I made a little lava material and it looks kind of how I want it, but there is a big problem when rendering it.
The material starts flickering and as soon as the camera is a certain distance away, it disappears completely.
It also seems depending on the viewing angle, because even further away, it satarts to show again as flickering.
If the camera is really up close, the flickering is mostly gone, but not completely.
I fiddled a bit with the bounds settings, but the problem still persists.
Just to test, I useda different mesh (a plane mesh from the engine content) and its giving me much better results.
So I think the mesh is the culprit afterall. The engine content mesh is however a bit low poly, so even with tesselation, the lava lacks somewhat of fidelity.
I think I will play aound with differently detailed meshes to find out whats best.
Download Lava Material
Download Zip 🔥 https://shoxet.com/2yGbna 🔥
My question is it possible to have some panning texure run thru my lava cracks? small movement
Currently have something working which pans a texure, but when I paint on my landscape
it paints like a blockshape. Its not masking out my main Tilling texture the (cracks)
Is this technical possible? How would you set this up? Big Thanks.
Thanks All, I made some more progress, but got some flow running thru my lava cracks it only looks strange like its transparant.
How could I have some more blending going on with these textures? Perhaps 2 fire textures. Thanks
Here is the node tree to add to the Emissive output of one of the layers - The OneMinus should attach to the B output of a Multiply with the A output of that Multiply set to the Diffuse texture for that layer and the input obviously coming from the Diffuse output of the main node. This will stop it from rendering under your Lava.
I had some results but I also noticed that EmissiveTexture is animating but then its
scalling is incorrect with this DifusseTexture03. As you know DiffuseTexture03 has its
own RelativeTilling does this mean you would need to assign to the EmissivePan tree?
Lava is molten or partially molten rock (magma) that has been expelled from the interior of a terrestrial planet (such as Earth) or a moon onto its surface. Lava may be erupted at a volcano or through a fracture in the crust, on land or underwater, usually at temperatures from 800 to 1,200 C (1,470 to 2,190 F). The volcanic rock resulting from subsequent cooling is also often called lava.
A lava flow is an outpouring of lava during an effusive eruption. (An explosive eruption, by contrast, produces a mixture of volcanic ash and other fragments called tephra, not lava flows.) The viscosity of most lava is about that of ketchup, roughly 10,000 to 100,000 times that of water. Even so, lava can flow great distances before cooling causes it to solidify, because lava exposed to air quickly develops a solid crust that insulates the remaining liquid lava, helping to keep it hot and inviscid enough to continue flowing.[1]
The word lava comes from Italian and is probably derived from the Latin word labes, which means a fall or slide.[2][3] An early use of the word in connection with extrusion of magma from below the surface is found in a short account of the 1737 eruption of Vesuvius, written by Francesco Serao, who described "a flow of fiery lava" as an analogy to the flow of water and mud down the flanks of the volcano (a lahar) after heavy rain.[4][5]
Solidified lava on the Earth's crust is predominantly silicate minerals: mostly feldspars, feldspathoids, olivine, pyroxenes, amphiboles, micas and quartz.[6] Rare nonsilicate lavas can be formed by local melting of nonsilicate mineral deposits[7] or by separation of a magma into immiscible silicate and nonsilicate liquid phases.[8]
Silicate lavas are molten mixtures dominated by oxygen and silicon, the most abundant elements of the Earth's crust, with smaller quantities of aluminium, calcium, magnesium, iron, sodium, and potassium and minor amounts of many other elements.[6] Petrologists routinely express the composition of a silicate lava in terms of the weight or molar mass fraction of the oxides of the major elements (other than oxygen) present in the lava.[9]
The silica component dominates the physical behavior of silicate magmas. Silicon ions in lava strongly bind to four oxygen ions in a tetrahedral arrangement. If an oxygen ion is bound to two silicon ions in the melt, it is described as a bridging oxygen, and lava with many clumps or chains of silicon ions connected by bridging oxygen ions is described as partially polymerized. Aluminium in combination with alkali metal oxides (sodium and potassium) also tends to polymerize the lava.[10] Other cations, such as ferrous iron, calcium, and magnesium, bond much more weakly to oxygen and reduce the tendency to polymerize.[11] Partial polymerization makes the lava viscous, so lava high in silica is much more viscous than lava low in silica.[10]
Because of the role of silica in determining viscosity and because many other properties of a lava (such as its temperature) are observed to correlate with silica content, silicate lavas are divided into four chemical types based on silica content: felsic, intermediate, mafic, and ultramafic.[12]
Felsic magmas can erupt at temperatures as low as 800 C (1,470 F).[16] Unusually hot (>950 C; >1,740 F) rhyolite lavas, however, may flow for distances of many tens of kilometres, such as in the Snake River Plain of the northwestern United States.[17]
Some silicate lavas have an elevated content of alkali metal oxides (sodium and potassium), particularly in regions of continental rifting, areas overlying deeply subducted plates, or at intraplate hotspots.[27] Their silica content can range from ultramafic (nephelinites, basanites and tephrites) to felsic (trachytes). They are more likely to be generated at greater depths in the mantle than subalkaline magmas.[28] Olivine nephelinite lavas are both ultramafic and highly alkaline, and are thought to have come from much deeper in the mantle of the Earth than other lavas.[29]
Lava viscosity determines the kind of volcanic activity that takes place when the lava is erupted. The greater the viscosity, the greater the tendency for eruptions to be explosive rather than effusive. As a result, most lava flows on Earth, Mars, and Venus are composed of basalt lava.[36] On Earth, 90% of lava flows are mafic or ultramafic, with intermediate lava making up 8% of flows and felsic lava making up just 2% of flows.[37] Viscosity also determines the aspect (thickness relative to lateral extent) of flows, the speed with which flows move, and the surface character of the flows.[13][38]
When highly viscous lavas erupt effusively rather than in their more common explosive form, they almost always erupt as high-aspect flows or domes. These flows take the form of block lava rather than a or phoehoe. Obsidian flows are common.[39] Intermediate lavas tend to form steep stratovolcanoes, with alternating beds of lava from effusive eruptions and tephra from explosive eruptions.[40] Mafic lavas form relatively thin flows that can move great distances, forming shield volcanoes with gentle slopes.[41]
In addition to melted rock, most lavas contain solid crystals of various minerals, fragments of exotic rocks known as xenoliths, and fragments of previously solidified lava. The crystal content of most lavas gives them thixotropic and shear thinning properties.[42] In other words, most lavas do not behave like Newtonian fluids, in which the rate of flow is proportional to the shear stress. Instead, a typical lava is a Bingham fluid, which shows considerable resistance to flow until a stress threshold, called the yield stress, is crossed.[43] This results in plug flow of partially crystalline lava. A familiar example of plug flow is toothpaste squeezed out of a toothpaste tube. The toothpaste comes out as a semisolid plug, because shear is concentrated in a thin layer in the toothpaste next to the tube and only there does the toothpaste behave as a fluid. Thixotropic behavior also hinders crystals from settling out of the lava.[44] Once the crystal content reaches about 60%, the lava ceases to behave like a fluid and begins to behave like a solid. Such a mixture of crystals with melted rock is sometimes described as crystal mush.[45]
Lava flow speeds vary based primarily on viscosity and slope. In general, lava flows slowly, with typical speeds for Hawaiian basaltic flows of 0.40 km/h (0.25 mph) and maximum speeds of 10 to 48 km/h (6 to 30 mph) on steep slopes.[37] An exceptional speed of 32 to 97 km/h (20 to 60 mph) was recorded following the collapse of a lava lake at Mount Nyiragongo.[37] The scaling relationship for lavas is that the average speed of a flow scales as the square of its thickness divided by its viscosity.[46] This implies that a rhyolite flow would have to be about a thousand times thicker than a basalt flow to flow at a similar speed.
The temperature of most types of molten lava ranges from about 800 C (1,470 F) to 1,200 C (2,190 F).[16] depending on the lava's chemical composition. This temperature range is similar to the hottest temperatures achievable with a forced air charcoal forge.[47] Lava is most fluid when first erupted, becoming much more viscous as its temperature drops.[13] 152ee80cbc
strange stories amazing facts free pdf download
meeting notes pdf free download