Most of the landforms at Venus's surface are typical of low-viscosity basaltic volcanic rocks: broad flat plains, fields of small shield volcanoes, and immense central shield volcanoes (Ivanov & Head, 2013). Key PointĪ fundamental question about Venus is whether its highland areas, its tesserae, and the “continent” of Ishtar Terra and Maxwell Montes, are made of granitic (silica-rich) igneous rock (Gilmore et al., 2015 Gilmore et al., 2017 Hashimoto et al., 2008 Shellnutt, 2013). Thus, the available evidence suggests that Ovda Fluctus had an emplacement rheology consistent with a basaltic composition this result provides no support for hypotheses that Ovda Regio (a highlands tessera terrain) is composed of granitic rock. The margin of Ovda Fluctus is at significantly higher elevation than its center, a characteristic seen in basalt flows on Earth, but not on more silica-rich flows. Outlines of Ovda Fluctus flow lobes have fractal dimensions consistent with basaltic pahoehoe lavas. The high-altitude region of Ovda Fluctus is continuous with the lower-elevation portions: the change in radar properties does not represent different flows. The flow complex includes a portion at high altitude (~5 km above mean planetary radius) that has low radar backscatter and high radar emissivity compared with lower-altitude portions of the complex. The flow includes multiple flow lobes and at least two distinct flow units. Ovda Fluctus is a “festoon flow complex,” whose surface is rumpled into arcuate folds. Using Magellan radar data, we find that the radar properties (emissivity, roughness, and backscatter) of Ovda Fluctus are similar to those of the surrounding tessera, although the flow is smoother at multiple scales.

We examined its morphology and geologic setting to determine if its apparent emplacement rheology is consistent with silica-rich (e.g., rhyolitic) lava this has significant implications for the compositions of Venus's tesserae. Twin Kohmak 5 forma – (110K – 553K DAMAGE PER MAGAZINE)Ĭhelsea Lowthorp on Akvasto – 43.Ovda Fluctus (6.1°S, 95.5☎) is a lava flow complex on the equatorial tessera highlands of Ovda Regio, Venus.Vauban Prime – Excavation / Survival camp.Vauban Prime Void build (33sec Vortex & 18.4 m Bastille for 42sec).Exterminate, Sabotage and Mobile Defense missions can yield weapon parts, while Interception missions can reward parts every 4 Rounds and Defense every 20 waves.

Part LocationsĬertain Archwing missions can reward components for various Archwings and Archwing weapons upon completion.

Recommend bringing Enemy Radar Auras to find stragglers and Elytron Archwings with high power range and power strength to kill enemies through walls. Instead, you must rush around aggressively killing everything to end waves ASAP, this way the 20 waves can be completed in less time thus facing enemies of reasonable levels. Enemies this strong risk destroying the objectives in a single shot. A cautious and defensive approach staying by the objectives will take 40 min or longer, and you will see enemies over level 100 before reaching the weapon rewards at Wave 20.

The level of enemies at each wave is based on time in mission instead of on Wave number, as though it were a Survival mission. Corpus Defense on Neptune Salacia has a difficult enemy scaling property, which is probably a bug.

Where to get fluctus parts