Daliedmarie Delgado Maisonet
Project:
The presence of ice deposits on the Moon is key for NASA’s future human-based solar system exploration, but little is currently known about the ice volume and distribution. I will be using a terrestrial lunar analog in the ESRP to evaluate morphometric relationships that arise from progressive sediment cover burying various lava flow types, and how that evolving bulk roughness influences self-shadowing. UAS equipped with LiDAR will collect high-resolution (~1cm/pixel) elevation data, visible wavelength imagery, and thermal data from ESRP lava flows. Methods like rugosity, root-mean-square height, slope, and insolation will be used to calculate terrain roughness, shadowing, and reservoir volumes for potential Ice Stability Regions (ISR). The goal of this work is to generate high-resolution digital elevation models (DEM) from aerial imagery.
Goals:
Complete a Master's degree
Improve scientific communication skills (written, presentations, networking)
Improve fieldwork, lab, and coding skills
Develop leadership skills
Improve teaching skills
For 7/19:
Do ARI map in regular Arc
plot insolation vs thermal measurement on per-pixel basis. What is the relationship?
After you have the TI thing sorted out: Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
IDEAS maps: send as printable atlas to SKN (3 sets)
Add section numbering system to thesis draft sections
Review thesis formatting requirements and start following them now
If time: work on expanding Ch2
Fix fall schedule
For 7/11:
Implement topography algorithm to create ARI map (Finish by Monday COB)
plot insolation vs thermal measurement on per-pixel basis. What is the relationship?
After you have the TI thing sorted out: Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
Finish updating IDEAS maps with alphanumeric values (Finish by Monday COB)
Update Ch2 (moving stuff around, adding list for updating directly to document)
For 7/5:
For Ciazela et al.: go through the math and write out a plan to adopt it in Arc (workflow or code)
implement to create ATI map
Send SKN day flight insolation summative from dawn to flight; compare with snapshot insolation calculated at time of flight uploaded in shared drive
plot insolation vs thermal measurement on per-pixel basis. What is the relationship?
After you have the TI thing sorted out: Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
Finish first draft of Ch1
Ch2: start a list of intended revisions/additions
Update IDEAS maps with alphanumeric values - all uploaded except for COTM because I messed up
For 6/20:
Read/summarize thermal inertia papers for Mars and Earth
work on adapting their approach for Earth -or- keep searching
Day flight insolation: summative from dawn until flight
plot insolation vs thermal measurement on per-pixel basis. What is the relationship?
After you have the TI thing sorted out: Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
Finish carving prospectus up into thesis chapters
For 6/6:
Reply to Erika
Finish N COTM inset-style guide
Finish slope maps
Check equations in Scheidt et al. (2010)
use for TI calc
If still an insolation echo, look for papers that adapt Scheidt method for variable slope/aspect
Finish raster images: consider the color ramps and adjusting as needed to avoid swamping the signal on a few extreme pixel values: try using percentile symbology
Make an insolation map for the same time of day as the daytime thermal flight
plot insolation vs thermal measurement on per-pixel basis. What is the relationship?
After you have the TI thing sorted out: Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
For 5/30:
Finish: each image set, include inset-style guide - in process, doing slope map and waiting for feedback
Email Brent/Erika/Donna for image feedback
Redo thermal inertia calc to determine whether process was correct before
if process seems fine, check insolation and daytime thermal image -- appears to be an insolation time-of-day artifact
Raster images: consider the color ramps and adjusting as needed to avoid swamping the signal on a few extreme pixel values
start with visual inspection of similar/different patterns
Does the insolation map used make a big difference?
Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots (https://pro.arcgis.com/en/pro-app/latest/help/data/imagery/image-scatter-plot.htm) - rasters only have one band
Write interpretation
Create a shared Drive with SKN for the thesis document
Make a subfolder for each chapter
put in copies of prospectus, relevant figures
Start an outline/draft in each chapter folder
For 5/22:
Send close/med/wide view imagery sets to Erika and Brent, hopefully via Erika's OneDrive folder
For each set, include inset-style guide - in process
Add letters/numbers to grids -- make sure that lines keep their same names between views - in process
Put thermal inertia map, insolation map, and roughness map together as layers within GIS
start with visual inspection of similar/different patterns
Does the insolation map used make a big difference?
Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots - did something in arcpro, not sure if it's correct
Write interpretation - started it with the visual comparison; the graphs interpretation needs to be added
Lunar thermal model: increase number of time steps (decrease duration of step)
for full sun: depth to freezing? (what is freezing/sublimating temp for water on moon?) - Sublimation rate for ice on the moon (Andreas, 2007), https://nssdc.gsfc.nasa.gov/planetary/ice/ice_moon.html
For 75%, 50%, 25%, 1%?
Write summary/interpretation
For 5/9:
Finish map gridlines
Check on bottom (deep) temperature used in thermal code (lower boundary?) and how the rock and regolith are handled
Play with lunar thermal model to get stable output
for full sun: depth to freezing? (what is freezing/sublimating temp for water on moon?)
For 75%, 50%, 25%, 1%?
Make thermal inertia map using the day/night thermal images
<Hold: finish thermal inertia map questions below>
For 5/2:
Finish prospectus final draft
Maps (key thing: grids MUST stay consistent across zooms; Priority)
Bear Trap: make much wider view option to see lava flow context
COTM Caves: make a zoomed in version on the main set of caves; check Weng et al. for other cave coordinates; add maps for Needles, Last Chance, etc.
Cerro Grande: make series of zoomed-in maps; suggest targets of high interest
Grand View: zoom out
HHA: zoom in
The Breaks: zoom in on E-W chain and N-S chain of craters
N Robbers: zoom in (series)
Split: Zoom in and out
Northern COTM: make series
Remove vegetation, fill holes, and re-run roughness (3x3 and 7x7)
Check on bottom (deep) temperature used in thermal code (lower boundary?) and how the rock and regolith are handled
Play with lunar thermal model to get stable output
for full sun: depth to freezing? (what is freezing/sublimating temp for water on moon?)
For 75%, 50%, 25%, 1%?
Make thermal inertia map using the day/night thermal images (did something, not sure if it's right)
<Hold: finish thermal inertia map questions below>
For 4/25:
Geostats final project presentation and MATLAB project
6603 prospectus presentation
Work on prospectus revisions
Export map copies as pdfs and upload to Floe (server)
Make zoomed sections, too (Mud Lake and N COTM splits, in particular) - Mud Lake is done
Remove vegetation, fill holes, and re-run roughness (3x3 and 7x7)
Check on bottom (deep) temperature used in thermal code (lower boundary?) and how the rock and regolith are handled
Play with lunar thermal model to get stable output
for full sun: depth to freezing? (what is freezing temp for water on moon?)
For 75%, 50%, 25%, 1%?
Make thermal inertia map using the day/night thermal images
<Hold: finish thermal inertia map questions below>
For 4/18:
Clip NAIP images, overlay with 50 x 50 m grid, and upload to server by Monday morning
Combine caves imagery/info into a single file; email a copy to Brent
Roughness via 3x3 and 7x7
check on whether veg was removed, whether holes were filled
convert to multi-color ramp
Run thermal code (single point)
Make thermal inertia map using the day/night thermal images
Put thermal inertia map, insolation map, and roughness map together as layers within GIS
start with visual inspection of similar/different patterns
Does the insolation map used make a big difference?
Export per-pixel values of insolation, thermal inertia, and roughness. Plot them as XY scatterplots
<SKN: feedback on prospectus>
For 4/11:
Combine/trim NAIP images to target features of interest - in process
Finish last documentation for caves imagery
Roughness rasters; compile outputs into a ppt
replace all instances of cmd_inputs
run thermal code
Add grids to NAIP images (50 x 50 m - needs to be checked) - in process
Prospectus draft!
For 4/4:
Combine/trim NAIP images to target features of interest
Add documentation for caves imagery
Roughness rasters; compile outputs into a ppt
run thermal code
Add grids to NAIP images (50 x 50 m - needs to be checked)
For 3/28:
Check remaining NAIP groups
See if less hazy coverage in another year
Clean up NAIP folders
in each area, add an explanation file that includes an outline of where the NAIP images cover (use target polygons) and citation information
Keep running roughness rasters
For 3/14:
Finish revising poster and give awesomesauce presentation
continue to download and organize NAIP imagery for field areas (floe)
Calculate roughness rasters
Update python code for inputs
Run thermal code
Meet with CoSE IT for compiler installation (schedule visit this week for next week)
For 3/7:
Why those scales (0.1, 0.5, 1, and 2 m)?
Revise Methods section
Calculate roughness rasters
Contact geohelp@isu.edu for compiler fix (fortran90 for RMS and AreaRatio) - they don't know a lot of fortran
Run thermal code
Work with Brooks to install rugosity calculator (Brooks is available to do it today-Thursday)
download and organize NAIP imagery for field areas (floe) - working on it
Set up VPN
For 2/29:
Get rugosity tool installed (talk to Donna/Brooks) - talked with Donna and she told me Brooks can get it installed by next week
calculate roughness rasters
Get help from a PC user on fixing the matplotlib installation/path/whatever (working with Kyleigh on this; matplotlib is installed but now is giving me permission error)
Run thermal code
After running code, return to roughness and insolation vs TI correlation
Methods section to SKN by 8 pm Saturday (don't forget to include thermal stuff)
For 2/22:
Calculate roughness rasters (try using rugosity tool in Arc; will need to install)
Ask Kyleigh about how she installed her compiler(s)
Use Tyler's thesis as a guide to reading the TI code; add comments to the code (almost done)
depending on how this goes, try running the code
After running code, return to roughness and insolation vs TI correlation
Write and submit abstract for ISU Research Symposium (due 2/21)
For 2/15:
Put insolation rasters on the same color ramp
Extend cumulative to 24 hours and put on same color ramp
Re-load roughness rasters
Use Tyler's thesis as a guide to reading the TI code; add comments to the code
depending on how this goes, try running the code
After running code, return to roughness and insolation vs TI correlation
Add content to TI paper summary
Update Background, email SKN when re-uploaded
For 2/8:
Take a screengrab of the insolation error message
put instantaneous insolation images into a shared Google folder
run cumulative insolation examples and add to folder
Calculate thermal inertia (TI) of HHA dataset
organize roughness rasters alongside thermal inertia and insolation rasters
Correlate roughness - TI and insolation - TI
Read/summarize a TI or other temperature modeling paper cited in Paladino Ch 5
For 2/1:
Re-run insolation using the newly updated tool
Identify the contribution of local lava roughness to thermal inertia or insolation in the HHA dataset
Revise methodology plan to describe how you could use a 1D heat model like from Paladino to estimate regolith thickness. (Assume flat lava surface and a clean/dry regolith.) (Concentrate on Paladino)
For 1/25:
Keep going with insolation maps (add the summation outputs)
Put together a methodology plan (bullet points is fine) to identify the contribution of local lava roughness to thermal inertia or insolation in the HHA dataset
Put together a methodology plan to describe how you could use a 1D heat model like from Paladino to estimate regolith thickness. (Assume flat lava surface and a clean/dry regolith.)
Chat with Kyleigh
Do first draft of problem statement
For 1/18:
Revise Paladino summary to focus on what did(not) work and why
Revisit Karki thesis and make a list of questions
Do HHA insolation maps for 10 am, 2 pm, and 8 pm on July 1 (are you getting an instantaneous output or summation output?)
Read/summarize lunar PSR paper
For 12/18 (zoom):
Read/summarize Paladino dissertation chapter about lava tubes and thermal inertia
Meet with Kyleigh
Calculate time-specific insolation on HHA data
Read/summarize Karki thesis
For 12/5:
Read/summarize Paladino dissertation chapter about lava tubes and thermal inertia
Meet with Kyleigh
Calculate time-specific insolation on HHA data
Read/summarize Karki thesis
For 11/28:
Read/summarize Lopes-Gautier
Try to identify source of plot error
review proposal
Try to meet with Kyleigh about what she's been working on
For 11/7 (email update):
Focus on UAS stuff
Scan book (send to SKN) and return it to library (if time, start reading)
Plot U vs MgO and U vs SiO2; look to see if anything else is worth plotting (concentrate on trace)
For 10/31:
ILL request for Lopes-Gautier, R. M. (2022). Extraterrestrial lava flows. Active Lavas, 107-144.
Read/summarize Cao and Cai (2018)
Review geochem maps: label key features, check scale bar, reduce number of breaks in scale
For 10/24:
Read/summarize Theilig and Greeley (1986)
With Geochem file: pick 3-4 elements and make a heat map of their distribution (ignore actual contacts, etc., and just look for major trends)
For 10/17:
Read/summarize Magma Composition chapter in Encyc. of Volc.
Read/summarize Greeley (1982)
Revise planetary section of Hughes summary
For 10/10:
Read/summarize Magma Composition chapter in Encyc. of Volc.
Read/summarize Hughes et al. (2020)
(for next week's readings: Greeley (1982)?)
Study for Volc midterm
For 10/3:
Read/summarize Xu et al. (2020), Warren (1985)
Snag gear for field trip
For 9/26 (skipping Seminar week):
Look for paper on lunar highlands
Condense last week's summaries into <300 words each
For 9/12:
Read/Summarize: Spudis (2000) and Kilburn (2000) (see big book)
More social things
Email Kyleigh to schedule time to talk about existing datasets; compare to the proposed flight polygons
For 9/5:
Read/Summarize: Cai and Fa (2020), Neish et al. (2017); add text about project relevance
Do another social thing... in addition to the department cookout
Join IDEAS telecon
For 8/29:
Populate upper part of website (ex. photos, simple project summary, mid- to long-term goals, etc.)
Read IDEAS proposal, write ~1 paragraph summary (include any questions, critiques, etc.)
Read Hester's thesis and write summary
Do something fun/social unrelated to Geology
{SKN: bring bike to campus; send Hester's thesis and proposal}