Mt. Etna, Italy Lava Flows from Remote Sensing
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remote sensing Mt. Etna lava flows↗
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Results for “LAVA”
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Recent Advancements in LAVA for Jet, Rotor-Blade and Fan Noise Prediction
No abstract available
Fan Noise↗
Probing Putative Biomarker Assignments in SEM Imagery from BRAILLE Investigations at Lava Beds National Monument (N. CA, USA) Using Machine Learning Tools
No abstract available
machine learning; microscopy↗
Average VNIR reflectance: A rapid, sample-free method to estimate glass content and crystallinity of fresh basaltic lava
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E. Rader↗
Assessing Lava Flow Subpixel Surface Roughness and Particle Size Distribution for Improved Thermal Inertia Interpretations
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Christine Simurda↗
Adaptation of a Thermorheological Lava Flow Model for Venus Conditions
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Ian. T. W. Flynn↗
Dynamics of the December 2020 Ash‐Poor Plume Formed by Lava‐Water Interaction at the Summit of Kīlauea Volcano, Hawaiʻi
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Ryan C. Cahalan↗
Synthetic analogs for lava flows on the surface of Mercury: A mid-infrared study
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Andreas Morlok↗
Determining Emplacement Conditions and Vent Locations for Channelized Lava Flows Southwest of Arsia Mons
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I. T. W. Flynn↗
Viscosity of lunar lavas
Synthetic silicate liquid viscosity with lunar rock composition compared with volcanic rock on earth
Mcbirney, A. R.↗
Paleomagnetism of Tertiary and recent lavas of Israel
Geomagnetic reversals in volcanic flows, computing paleomagnetic pole positions similar to Tertiary rocks
Helsley, C. E.↗
Lava tubes of the Cave Basalt, Mount St. Helens, Washington.
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Greeley, R.↗
The petrochemistry of a unique cordierite-bearing lava from St. Helena Island, South Atlantic
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Ridley, W. I.↗
Lava flows in Mare Imbrium - An evaluation of anomalously low earth-based radar reflectivity
The surface of Mare Imbrium contains some of the most distinct red-blue colorimetric boundaries and depolarized 70-cm wavelength-reflectivity variations on the near side of the moon. The weakest levels of both 3.8-cm and 70-cm reflectivity within Imbrium are confined to spectrally blue regional mare surfaces that can be recognized as stratigraphically unique flow surfaces. Frequency distributions of the 70-cm polarized and depolarized radar-return power for five mare surfaces within the basin indicate that signal absorption, and probably ilmenite content, increases generally from the beginning of the Imbrium Period to the end of the Eratosthenian Period with slight reversal between the end of the Imbrium and beginning of the Eratosthenian. TiO2 calibrated radar-reflectivity curves can be utilized for lunar-maria geochemical mapping in the same manner as the TiO2 calibrated spectral-reflectivity curves of Charette et al. (1974).
Schaber, G. D.↗