Add to ORKGSurface features on the flanks of Martian shield volcanoes photographed by Mariner 9 are identified as lava flow channels, rift zones, and partly collapsed lava tubes by comparisons with similar structures on the flanks of Mauna Loa shield volcano, Hawaii. From these identifications, the composition of the Martian lava flows is interpreted to be basaltic, with viscosities ranging from those of fluid pahoehoe to more viscous aa
We present a theoretical treatment of the ascent, emplacement, and eruption of magma on Mars. Becaus...
The morphology and topography of volcanic landforms provide critical information to the investigatio...
In the southeastern part of the Elysium region is a unit that exhibits little texture and a generall...
Martian volcanism is reviewed. It is emphasized that lava plains constitute the major type of effusi...
Channels and valleys were known on the Martian volcanoes since their discovery by the Mariner 9 miss...
Despite the difference in size Martian and Hawaiian volcanoes have numerous characteristics in commo...
The long lava flows of Mauna Loa, Hawaii have been cited as Earth's closed analogs to the large Mart...
A ground examination is made of lave tubes and channels. The surface morphology and the changes note...
Several remote sensing techniques have been developed to determine various properties of lava flows....
Extensive changes occurred after the initial observations (Greeley, 1971) of lava tube and channel f...
Huge volcanoes with diameters of >>100 km are well known from Mars. However, the planet‘s two large...
The dynamics of lava flow movement are controlled by the fluid interior. Crust, solids, and nondefor...
Volcanism has played a significant role throughout Mars’ geologic history. Extensive lava flows are ...
Tyrrhena Patera (TP) (22 degrees S, 253.5 degrees W), a large, low-relief volcano located in the anc...
Abstract: Lava tubes form when narrow lava channels crust over, build levees which arch over the cha...
We present a theoretical treatment of the ascent, emplacement, and eruption of magma on Mars. Becaus...
The morphology and topography of volcanic landforms provide critical information to the investigatio...
In the southeastern part of the Elysium region is a unit that exhibits little texture and a generall...
Martian volcanism is reviewed. It is emphasized that lava plains constitute the major type of effusi...
Channels and valleys were known on the Martian volcanoes since their discovery by the Mariner 9 miss...
Despite the difference in size Martian and Hawaiian volcanoes have numerous characteristics in commo...
The long lava flows of Mauna Loa, Hawaii have been cited as Earth's closed analogs to the large Mart...
A ground examination is made of lave tubes and channels. The surface morphology and the changes note...
Several remote sensing techniques have been developed to determine various properties of lava flows....
Extensive changes occurred after the initial observations (Greeley, 1971) of lava tube and channel f...
Huge volcanoes with diameters of >>100 km are well known from Mars. However, the planet‘s two large...
The dynamics of lava flow movement are controlled by the fluid interior. Crust, solids, and nondefor...
Volcanism has played a significant role throughout Mars’ geologic history. Extensive lava flows are ...
Tyrrhena Patera (TP) (22 degrees S, 253.5 degrees W), a large, low-relief volcano located in the anc...
Abstract: Lava tubes form when narrow lava channels crust over, build levees which arch over the cha...
We present a theoretical treatment of the ascent, emplacement, and eruption of magma on Mars. Becaus...
The morphology and topography of volcanic landforms provide critical information to the investigatio...
In the southeastern part of the Elysium region is a unit that exhibits little texture and a generall...