change the docs

Author: yzh211

docs/notebooks/pyosp_licking.ipynb

@@ -130,15 +130,15 @@
    "id": "ae8d4b4d",
    "metadata": {},
    "source": [
-    "In the figure above, the dark red clusters overlap at tread elevations as we identified in the field. Details are presented in Figure 10 of PyOSP paper. \n",
+    "In the figure above, the dark red clusters correspond to terrace tread elevations as we identified in the field. Details are presented in Figure 10 of PyOSP paper. \n",
     "\n",
     "### Cross-swath profiles\n",
     "\n",
     "Four cross-swath sections were selected to examine the topographic view of each area.\n",
     "\n",
     "As we mentioned in the Teton case study, there are two ways to define the boundary of cross swath profile:\n",
     "\n",
-    "1. Specify the start and end points distance away from the starting point of baseline.\n",
+    "1. Specify the start and end points positions away from the starting point of baseline.\n",
     "2. Draw the points along the baseline, and then pass the shapefile of points to the function. \n",
     "\n",
     "In the documentation of PyOSP, there is a tutorial about application process of these two methods.\n",
@@ -307,7 +307,7 @@
    "id": "7d140d22",
    "metadata": {},
    "source": [
-    "Discussion of histograms and cross-swath areas' correlation with terrace treads are presented in the [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). "
+    "Discussion of above results correlation with terrace treads are presented in the [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). "
    ]
   },
   {
@@ -344,4 +344,4 @@
  },
  "nbformat": 4,
  "nbformat_minor": 5
-}
+}

docs/notebooks/pyosp_olympus.ipynb

@@ -7,7 +7,7 @@
    "source": [
     "# Circular swath analysis of Olympus Mons, Mars\n",
     "\n",
-    "In this tutorial, we will perform circular swath analysis toward the largest known shield volcano in the solar system, Olympus Mons, Mars. It consists of TPI bases swath analysis, slice of the profile, and comparison with traditional circular swath profile. The content introduced here corresponds to the section 4.3 of [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). The installation of PyOSP is introduced by the tutorial [Topographic analysis of Teton Range, Wyoming](./pyosp_teton.ipynb), which will not be repeated here.\n",
+    "In this tutorial, we will perform circular swath analysis toward the largest known shield volcano in the solar system, Olympus Mons, Mars. It consists of TPI bases swath analysis, slice of the profile, and comparison between traditional and TPI based circular swath profile. The content introduced here corresponds to the section 4.3 of [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). The installation of PyOSP is introduced by the tutorial [Topographic analysis of Teton Range, Wyoming](./pyosp_teton.ipynb), which will not be repeated here.\n",
     "\n",
     "## Traditional and TPI-based circular swath profiles\n",
     "\n",
@@ -112,11 +112,11 @@
    "id": "eebf7bd7",
    "metadata": {},
    "source": [
-    "The calibrated polygons overlapping the hillshade of Olympus Mons are shown in Figure 12 of [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). Results show that the TPI-based method accurately delineates the edifice along the boundary of the basal scarp, whereas the fixed-radius swath invariably generated a circular area that includes unwanted areas beyond the volcano.The pronounced fall in IQR at 255,000mon the TPI-based swath signals a reduction in datapoints along the southeastern basal scarp and marks the boundary of asymmetry.\n",
+    "The calibrated polygons overlapping the hillshade of Olympus Mons are shown in Figure 12 of [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). Results show that the TPI-based method accurately delineates the edifice along the boundary of the basal scarp, whereas the fixed-radius swath invariably generated a circular area that includes unwanted areas beyond the volcano.The pronounced fall in IQR at 255,000m on the TPI-based swath signals a reduction in datapoints along the southeastern basal scarp and marks the boundary of asymmetry.\n",
     "\n",
     "### Slice plot across the valcano\n",
     "\n",
-    "Finally, we used PyOSP to plot four topographic profiles across the volcano."
+    "Next, we used PyOSP to plot four topographic profiles across the volcano."
    ]
   },
   {
@@ -213,7 +213,9 @@
    "source": [
     "## Summary\n",
     "\n",
-    "This tutorial introduces the swath analysis of Olympus Mons by PyOSP, which corresponds to section 4.3 of PyOSP paper. [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). If you have any further questions, you can open an issue at https://github.com/PyOSP-devs/PyOSP, or send email to yichuan211@gmail.com\n",
+    "This tutorial introduces the swath analysis of Olympus Mons by PyOSP, which corresponds to section 4.3 of [PyOSP paper](https://www.sciencedirect.com/science/article/abs/pii/S0169555X21001860). \n",
+    "\n",
+    "If you have any questions, you can open an issue at https://github.com/PyOSP-devs/PyOSP, or send email to yichuan211@gmail.com\n",
     "\n",
     "Cheers!"
    ]

docs/notebooks/pyosp_teton.ipynb

@@ -298,7 +298,7 @@
     "## Cross swath profile\n",
     "Next, we evaluate five cross swath profiles along the striking of the baseline. There are two ways to define the boundary of cross swath profile:\n",
     "\n",
-    "1. Specify the start and end points distance away from the starting point of baseline.\n",
+    "1. Specify the start and end points distance positions from the starting point of baseline.\n",
     "2. Draw the points along the baseline, and then pass the shapefile of points to the function. \n",
     "\n",
     "In the documentation of PyOSP, there is a tutorial about application process of these two methods.\n",