ARCHIVE
NMR solid state data.zip (1.68 MB)
ARCHIVE
FTIR after comminution.zip (304.95 kB)
ARCHIVE
FTIR scans of as received samples.zip (91.93 kB)
ARCHIVE
TGA composit data.zip (3 MB)
DATASET
paramagnetism data.xlsx (12.73 kB)
ARCHIVE
raw XPS vms files.zip (2.2 MB)
ARCHIVE
XPS data.zip (246.23 kB)
TEXT
README_data for Aeolian driven silicate comminution unlikely to be responsible for the rapid loss of Martian methane.txt (5.58 kB)
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Aeolian driven silicate comminution unlikely to be responsible for the rapid loss of Martian methane
Version 2 2021-12-06, 10:05
Version 1 2021-12-03, 14:06
dataset
posted on 2021-12-06, 10:05 authored by Graham PurvisGraham Purvis, Jon Telling, Corinne Wills, Casey Dixon, Lidija Šiller, Emmal Safi, john edgarA dataset in support of results published in Icarus entitled "Aeolian driven silicate comminution unlikely to be responsible for the rapid loss of Martian methane"
containing
-FTIR spectra
-X-ray photoelectron spectroscopy spectra
-Nuclear magnetic resonance spectra
-Thermogravimetric-digital scanning calorimetry-mass spectrometry
-paramagnetic measurmants
Funding
UK Space Agency Aurora grants ST/R001421/1
UK Engineering and Physical Sciences Research Council (EPSRC), on grant number NS/A000015/1
ST/S001484/1 (to J.T.).
History
UoA
- Earth Systems and Environmental Sciences
