Atai Mons, Venus, is classified as a large volcano yet diplays characteristics that are typical of coronae. Coronae are widespread volcano-tectonic features that are apparently unique to Venus. Detailed analysis of Atai Mons using photogeological and geophysical technigues illustrate that it has experienced a complex history and may still be active. We show that processes found at both coronae and large volcanoes have occurred throughout the history of Atai Mons with no definite temporal preference. It does not have an evolution that can be described simply as the evolution of one feature into another. These results suggest that large volcanoes and coronae are more intimately linked than previously thought, and that detailed mapping and gra...
Crustal plateaus and volcanic rises, major physiographic features on Venus, both formed over mantle ...
Magellan images confirm that volcanism is widespread and has been fimdamentally important in the for...
Magellan images show that small volcanoes (< 20 km in diameter) are ubiquitous in the plains of Venu...
This thesis reports the results of a study of volcanic processes at coronae on Venus. The Aglaonice ...
Abstract. Large-scale volcanism, in the form of areally extensive flow fields, is a previously unrec...
A great variety of tectonic and volcanic features have been documented on Venus. It is widely apprec...
A new analysis of the spatial relationships between volcanic features and rifts on Venus provides ne...
Coronae and novae are two examples of Venusian volcano-tectonic structure types. Both these structur...
Coronae and ovoids on Venus were first identified in Venera 15/16 data. They are distinctive and app...
Coronae and novae are two examples of Venusian volcano-tectonic structure types. Both these structur...
In the absence of global plate tectonics, mantle convection and plume–lithosphere interaction are th...
Coronae are large circular features on Venus, whose complex structure, with traces of tectonic and v...
Abstract Venus is known to have been volcanically resurfaced in the last third of solar system histo...
After a long hiatus due to competing tasks with the PI, mapping of Venus' Nepthys Mons Quadrangle (V...
The formation and evolution of coronae on Venus are thought to be the result of mantle upwellings ag...
Crustal plateaus and volcanic rises, major physiographic features on Venus, both formed over mantle ...
Magellan images confirm that volcanism is widespread and has been fimdamentally important in the for...
Magellan images show that small volcanoes (< 20 km in diameter) are ubiquitous in the plains of Venu...
This thesis reports the results of a study of volcanic processes at coronae on Venus. The Aglaonice ...
Abstract. Large-scale volcanism, in the form of areally extensive flow fields, is a previously unrec...
A great variety of tectonic and volcanic features have been documented on Venus. It is widely apprec...
A new analysis of the spatial relationships between volcanic features and rifts on Venus provides ne...
Coronae and novae are two examples of Venusian volcano-tectonic structure types. Both these structur...
Coronae and ovoids on Venus were first identified in Venera 15/16 data. They are distinctive and app...
Coronae and novae are two examples of Venusian volcano-tectonic structure types. Both these structur...
In the absence of global plate tectonics, mantle convection and plume–lithosphere interaction are th...
Coronae are large circular features on Venus, whose complex structure, with traces of tectonic and v...
Abstract Venus is known to have been volcanically resurfaced in the last third of solar system histo...
After a long hiatus due to competing tasks with the PI, mapping of Venus' Nepthys Mons Quadrangle (V...
The formation and evolution of coronae on Venus are thought to be the result of mantle upwellings ag...
Crustal plateaus and volcanic rises, major physiographic features on Venus, both formed over mantle ...
Magellan images confirm that volcanism is widespread and has been fimdamentally important in the for...
Magellan images show that small volcanoes (< 20 km in diameter) are ubiquitous in the plains of Venu...