diff --git a/StudentNotebooks/Assignment01/vanesm-f24-assignment1.Rmd b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.Rmd new file mode 100644 index 0000000..10eb3a7 --- /dev/null +++ b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.Rmd @@ -0,0 +1,419 @@ +--- +title: "RPI github and Mars 2020 PIXL Notebook:" +subtitle: "DAR Assignment 1" +author: "Margo VanEsselstyn" +date: "`r format(Sys.time(), '%d %B %Y')`" +output: + pdf_document: default + html_document: + toc: true + number_sections: true + df_print: paged +--- +```{r setup, include=FALSE} +# REQUIRE R PACKAGE INSTALLATIONS +# This section installs packages if they are not already installed. +# This block will not be shown in the knitted file. + +# RUN THIS BLOCK BEFORE ATTEMPTING TO KNIT THIS NOTEBOOK!!! + +# Set the default CRAN repository +local({r <- getOption("repos") + r["CRAN"] <- "http://cran.r-project.org" + options(repos=r) +}) + +if (!require("pandoc")) { + install.packages("pandoc") + library(pandoc) +} + +if (!require("knitr")) { + install.packages("knitr") + library(knitr) +} + +# Required packages for M20 LIBS analysis +if (!require("rmarkdown")) { + install.packages("rmarkdown") + library(rmarkdown) +} + +if (!require("tidyverse")) { + install.packages("tidyverse") + library(tidyverse) +} + +if (!require("stringr")) { + install.packages("stringr") + library(stringr) +} + +if (!require("ggbiplot")) { + install.packages("ggbiplot") + library(ggbiplot) +} + +if (!require("pheatmap")) { + install.packages("pheatmap") + library(pheatmap) +} + +if (!require("ggrepel")) { + install.packages("ggrepel") + library(ggrepel) +} + +if (!require("farver")) { + install.packages("farver") + library(farver) +} + +if (!require("labeling")) { + install.packages("labeling") + library(labeling) +} + +knitr::opts_chunk$set(echo = TRUE) + +``` + +# Introductory Data Analytics Research Notebook + +This notebook is broken into two main parts: + +* Part 1: A basic introduction to github and RStudio Server +* Part 2: An introduction to the Mars 2020 PIXL dataset + +The RPI github repository for all the code and data required for this notebook may be found at: + +* https://github.rpi.edu/DataINCITE/DAR-Mars-F24 + + +## BEFORE YOU BEGIN: github account setup + +To contribute to any RPI github repository or read private repos you _must_ validate your RPI github.com ID and send a confirmation email to John Erickson at `erickj4@rpi.edu`. Please do the following **now**: + +**Enabling 2FA on the RPI github and saving personal access tokens, et.al.** + +* Browse to http://github.rpi.edu +* Login using your RPI credentials +* Enable github two-factor authentication (2FA) +* Under "Settings" -> "Password and authentication" +* Select "Authenticator app" (Duo or Google authenticator are recommended) + * Follow steps to set up authenticator app; may involve scanning a QR Code) + * See directions for 2FA at https://itssc.rpi.edu/hc/en-us/articles/360004801811-GitHub-Enterprise-Overview#2fa + * **CRITICAL:** Make sure to save your **recovery codes** in a safe place! Recovery codes can be used to access your account in the event you lose access to your device and cannot receive two-factor authentication codes. +* Create and save a *personal access token* + * Under "Settings" -> "Developer settings" + * Select "Personal access tokens" + * Click on "Generate new token (classic)" + * Set an expiration period for the end of the Fall 2024 term + * Enable everything (check the left-most boxes) + * Generate (green button) + * SAVE THE RESULT! You won't be able to see it again... +* _Use this token when command-line git asks you for a password_ +* **PLEASE DO THIS IMMEDIATELY BEFORE READING ANY FURTHER!!** + +# DAR ASSIGNMENT 1 (Part 1): CLONING A NOTEBOOK AND UPDATING THE REPOSITORY + +In this assignment we're asking you to + +* clone the `DAR-Mars-F24` github repository, +* create a personal branch using git, +* create a new notebook that includes your answers to questions in this notebook, +* make additions to the repository by adding your notebook to the repository. + +_The instructions which follow explain how to accomplish this._ + +**For DAR Fall 2024** you *must* be using RStudio Server on the IDEA Cluster. Instructions for accessing "The Cluster" appear at the end of this notebook. Don't forget to validate your RPI github ID as above and email `erickj4@rpi.edu` + +### Cloning an RPI github repository + +The recommended procedure for cloning and using this repository is as follows: + +* Access the RPI network via VPN + * See https://itssc.rpi.edu/hc/en-us/articles/360008783172-VPN-Connection-and-Installation for information + +* Access RStudio Server on the IDEA Cluster at http://lp01.idea.rpi.edu/rstudio-ose/ + * You must be on the RPI VPN!! +* Access the Linux shell on the IDEA Cluster by clicking the **Terminal** tab of RStudio Server (lower left panel). + * You now see the Linux shell on the IDEA Cluster + * `cd` (change directory) to enter your home directory using: `cd ~` + * Type `pwd` to confirm + * NOTE: Advanced users may use `ssh` to directly access the Linux shell from a macOS or Linux command line +* Type `git clone https://github.rpi.edu/DataINCITE/DAR-Mars-F24` from within your `home` directory + * Enter your RCS ID and your saved personal access token when asked + * This will create a new directory `DAR-Mars-F24` +* In the Linux shell, `cd` to `DAR-Mars-F24/StudentNotebooks/Assignment01` + * Type `ls -al` to list the current contents + * Don't be surprised if you see many files! +* In the Linux shell, type `git checkout -b dar-yourrcs` where `yourrcs` is your RCS id + * For example, if your RCS is `erickj4`, your new branch should be `dar-erickj4` + * It is _critical_ that you include your RCS id in your branch id! +* Back in the RStudio Server UI, navigate to the `DAR-Mars-F24/StudentNotebooks/Assignment01` directory via the **Files** panel (lower right panel) + * Under the **More** menu, set this to be your R working directory + * Setting the correct working directory is essential for interactive R use! + +## REQUIRED FOR ASSIGNMENT 1 + +1. In RStudio, make a **copy** of `dar-f24-assignment1-template.Rmd` file using a *new, original, descriptive* filename that **includes your RCS ID!** + * Open `darf24-assignment1-template.Rmd` + * **Save As...** using a new filename that includes your RCS ID + * Example filename for user `erickj4`: `erickj4-assignment1-f24.Rmd` + * POINTS OFF IF: + * You don't create a new filename! + * You don't include your RCS ID! + * You include `template` in your new filename! +2. Edit your new notebook using RStudio and save + * Change the `title:` and `subtitle:` headers (at the top of the file) + * Change the `author:` + * Don't bother changing the `date:`; it should update automagically... + * **Save** your changes +3. Use the RStudio `Knit` command to create an HTML file; repeat as necessary + * Use the down arrow next to the word `Knit` and select **Knit to HTML** + * You may also knit to PDF... +4. In the Linux terminal, use `git add` to add each new file you want to add to the repository + * Type: `git add yourfilename.Rmd` + * Type: `git add yourfilename.html` (created when you knitted) + * Add your PDF if you also created one... +5. Continue making changes to your personal notebook + * Add code where specified + * Answer questions were indicated. +6. When you're ready, in Linux commit your changes: + * Type: `git commit -m "some comment"` where "some comment" is a useful comment describing your changes + * This commits your changes to your local repo, and sets the stage for your next operation. +7. Finally, push your commits to the RPI github repo + * Type: `git push origin dar-yourrcs` (where `dar-yourrcs` is the branch you've been working in) + * Enter your RCS ID and personal access token (as a password) when asked. + * Your changes are now safely on the RPI github. +8. **REQUIRED:** On the RPI github, submit a pull request. + * In a web browser, navigate to https://github.rpi.edu/DataINCITE/DAR-Mars-F24.git + and log in using 2FA + * In the branch selector drop-down (by default says **main**), select your branch + * **Submit a pull request for your branch** + * One of the DAR instructors will merge your branch, and your new files will be added to the master branch of the repo. + +Please also see these handy github "cheatsheets": + + * https://education.github.com/git-cheat-sheet-education.pdf + +# DAR ASSIGNMENT 1 (Part 2): Exploring the Mars 2020 (M20) PIXL Dataset + +This part of the notebook demonstrates some basic analysis of data from the M20 PIXL (Planetary Instrument for X-ray Lithochemistry) experiment. + +PIXL (Planetary Instrument for X-ray Lithochemistry) is a microfocus X-ray fluorescence instrument that measures elemental chemistry at sub-millimeter scales. This is achieved by focusing an X-ray beam to a small spot ~ 150 µm, scanning the surface with this beam, and then measuring the induced X-ray fluorescence. PIXL observations consist of a suite of X-ray fluorescence measurements, context images, and metadata. The XRF measurements can be executed in a variety of geometries depending on target type and available observation time, and are accompanied by a set of images documenting the target and its position relative to the instrument. + +In this notebook we will be looking at pre-processed PIXL data that is ready for your next steps. + +* More about the PIXL instrument: https://an.rsl.wustl.edu/help/Content/About%20the%20mission/M20/Instruments/M20%20PIXL.htm +* Raw PIXL data bundle: https://pds-geosciences.wustl.edu/m2020/urn-nasa-pds-mars2020_pixl/ + +## Load the PIXL Data and display summary + +Here is the MARS PIXL data. Take note of the variables, their types, and distriubtions. + +```{r} +# Saved LIBS data with locations added + +# NOTE: Use course directory version during the semester +pixl.df<- readRDS("~/DAR-Mars-F24/Data/samples_pixl_wide.Rds") +# Use this version to use downloaded data from github +# pixl.df <- readRDS("~/DAR-Mars-F24/Data/samples_pixl_wide.Rds") +#/academics/MATP-4910-F24/DAR-Mars-F24/Data/samples_pixl_wide.Rds + +# convert location to a number +pixl.df$location <- as.numeric(pixl.df$location ) + +# Automatically converts all strings to factors +pixl.df[sapply(pixl.df, is.character)] <- + lapply(pixl.df[sapply(pixl.df, + is.character)], as.factor) + +# Show summary of the data +summary(pixl.df) + +``` + + +Create a matrix containing the measurements without any meta data to prepare for clustering. Here we delibrately do not scale the data to get preliminary results. + +```{r} +# Prepare dataset for clustering selecting specific columns of interest and putting in a matrix +pixl_trim.mat <- pixl.df %>% + dplyr::select(c("Na20","Mgo","Al203","Si02", + "P205","S03","Cl","K20","Cao","Ti02", + "Cr203","Mno","FeO-T")) %>% as.matrix() +summary(pixl_trim.mat) +``` + +# Clustering + +Our first analysis goal is to cluster the mineralogy data using K-means and pick the appropriate number of clusters. + +Here we recall the function `wssplot` we created in MATP-4400 (IDM) to examine cluster sizes in order to perform the "elbow" test. The function takes as its arguments a matrix, the maximum number of clusters and a random seed. It creates clusters for each possible value of k and plots the k-means objective function. + +NOTE: The basic syntax for creating a user-defined function in R is: + +`output <- function(arguments){ do stuff }` + +The following plot shows the K-Means objective value for up to eight clusters. + +```{r} +# A user-defined function to examine clusters and plot the results +wssplot <- function(data, nc=15, seed=10){ + wss <- data.frame(cluster=1:nc, quality=c(0)) + for (i in 1:nc){ + set.seed(seed) + wss[i,2] <- kmeans(data, centers=i)$tot.withinss} + ggplot(data=wss,aes(x=cluster,y=quality)) + + geom_line() + + ggtitle("Quality of k-means by Cluster") +} + +# Apply `wssplot()` to our PIXL data +wssplot(pixl_trim.mat, nc=8, seed=2) +``` + + +Based on where the "elbow" occurs, it looks like `d` might be a good `k` choice for k-means clustering. + +## k-means Clustering + +We create the final clustering with 5 clusters. + +```{r} +# Use our chosen 'k' to perform k-means clustering +set.seed(2) +k <- 3 +km <- kmeans(pixl_trim.mat,k) + +``` + +## Examine cluster means + +Below is a heat map of the cluster centers with rows and columns clustered. We keep the scale the same as in the original data. + +```{r} + +pheatmap(km$centers,scale="none") + +``` + +Notice how the means of the clusters vary. + +## Perform PCA on PIXL Data + +We're now ready to perform PCA. Note we have already scaled data so set `scale=FALSE`. + +We first show a [Scree plot](https://en.wikipedia.org/wiki/Scree_plot) to understand the explained variance by principal component. Note the elbow in the Scree plot should roughly match the one you saw in k-means. + +```{r} +# Perform the PCA on the matrix `pixl_trim.mat` we created earlier + +pixl_trim.mat.pca <- prcomp(pixl_trim.mat, scale=FALSE) + +# generate the Scree plot +ggscreeplot(pixl_trim.mat.pca) +``` + +Make a table indicating how many samples are in each cluster. + +```{r} +# clusters sizes are in the km object produced by kmeans +cluster.df<-data.frame(cluster= 1:3, size=km$size) +kable(cluster.df,caption="Samples per cluster") +``` + + +## Create a PCA Biplot using ggbiplot + +Now we'll create a biplot of the data colored by cluster and label by rock type. + +```{r message=FALSE, warning=FALSE} +# For this lab we'll create a PCA biplot the easy way using ggbiplot! +ggbiplot::ggbiplot(pixl_trim.mat.pca, + labels = pixl.df$type, + groups = as.factor(km$cluster)) + + xlim(-2,2) + ylim(-2,2) + +``` + +## ANSWER THESE QUESTIONS! + +Add a description of each cluster here in your own words. + +Describe Cluster 1: Cluster 1 is made up of igneous rocks with high silicon dioxide + +Describe Cluster 2: Cluster 2 is made up of only sedimentary rocks and contains all the sedimentary samples + +Describe Cluster 3: Cluster 3 is made up of igneous rocks and other samples + + +What do the clustering and PCA results tell us about the data detected by the M20 PIXL experiment? _Feel free to add graphs or analyses to support your conclusions._ + +The clustering and PCA results show us that the amount of silicon dioxide is heavily correlated with whether a rock is igneous or sedimentary, and that the amount of silicon dioxide differs very heavily in the clusters. Maybe if the data was scaled differently this wouldn't necessarily be true though. + +```{r} +# Student's code for graphs and analysis here! + +pheatmap(km$centers, + scale = "none", + main = "Kmeans Cluster Centers Unscaled", + angle_col=0, + cluster_rows = FALSE, + cluster_cols = FALSE + ) +``` + +## SAVE, COMMIT and PUSH YOUR CHANGES! + +When you are satisfied with your edits and your notebook knits successfully, remember to push your changes to the repo using **steps 4-8** in **Section 2.2**, summarized here: + +**In the Linux terminal:** + +* `git branch` + * To double-check that you are in your working branch +* `git add ` + * Your Rmd and knitted PDF +* `git commit -m "Some useful comments"` +* `git push origin ` + +**On github:** + +* Log in at https://github.rpi.edu/DataINCITE/DAR-Mars-F24 +* Select your branch from drop-down (default is **main**) +* Submit a "pull request" for your branch +* DO NOT MERGE!!! + +# APPENDIX: Accessing RStudio Server on the IDEA Cluster + +The IDEA Cluster provides seven compute nodes (4x 48 cores, 3x 80 cores, 1x storage server) + +* The Cluster requires RCS credentials, enabled via registration in class + * email John Erickson for problems `erickj4@rpi.edu` +* RStudio, Jupyter, MATLAB, GPUs (on two nodes); lots of storage and computes +* Access via RPI physical network or VPN only + +# More info about Rstudio on our Cluster + +## RStudio GUI Access: + +* Use: + * http://lp01.idea.rpi.edu/rstudio-ose/ + * http://lp01.idea.rpi.edu/rstudio-ose-3/ + * http://lp01.idea.rpi.edu/rstudio-ose-6/ + * http://lp01.idea.rpi.edu/rstudio-ose-7/ +* Linux terminal accessible from within RStudio "Terminal" or via ssh (below) + +## Shared Data on Cluster: + +* Users enrolled in DAR have access to `/academics/MATP-4910-F24` + * Usually DAR users will see a symbolic ("soft") link in their home directories + * If you do not, type the following in the **Terminal** via RStudio: `ln -s /academics/MATP-4910-F23/ MATP-4910-F24` +* All idea_users have access to shared storage via `/data` ("data" in your home directories) + * You might wish to use this for data sharing in team projects... + * ...but we recommend using github for shared code development +* Shell access to nodes: You must access "landing pad" first, then compute node: +* `ssh your_rcs@lp01.idea.rpi.edu` For example: `ssh erickj4@lp01.idea.rpi.edu` +* Then, `ssh` to the desired compute node, e.g.: `ssh idea-node-02` \ No newline at end of file diff --git a/StudentNotebooks/Assignment01/vanesm-f24-assignment1.html b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.html new file mode 100644 index 0000000..5697c55 --- /dev/null +++ b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.html @@ -0,0 +1,683 @@ + + + + + + + + + + + + + + + +RPI github and Mars 2020 PIXL Example Notebook: + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + +
+ + + + + + + + +
+

1 Introductory Data Analytics Research Notebook

+

This notebook is broken into two main parts:

+
    +
  • Part 1: A basic introduction to github and RStudio Server
    • +
  • Part 2: An introduction to the Mars 2020 PIXL dataset
    • +
+

The RPI github repository for all the code and data required for this notebook may be found at:

+ +
+

1.1 BEFORE YOU BEGIN: github account setup

+

To contribute to any RPI github repository or read private repos you must validate your RPI github.com ID and send a confirmation email to John Erickson at erickj4@rpi.edu. Please do the following now:

+

Enabling 2FA on the RPI github and saving personal access tokens, et.al.

+
    +
  • Browse to http://github.rpi.edu
    • +
  • Login using your RPI credentials
    • +
  • Enable github two-factor authentication (2FA)
    • +
  • Under “Settings” -> “Password and authentication”
    • +
  • Select “Authenticator app” (Duo or Google authenticator are recommended) +
    • +
  • Create and save a personal access token +
      +
    • Under “Settings” -> “Developer settings”
      • +
    • Select “Personal access tokens”
      • +
    • Click on “Generate new token (classic)”
      • +
    • Set an expiration period for the end of the Fall 2024 term
      • +
    • Enable everything (check the left-most boxes)
      • +
    • Generate (green button)
      • +
    • SAVE THE RESULT! You won’t be able to see it again…
      • +
    • +
  • Use this token when command-line git asks you for a password
    • +
  • PLEASE DO THIS IMMEDIATELY BEFORE READING ANY FURTHER!!
    • +
+
+
+
+

2 DAR ASSIGNMENT 1 (Part 1): CLONING A NOTEBOOK AND UPDATING THE REPOSITORY

+

In this assignment we’re asking you to

+
    +
  • clone the DAR-Mars-F24 github repository,
    • +
  • create a personal branch using git,
    • +
  • create a new notebook that includes your answers to questions in this notebook,
    • +
  • make additions to the repository by adding your notebook to the repository.
    • +
+

The instructions which follow explain how to accomplish this.

+

For DAR Fall 2024 you must be using RStudio Server on the IDEA Cluster. Instructions for accessing “The Cluster” appear at the end of this notebook. Don’t forget to validate your RPI github ID as above and email erickj4@rpi.edu

+
+

2.0.1 Cloning an RPI github repository

+

The recommended procedure for cloning and using this repository is as follows:

+
    +
  • Access the RPI network via VPN +
    • +
  • Access RStudio Server on the IDEA Cluster at http://lp01.idea.rpi.edu/rstudio-ose/ +
      +
    • You must be on the RPI VPN!!
      • +
    • +
  • Access the Linux shell on the IDEA Cluster by clicking the Terminal tab of RStudio Server (lower left panel). +
      +
    • You now see the Linux shell on the IDEA Cluster
      • +
    • cd (change directory) to enter your home directory using: cd ~
      • +
    • Type pwd to confirm
      • +
    • NOTE: Advanced users may use ssh to directly access the Linux shell from a macOS or Linux command line
      • +
    • +
  • Type git clone https://github.rpi.edu/DataINCITE/DAR-Mars-F24 from within your home directory +
      +
    • Enter your RCS ID and your saved personal access token when asked
      • +
    • This will create a new directory DAR-Mars-F24
      • +
    • +
  • In the Linux shell, cd to DAR-Mars-F24/StudentNotebooks/Assignment01 +
      +
    • Type ls -al to list the current contents
      • +
    • Don’t be surprised if you see many files!
      • +
    • +
  • In the Linux shell, type git checkout -b dar-yourrcs where yourrcs is your RCS id +
      +
    • For example, if your RCS is erickj4, your new branch should be dar-erickj4
      • +
    • It is critical that you include your RCS id in your branch id!
      • +
    • +
  • Back in the RStudio Server UI, navigate to the DAR-Mars-F24/StudentNotebooks/Assignment01 directory via the Files panel (lower right panel) +
      +
    • Under the More menu, set this to be your R working directory
      • +
    • Setting the correct working directory is essential for interactive R use!
      • +
    • +
+
+
+

2.1 REQUIRED FOR ASSIGNMENT 1

+
    +
  1. In RStudio, make a copy of dar-f24-assignment1-template.Rmd file using a new, original, descriptive filename that includes your RCS ID! +
      +
    • Open darf24-assignment1-template.Rmd
      • +
    • Save As… using a new filename that includes your RCS ID
      • +
    • Example filename for user erickj4: erickj4-assignment1-f24.Rmd
      • +
    • POINTS OFF IF: +
        +
      • You don’t create a new filename!
        • +
      • You don’t include your RCS ID!
        • +
      • You include template in your new filename!
        • +
      • +
    2. +
  2. Edit your new notebook using RStudio and save +
      +
    • Change the title: and subtitle: headers (at the top of the file)
      • +
    • Change the author:
      • +
    • Don’t bother changing the date:; it should update automagically…
      • +
    • Save your changes
      • +
    3. +
  3. Use the RStudio Knit command to create an HTML file; repeat as necessary +
      +
    • Use the down arrow next to the word Knit and select Knit to HTML
      • +
    • You may also knit to PDF…
      • +
    4. +
  4. In the Linux terminal, use git add to add each new file you want to add to the repository +
      +
    • Type: git add yourfilename.Rmd
      • +
    • Type: git add yourfilename.html (created when you knitted)
      • +
    • Add your PDF if you also created one…
      • +
    5. +
  5. Continue making changes to your personal notebook +
      +
    • Add code where specified
      • +
    • Answer questions were indicated.
      • +
    6. +
  6. When you’re ready, in Linux commit your changes: +
      +
    • Type: git commit -m "some comment" where “some comment” is a useful comment describing your changes
      • +
    • This commits your changes to your local repo, and sets the stage for your next operation.
      • +
    7. +
  7. Finally, push your commits to the RPI github repo +
      +
    • Type: git push origin dar-yourrcs (where dar-yourrcs is the branch you’ve been working in)
      • +
    • Enter your RCS ID and personal access token (as a password) when asked.
      • +
    • Your changes are now safely on the RPI github.
      • +
    8. +
  8. REQUIRED: On the RPI github, submit a pull request. +
      +
    • In a web browser, navigate to https://github.rpi.edu/DataINCITE/DAR-Mars-F24.git and log in using 2FA
      • +
    • In the branch selector drop-down (by default says main), select your branch
      • +
    • Submit a pull request for your branch
      • +
    • One of the DAR instructors will merge your branch, and your new files will be added to the master branch of the repo.
      • +
    9. +
+

Please also see these handy github “cheatsheets”:

+ +
+
+
+

3 DAR ASSIGNMENT 1 (Part 2): Exploring the Mars 2020 (M20) PIXL Dataset

+

This part of the notebook demonstrates some basic analysis of data from the M20 PIXL (Planetary Instrument for X-ray Lithochemistry) experiment.

+

PIXL (Planetary Instrument for X-ray Lithochemistry) is a microfocus X-ray fluorescence instrument that measures elemental chemistry at sub-millimeter scales. This is achieved by focusing an X-ray beam to a small spot ~ 150 µm, scanning the surface with this beam, and then measuring the induced X-ray fluorescence. PIXL observations consist of a suite of X-ray fluorescence measurements, context images, and metadata. The XRF measurements can be executed in a variety of geometries depending on target type and available observation time, and are accompanied by a set of images documenting the target and its position relative to the instrument.

+

In this notebook we will be looking at pre-processed PIXL data that is ready for your next steps.

+ +
+

3.1 Load the PIXL Data and display summary

+

Here is the MARS PIXL data. Take note of the variables, their types, and distriubtions.

+
# Saved LIBS data with locations added
+
+# NOTE: Use course directory version during the semester
+pixl.df<- readRDS("~/DAR-Mars-F24/Data/samples_pixl_wide.Rds")
+# Use this version to  use downloaded data from github
+# pixl.df <- readRDS("~/DAR-Mars-F24/Data/samples_pixl_wide.Rds")
+#/academics/MATP-4910-F24/DAR-Mars-F24/Data/samples_pixl_wide.Rds
+
+# convert location to a number
+pixl.df$location <- as.numeric(pixl.df$location )
+
+# Automatically converts all strings to factors
+pixl.df[sapply(pixl.df, is.character)] <-
+  lapply(pixl.df[sapply(pixl.df, 
+                                  is.character)], as.factor)
+
+# Show summary of the data 
+summary(pixl.df)
+
##      sample           Na20            Mgo             Al203       
+##  Min.   : 1.00   Min.   :1.000   Min.   : 0.730   Min.   : 1.700  
+##  1st Qu.: 4.75   1st Qu.:1.853   1st Qu.: 2.533   1st Qu.: 2.220  
+##  Median : 8.50   Median :1.900   Median :12.800   Median : 3.710  
+##  Mean   : 8.50   Mean   :2.672   Mean   :11.682   Mean   : 5.072  
+##  3rd Qu.:12.25   3rd Qu.:4.500   3rd Qu.:19.100   3rd Qu.: 7.117  
+##  Max.   :16.00   Max.   :5.550   Max.   :22.700   Max.   :11.600  
+##                                                                   
+##       Si02            P205             S03               Cl       
+##  Min.   :22.60   Min.   :0.1000   Min.   : 0.780   Min.   :0.400  
+##  1st Qu.:31.22   1st Qu.:0.2350   1st Qu.: 1.495   1st Qu.:0.940  
+##  Median :38.85   Median :0.5250   Median : 2.600   Median :1.740  
+##  Mean   :38.55   Mean   :0.6512   Mean   : 5.562   Mean   :1.846  
+##  3rd Qu.:41.17   3rd Qu.:0.8400   3rd Qu.: 3.800   3rd Qu.:2.080  
+##  Max.   :57.10   Max.   :2.7600   Max.   :21.530   Max.   :4.500  
+##                                                                   
+##       K20              Cao             Ti02            Cr203      
+##  Min.   :0.0000   Min.   :1.500   Min.   :0.2000   Min.   :0.000  
+##  1st Qu.:0.1600   1st Qu.:2.655   1st Qu.:0.5900   1st Qu.:0.025  
+##  Median :0.2000   Median :3.120   Median :0.7000   Median :0.155  
+##  Mean   :0.5800   Mean   :3.688   Mean   :0.8194   Mean   :0.355  
+##  3rd Qu.:0.8275   3rd Qu.:4.310   3rd Qu.:0.9900   3rd Qu.:0.290  
+##  Max.   :1.9000   Max.   :7.770   Max.   :2.4900   Max.   :1.900  
+##                                                                   
+##       Mno             FeO-T               name             type  
+##  Min.   :0.1000   Min.   :13.24   Atsah     : 1   Igneous    :8  
+##  1st Qu.:0.2800   1st Qu.:16.71   Bearwallow: 1   N/A        :1  
+##  Median :0.4000   Median :23.86   Coulettes : 1   Sedimentary:7  
+##  Mean   :0.3812   Mean   :21.45   Hahonih   : 1                  
+##  3rd Qu.:0.4900   3rd Qu.:25.70   Hazeltop  : 1                  
+##  Max.   :0.6900   Max.   :30.05   Kukaklek  : 1                  
+##                                   (Other)   :10                  
+##          campaign    location             abrasion
+##  Crater Floor:9   Min.   : 1.00   Alfalfa     :2  
+##  Delta Front :7   1st Qu.: 4.75   Bellegrade  :2  
+##                   Median : 8.50   Berry Hollow:2  
+##                   Mean   : 8.50   Dourbes     :2  
+##                   3rd Qu.:12.25   Novarupta   :2  
+##                   Max.   :16.00   Quartier    :2  
+##                                   (Other)     :4
+

Create a matrix containing the measurements without any meta data to prepare for clustering. Here we delibrately do not scale the data to get preliminary results.

+
# Prepare dataset for clustering selecting specific columns of interest and putting in a matrix
+pixl_trim.mat <- pixl.df %>% 
+  dplyr::select(c("Na20","Mgo","Al203","Si02",
+           "P205","S03","Cl","K20","Cao","Ti02",
+           "Cr203","Mno","FeO-T")) %>% as.matrix() 
+summary(pixl_trim.mat)
+
##       Na20            Mgo             Al203             Si02      
+##  Min.   :1.000   Min.   : 0.730   Min.   : 1.700   Min.   :22.60  
+##  1st Qu.:1.853   1st Qu.: 2.533   1st Qu.: 2.220   1st Qu.:31.22  
+##  Median :1.900   Median :12.800   Median : 3.710   Median :38.85  
+##  Mean   :2.672   Mean   :11.682   Mean   : 5.072   Mean   :38.55  
+##  3rd Qu.:4.500   3rd Qu.:19.100   3rd Qu.: 7.117   3rd Qu.:41.17  
+##  Max.   :5.550   Max.   :22.700   Max.   :11.600   Max.   :57.10  
+##       P205             S03               Cl             K20        
+##  Min.   :0.1000   Min.   : 0.780   Min.   :0.400   Min.   :0.0000  
+##  1st Qu.:0.2350   1st Qu.: 1.495   1st Qu.:0.940   1st Qu.:0.1600  
+##  Median :0.5250   Median : 2.600   Median :1.740   Median :0.2000  
+##  Mean   :0.6512   Mean   : 5.562   Mean   :1.846   Mean   :0.5800  
+##  3rd Qu.:0.8400   3rd Qu.: 3.800   3rd Qu.:2.080   3rd Qu.:0.8275  
+##  Max.   :2.7600   Max.   :21.530   Max.   :4.500   Max.   :1.9000  
+##       Cao             Ti02            Cr203            Mno        
+##  Min.   :1.500   Min.   :0.2000   Min.   :0.000   Min.   :0.1000  
+##  1st Qu.:2.655   1st Qu.:0.5900   1st Qu.:0.025   1st Qu.:0.2800  
+##  Median :3.120   Median :0.7000   Median :0.155   Median :0.4000  
+##  Mean   :3.688   Mean   :0.8194   Mean   :0.355   Mean   :0.3812  
+##  3rd Qu.:4.310   3rd Qu.:0.9900   3rd Qu.:0.290   3rd Qu.:0.4900  
+##  Max.   :7.770   Max.   :2.4900   Max.   :1.900   Max.   :0.6900  
+##      FeO-T      
+##  Min.   :13.24  
+##  1st Qu.:16.71  
+##  Median :23.86  
+##  Mean   :21.45  
+##  3rd Qu.:25.70  
+##  Max.   :30.05
+
+
+
+

4 Clustering

+

Our first analysis goal is to cluster the mineralogy data using K-means and pick the appropriate number of clusters.

+

Here we recall the function wssplot we created in MATP-4400 (IDM) to examine cluster sizes in order to perform the “elbow” test. The function takes as its arguments a matrix, the maximum number of clusters and a random seed. It creates clusters for each possible value of k and plots the k-means objective function.

+

NOTE: The basic syntax for creating a user-defined function in R is:

+

output <- function(arguments){ do stuff }

+

The following plot shows the K-Means objective value for up to eight clusters.

+
# A user-defined function to examine clusters and plot the results
+wssplot <- function(data, nc=15, seed=10){
+  wss <- data.frame(cluster=1:nc, quality=c(0))
+  for (i in 1:nc){
+    set.seed(seed)
+    wss[i,2] <- kmeans(data, centers=i)$tot.withinss}
+  ggplot(data=wss,aes(x=cluster,y=quality)) + 
+    geom_line() + 
+    ggtitle("Quality of k-means by Cluster")
+}
+
+# Apply `wssplot()` to our PIXL data
+wssplot(pixl_trim.mat, nc=8, seed=2)
+

+

Based on where the “elbow” occurs, it looks like d might be a good k choice for k-means clustering.

+
+

4.1 k-means Clustering

+

We create the final clustering with 5 clusters.

+
# Use our chosen 'k' to perform k-means clustering
+set.seed(2)
+k <- 3
+km <- kmeans(pixl_trim.mat,k)
+
+
+

4.2 Examine cluster means

+

Below is a heat map of the cluster centers with rows and columns clustered. We keep the scale the same as in the original data.

+
pheatmap(km$centers,scale="none")
+

+

Notice how the means of the clusters vary.

+
+
+

4.3 Perform PCA on PIXL Data

+

We’re now ready to perform PCA. Note we have already scaled data so set scale=FALSE.

+

We first show a Scree plot to understand the explained variance by principal component. Note the elbow in the Scree plot should roughly match the one you saw in k-means.

+
# Perform the PCA on the matrix `pixl_trim.mat` we created earlier
+
+pixl_trim.mat.pca <- prcomp(pixl_trim.mat, scale=FALSE)
+
+# generate the Scree plot
+ggscreeplot(pixl_trim.mat.pca)
+

+

Make a table indicating how many samples are in each cluster.

+
# clusters sizes are in the km object produced by kmeans
+cluster.df<-data.frame(cluster= 1:3, size=km$size)
+kable(cluster.df,caption="Samples per cluster")
+ + + + + + + + + + + + + + + + + + + + + + +
Samples per cluster
clustersize
13
27
36
+
+
+

4.4 Create a PCA Biplot using ggbiplot

+

Now we’ll create a biplot of the data colored by cluster and label by rock type.

+
# For this lab we'll create a PCA biplot the easy way using ggbiplot!
+ggbiplot::ggbiplot(pixl_trim.mat.pca,
+                   labels = pixl.df$type,
+                   groups = as.factor(km$cluster)) +
+  xlim(-2,2) + ylim(-2,2)
+

+
+
+

4.5 ANSWER THESE QUESTIONS!

+

Add a description of each cluster here in your own words.

+

Describe Cluster 1: Your description here

+

Describe Cluster 2: Your description here

+

Describe Cluster 3: Your description here

+

What do the clustering and PCA results tell us about the data detected by the M20 PIXL experiment? Feel free to add graphs or analyses to support your conclusions.

+
# Student's code for graphs and analysis here!
+
+
+

4.6 SAVE, COMMIT and PUSH YOUR CHANGES!

+

When you are satisfied with your edits and your notebook knits successfully, remember to push your changes to the repo using steps 4-8 in Section 2.2, summarized here:

+

In the Linux terminal:

+
    +
  • git branch +
      +
    • To double-check that you are in your working branch
      • +
    • +
  • git add <your changed files> +
      +
    • Your Rmd and knitted PDF
      • +
    • +
  • git commit -m "Some useful comments"
    • +
  • git push origin <your branch name>
    • +
+

On github:

+ +
+
+
+

5 APPENDIX: Accessing RStudio Server on the IDEA Cluster

+

The IDEA Cluster provides seven compute nodes (4x 48 cores, 3x 80 cores, 1x storage server)

+
    +
  • The Cluster requires RCS credentials, enabled via registration in class +
      +
    • email John Erickson for problems erickj4@rpi.edu
      • +
    • +
  • RStudio, Jupyter, MATLAB, GPUs (on two nodes); lots of storage and computes
    • +
  • Access via RPI physical network or VPN only
    • +
+
+
+

6 More info about Rstudio on our Cluster

+
+

6.1 RStudio GUI Access:

+ +
+
+

6.2 Shared Data on Cluster:

+
    +
  • Users enrolled in DAR have access to /academics/MATP-4910-F24 +
      +
    • Usually DAR users will see a symbolic (“soft”) link in their home directories
      • +
    • If you do not, type the following in the Terminal via RStudio: ln -s /academics/MATP-4910-F23/ MATP-4910-F24
      • +
    • +
  • All idea_users have access to shared storage via /data (“data” in your home directories) +
      +
    • You might wish to use this for data sharing in team projects…
      • +
    • …but we recommend using github for shared code development
      • +
    • +
  • Shell access to nodes: You must access “landing pad” first, then compute node:
    • +
  • ssh your_rcs@lp01.idea.rpi.edu For example: ssh erickj4@lp01.idea.rpi.edu
    • +
  • Then, ssh to the desired compute node, e.g.: ssh idea-node-02
    • +
+
+
+ + + + +
+ + + + + + + + + + + + + + + diff --git a/StudentNotebooks/Assignment01/vanesm-f24-assignment1.pdf b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.pdf new file mode 100644 index 0000000..d9eea0e Binary files /dev/null and b/StudentNotebooks/Assignment01/vanesm-f24-assignment1.pdf differ