#LPSC2023
#LPSC2023

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Poster Session: Volcanoes! …From a Distance
Wednesday, March 15, 2023, 6:30 PM
iPosters/Gather.town
Crown D. A.*
Scheidt S. P.
Ruff S. W.
Rice J. R.
Chuang F. C.
Terrestrial Analog Studies of Volcanic Embayment Relationships: Implications for Interpretations of Volcanic Contacts on Mars
[#2710]
Terrestrial analog studies of basaltic lava flow fields in New Mexico provide constraints for interpretations of volcanic contacts on Mars.
Terrestrial analog studies of basaltic lava flow fields in New Mexico provide constraints for interpretations of volcanic contacts on Mars.
Crown D. A.*
Garry W. B.
Berman D. C.
Anderson S. W.
Scheidt S. P.
et al.
Mapping Martian Lava Flow Fields: Investigations of Pahoehoe-Like Flow Morphologies in the Tharsis and Elysium Volcanic Provinces
[#2269]
Mapping martian lava flow fields reveals the distribution, types, topographic attributes, and spatial and temporal contexts of pāhoehoe flow morphologies.
Mapping martian lava flow fields reveals the distribution, types, topographic attributes, and spatial and temporal contexts of pāhoehoe flow morphologies.
Keszthelyi L.*
Kerber L.
Fagents S. A.
Liu Y.
Using Fuzzy Logic to Classify Planetary Lava Flows Seen in Cross-Section
[#2691]
We are starting to see lava flows in cross-section up close. We present a systematic method for interpreting such observations.
We are starting to see lava flows in cross-section up close. We present a systematic method for interpreting such observations.
Wilson L.*
Head J. W.
Formation of Magma Reservoirs Supplying Volcanic Complexes on the Moon
[#1453]
We link small-volume eruptions in volcanic provinces on the Moon to the formation and evolution of reservoirs at the base of the crust.
We link small-volume eruptions in volcanic provinces on the Moon to the formation and evolution of reservoirs at the base of the crust.
Wilson L.*
Head J. W.
Eruption Conditions Deduced from the Extents of Pyroclastic Constructional Features Surrounding Volcanic Vents on the Moon
[#1469]
Diameters of lunar pyroclastic deposits are controlled by magma volatile contents and radial thickness variations measure magma volume eruption rates.
Diameters of lunar pyroclastic deposits are controlled by magma volatile contents and radial thickness variations measure magma volume eruption rates.
Ahmad A.*
Chaudhary H.
Nair A. M.
Mineralogical Analysis of Hesparian-Aged Regions of Ius Chasma, Melas Chasma and Capri Chasma of Valles Marineris
[#2003]
We carried out a comparative study based on mineralogical analysis across the Hesperian-aged region of three Chasmata: Ius Chasma, Melas Chasma, and Capri Chasma.
We carried out a comparative study based on mineralogical analysis across the Hesperian-aged region of three Chasmata: Ius Chasma, Melas Chasma, and Capri Chasma.
*presenter