Sentences with phrase «water surface conditions»

Winds at the time of the report were very light onshore providing us with warm and clear water surface conditions.

Winds at the time of the report were no wind providing us with glassy water surface conditions.

Winds at the time of the report were offshore providing us with semi glassy water surface conditions.

Winds at the time of the report were offshore providing us clear water surface conditions.

The winds at the time of the report were a very light onshore providing us with choppy water surface conditions.

Winds at the time of the report were no wind providing us with warm and clear water surface conditions.

Winds at the time of the report were no wind providing us with choppy water surface conditions.

Winds at the time of the report were gentle wind providing us with moved water surface conditions.

Winds at the time of the report were onshore providing us with choppy water surface conditions.

Winds at the time of the report on shore wind providing us with warm and clear water surface conditions.

Winds at the time of the report were offshore providing us with glassy water surface conditions.

Winds at the time of the report were gentle offshore providing us with glassy water surface conditions.

Not exact matches

For oil and gas companies that want to install drilling and pumping infrastructure there, continuous monitoring of conditions above, below and at the surface of the water will be integral, and right now drones are the only feasibly deployable technology that can collect and relay all that data in a cost - effective manner.

Under certain conditions, the warm water of the lower layer can reach the surface and melt the ice.

The name «water mould» refers to the fact that they thrive under conditions of high humidity and running surface water.

As for the increase in phosphorus content, it was caused by the phosphorus that in the summer of 2014 flowed in from the deep waters in the north of the Baltic Sea main basin and the phosphorus that was released from the Gulf of Finland's own seabed in the poor oxygen conditions and mixed with the surface layer during last winter.

Their moons, though, might have the right conditions for liquid surface water and therefore for life to emerge and evolve.

Under some conditions — particularly when CO2 - rich deep water wells up to the surface in the tropics — seawater also releases CO2 back into the air.

Current methods can estimate the size and temperature of an exoplanet planet in order to determine whether liquid water could exist on the planet's surface, believed to be one of the criteria for a planet hosting the right conditions for life.

In aqueous fluids, amino acid residues that have polar sidechains — components that can have a charge under certain physiological conditions or that participate in hydrogen bonding — tend to be located on the surface of the protein where they can interact with water, which has negatively and positively side charges to its molecule.

The team found that during Martian winter, conditions throughout the cold but humid nights would allow liquid water to be stable in the first 5 centimetres of the surface.

But the soil on Mars is known to host perchlorate salts, which lower the freezing point of water, meaning the chilly surface conditions are not an absolute barrier to liquid water.

They examined light adaptation mechanisms of visible - and IR - radiation - using phototrophs required for adapting to land habitats and found out that IR - using phototrophs struggle to adapt to changing light condition at the boundary of water and land surface.

Prospects for Venusian life have been dismissed because of harsh conditions on the planet's surface: there is no water, temperatures reach 477 °C and the atmospheric pressure is 92 times that on Earth's surface.

«It's an incredibly clever natural solution to this problem of how to deal with a water barrier on a surface it will change the way we think about developing bio-inspired adhesives that are safe and already optimised to work in conditions similar to those in the human body, as well as marine paints that stop barnacles from sticking.»

Brown researchers have compiled a detailed Indonesian climate record of the last 60,000 years, tracking telltale indicators in sedimentary cores: titanium levels (a marker for surface water runoff) and the carbon isotopes of leaf wax, a marker for plant varieties (grasses indicate dry conditions).

This enabled the research team to reconstruct, for the first time, a detailed picture of the environmental conditions at the ocean's surface, as well as in deeper water layers, over the last 30,000 years.

Experiments carried out in the OU Mars Simulation Chamber — specialised equipment, which is able to simulate the atmospheric conditions on Mars — reveal that Mars» thin atmosphere (about 7 mbar — compared to 1,000 mbar on Earth) combined with periods of relatively warm surface temperatures causes water flowing on the surface to violently boil.

The Iceland and Greenland Seas are among the only places worldwide where conditions are right and this heat exchange is able to change the ocean's density enough to cause the surface waters to sink.

When the planet K2 - 18b was first discovered in 2015, it was found to be orbiting within the star's habitable zone, making it an ideal candidate to have liquid surface water, a key element in harbouring conditions for life as we know it.

Such conditions would make photosynthesis impossible, both for the algae in the surface water directly under the ice and those dwelling deeper in the ice close to the ice - water interface.

The tanks held seawater with a range of pH levels reflecting current conditions as well as the lower pH occasionally encountered in Puget Sound when deep water wells up near the surface.

Multiple lines of evidence point to past flows of water across the Martian surface, but conditions on the planet now preclude the existence of liquid water.

She found that in anoxic conditions, when there is no oxygen in the bottom layers of the Chesapeake Bay's waters, dissolved methane built up, probably coming from the mud, and when storms mixed up the invisible layers of the Bay's waters, the methane made it to the surface and into the atmosphere.

The resource geologist examined the possibility of this middle way, by calculating the chemical solubility of the precious metal in surface water under the prevailing atmospheric and climatic conditions.

For example, scientists have found that El Niño and La Niña, the periodic warming and cooling of surface waters in the central and eastern tropical Pacific Ocean, are correlated with a higher probability of wet or dry conditions in different regions around the globe.

In normal, non-El Niño conditions, Pacific trade winds near the equator blow from east to west, moving warm surface water with them.

The water - restricted conditions that exist on Mars would make it difficult for Earth - like life to exist near the surface of the planet.

So far, these early results showed that physical conditions where the air and the ocean interact must be a vital part of any successful hurricane forecasting model and would help explain, and predict, how a storm might intensify as it moves through across the water based on the physical stress at the ocean's surface.

With no water left on the surface, carbon dioxide built up in the atmosphere, leading to a so - called runaway greenhouse effect that created present conditions.

Organisms that have evolved in environments that have little if any change in environmental conditions, for example, may not be able to adapt well if currents increasingly mix warm surface waters down to the seafloor.

«This is the first exoplanet that really has the right conditions for water to exist in liquid form on its surface.»

As Jake Lanphere, a UC Riverside graduate student who co-authored the paper, which was published in the journal Environmental Engineering Science («Stability and Transport of Graphene Oxide Nanoparticles in Groundwater and Surface Water»), explained to Nanoclast in an email interview: «Other studies have looked at ideal lab conditions that do not necessarily reflect the conditions one might find in aquatic environments.

Satellites «make their best guess» from 400 kilometers up, Vass says, and can track only conditions near the water's surface, but the gliders «feel the full breadth of the current.»

All experiments were carried out in laboratory conditions where ambient temperature was maintained around 23 °C, so as not to vary the surface tension of water.

More importantly, the first one, called Kapteyn b, was found to lie inside its star habitable zone where conditions are just right for liquid water to exist on its surface.

A stunning claim that 40 percent of our galaxy's 160 billion red dwarf stars have plus - sized Earths orbiting the right distance for liquid water to exist on their surfaces, a condition believed to be necessary for life.

But conditions that allowed for the presence of liquid water on the surface of Mars must have lasted for at least 10,000 years, Barnhart said.

«It's hard to study surfaces under water because most available surface science techniques require vacuum conditions, under which water evaporates or freezes,» explains Geiger.

During normal conditions, trade winds blow to the west across the tropical Pacific Ocean, piling up warm surface water in the western Pacific, and cold, deeper water rises up, or upwells, off the west coast of South America.