%3D?line=10'>11</a>\u001b[0m swath \u001b[39m=\u001b[39m payload\u001b[39m.\u001b[39mget_swath(altitude\u001b[39m=\u001b[39morbital_altitude, skew_angle\u001b[39m=\u001b[39mskew_angle)\n",
"File \u001b[1;32m~\\Documents\\GitHub\\architect\\architect\\systems\\optical\\spectrometers.py:280\u001b[0m, in \u001b[0;36mHyperspectralImager.get_spatial_resolution\u001b[1;34m(self, wavelength, target_distance, skew_angle)\u001b[0m\n\u001b[0;32m 270\u001b[0m sensor_spatial_resolution \u001b[39m=\u001b[39m \u001b[39mself\u001b[39m\u001b[39m.\u001b[39mget_sensor_spatial_resolution(\n\u001b[0;32m 271\u001b[0m target_distance\u001b[39m=\u001b[39mtarget_distance\n\u001b[0;32m 272\u001b[0m )\n\u001b[0;32m 274\u001b[0m optical_spatial_resolution \u001b[39m=\u001b[39m \u001b[39mself\u001b[39m\u001b[39m.\u001b[39mget_optical_spatial_resolution(\n\u001b[0;32m 275\u001b[0m wavelength\u001b[39m=\u001b[39mwavelength,\n\u001b[0;32m 276\u001b[0m target_distance\u001b[39m=\u001b[39mtarget_distance,\n\u001b[0;32m 277\u001b[0m skew_angle\u001b[39m=\u001b[39mskew_angle,\n\u001b[0;32m 278\u001b[0m )\n\u001b[1;32m--> 280\u001b[0m spatial_resolution \u001b[39m=\u001b[39m np\u001b[39m.\u001b[39;49mmaximum(\n\u001b[0;32m 281\u001b[0m sensor_spatial_resolution, optical_spatial_resolution\n\u001b[0;32m 282\u001b[0m )\n\u001b[0;32m 284\u001b[0m \u001b[39mreturn\u001b[39;00m spatial_resolution\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\quantity.py:591\u001b[0m, in \u001b[0;36mQuantity.__array_ufunc__\u001b[1;34m(self, function, method, *inputs, **kwargs)\u001b[0m\n\u001b[0;32m 569\u001b[0m \u001b[39m\"\"\"Wrap numpy ufuncs, taking care of units.\u001b[39;00m\n\u001b[0;32m 570\u001b[0m \n\u001b[0;32m 571\u001b[0m \u001b[39mParameters\u001b[39;00m\n\u001b[1;32m (...)\u001b[0m\n\u001b[0;32m 585\u001b[0m \u001b[39m Results of the ufunc, with the unit set properly.\u001b[39;00m\n\u001b[0;32m 586\u001b[0m \u001b[39m\"\"\"\u001b[39;00m\n\u001b[0;32m 587\u001b[0m \u001b[39m# Determine required conversion functions -- to bring the unit of the\u001b[39;00m\n\u001b[0;32m 588\u001b[0m \u001b[39m# input to that expected (e.g., radian for np.sin), or to get\u001b[39;00m\n\u001b[0;32m 589\u001b[0m \u001b[39m# consistent units between two inputs (e.g., in np.add) --\u001b[39;00m\n\u001b[0;32m 590\u001b[0m \u001b[39m# and the unit of the result (or tuple of units for nout > 1).\u001b[39;00m\n\u001b[1;32m--> 591\u001b[0m converters, unit \u001b[39m=\u001b[39m converters_and_unit(function, method, \u001b[39m*\u001b[39;49minputs)\n\u001b[0;32m 593\u001b[0m out \u001b[39m=\u001b[39m kwargs\u001b[39m.\u001b[39mget(\u001b[39m'\u001b[39m\u001b[39mout\u001b[39m\u001b[39m'\u001b[39m, \u001b[39mNone\u001b[39;00m)\n\u001b[0;32m 594\u001b[0m \u001b[39m# Avoid loop back by turning any Quantity output into array views.\u001b[39;00m\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\quantity_helper\\converters.py:174\u001b[0m, in \u001b[0;36mconverters_and_unit\u001b[1;34m(function, method, *args)\u001b[0m\n\u001b[0;32m 171\u001b[0m units \u001b[39m=\u001b[39m [\u001b[39mgetattr\u001b[39m(arg, \u001b[39m'\u001b[39m\u001b[39munit\u001b[39m\u001b[39m'\u001b[39m, \u001b[39mNone\u001b[39;00m) \u001b[39mfor\u001b[39;00m arg \u001b[39min\u001b[39;00m args]\n\u001b[0;32m 173\u001b[0m \u001b[39m# Determine possible conversion functions, and the result unit.\u001b[39;00m\n\u001b[1;32m--> 174\u001b[0m converters, result_unit \u001b[39m=\u001b[39m ufunc_helper(function, \u001b[39m*\u001b[39;49munits)\n\u001b[0;32m 176\u001b[0m \u001b[39mif\u001b[39;00m \u001b[39many\u001b[39m(converter \u001b[39mis\u001b[39;00m \u001b[39mFalse\u001b[39;00m \u001b[39mfor\u001b[39;00m converter \u001b[39min\u001b[39;00m converters):\n\u001b[0;32m 177\u001b[0m \u001b[39m# for multi-argument ufuncs with a quantity and a non-quantity,\u001b[39;00m\n\u001b[0;32m 178\u001b[0m \u001b[39m# the quantity normally needs to be dimensionless, *except*\u001b[39;00m\n\u001b[1;32m (...)\u001b[0m\n\u001b[0;32m 181\u001b[0m \u001b[39m# can just have the unit of the quantity\u001b[39;00m\n\u001b[0;32m 182\u001b[0m \u001b[39m# (this allows, e.g., `q > 0.` independent of unit)\u001b[39;00m\n\u001b[0;32m 183\u001b[0m \u001b[39mtry\u001b[39;00m:\n\u001b[0;32m 184\u001b[0m \u001b[39m# Don't fold this loop in the test above: this rare case\u001b[39;00m\n\u001b[0;32m 185\u001b[0m \u001b[39m# should not make the common case slower.\u001b[39;00m\n",
"File \u001b[1;32mc:\\Users\\Optics\\Documents\\GitHub\\architect\\.venv\\lib\\site-packages\\astropy\\units\\quantity_helper\\helpers.py:70\u001b[0m, in \u001b[0;36mget_converters_and_unit\u001b[1;34m(f, unit1, unit2)\u001b[0m\n\u001b[0;32m 68\u001b[0m converters[changeable] \u001b[39m=\u001b[39m get_converter(unit2, unit1)\n\u001b[0;32m 69\u001b[0m \u001b[39mexcept\u001b[39;00m UnitsError:\n\u001b[1;32m---> 70\u001b[0m \u001b[39mraise\u001b[39;00m UnitConversionError(\n\u001b[0;32m 71\u001b[0m \u001b[39m\"\u001b[39m\u001b[39mCan only apply \u001b[39m\u001b[39m'\u001b[39m\u001b[39m{}\u001b[39;00m\u001b[39m'\u001b[39m\u001b[39m function to quantities \u001b[39m\u001b[39m\"\u001b[39m\n\u001b[0;32m 72\u001b[0m \u001b[39m\"\u001b[39m\u001b[39mwith compatible dimensions\u001b[39m\u001b[39m\"\u001b[39m\n\u001b[0;32m 73\u001b[0m \u001b[39m.\u001b[39mformat(f\u001b[39m.\u001b[39m\u001b[39m__name__\u001b[39m))\n\u001b[0;32m 75\u001b[0m \u001b[39mreturn\u001b[39;00m converters, unit1\n",
"\u001b[1;31mUnitConversionError\u001b[0m: Can only apply 'maximum' function to quantities with compatible dimensions"
]
"data": {
"text/plain": [
"'Sensor-limited spatial resolution test shape: (29, 2)'"
]
},
"metadata": {},
"output_type": "display_data"
},
{
"data": {
"text/plain": [
"'Swath shape: (29, 2)'"
]
},
"metadata": {},
"output_type": "display_data"
}
],
"source": [
Expand All @@ -166,7 +171,7 @@
},
{
"cell_type": "code",
"execution_count": 6,
"execution_count": 39,
"metadata": {},
"outputs": [
{
Expand Down Expand Up @@ -424,9 +429,6 @@
},
"tracegroupgap": 0
},
"margin": {
"t": 60
},
"template": {
"data": {
"bar": [
Expand Down Expand Up @@ -1252,6 +1254,9 @@
}
}
},
"title": {
"text": "Spatial Resolution and Swath vs. Focal Length"
},
"xaxis": {
"anchor": "y",
"domain": [
Expand Down Expand Up @@ -1614,15 +1619,50 @@
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>components</th>\n",
" <th>systems</th>\n",
" <td>list [4]</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>dimensions</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>mass</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>volume</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>density</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>index</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>transmittance</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" <tr>\n",
" <th>spatial_resolution</th>\n",
" <td>None</td>\n",
" <td>None</td>\n",
" </tr>\n",
" </tbody>\n",
"</table>"
],
"text/plain": [
"<architect.systems.spectrometers.HyperspectralImager at 0x21e5db122f0>"
"<architect.systems.optical.spectrometers.HyperspectralImager at 0x1a916eee7a0>"
]
},
"metadata": {},
Expand Down Expand Up @@ -1655,7 +1695,7 @@
" swath_label_x,\n",
" swath_label_y,\n",
" ],\n",
" title=None,\n",
" title=\"Spatial Resolution and Swath vs. Focal Length\",\n",
" dark=True,\n",
")\n",
"\n",
Expand Down

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