Individual lava flow thicknesses in oceanus procellarum and mare serenitatis determined from clementine multispectral data
- DOI
- 10.1016/j.icarus.2010.05.010
- Published
- 2010-09-04
- Container
- Icarus
- Publisher
- Not recorded
- Open access
- yes
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Cite this work
BibTeX
@article{allodium:10.1016/j.icarus.2010.05.010,
title = {Individual lava flow thicknesses in oceanus procellarum and mare serenitatis determined from clementine multispectral data},
author = {Shoshana Z. Weider and Ian A. Crawford and Katherine H. Joy},
year = {2010},
journal = {Icarus},
doi = {10.1016/j.icarus.2010.05.010},
url = {https://doi.org/10.1016/j.icarus.2010.05.010}
}RIS
TY - JOUR TI - Individual lava flow thicknesses in oceanus procellarum and mare serenitatis determined from clementine multispectral data AU - Shoshana Z. Weider AU - Ian A. Crawford AU - Katherine H. Joy PY - 2010 JO - Icarus DO - 10.1016/j.icarus.2010.05.010 UR - https://doi.org/10.1016/j.icarus.2010.05.010 ER -
APA
Weider, S. Z., Crawford, I. A., & Joy, K. H. (2010). Individual lava flow thicknesses in oceanus procellarum and mare serenitatis determined from clementine multispectral data. Icarus. https://doi.org/10.1016/j.icarus.2010.05.010
Source records
- hal · retrieved 2026-09-25T18:31:05.418Z