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Cumulus mediocris cloud

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Cumulus mediocris is a specific type of cloud within the cumulus genus. It exists at both low and middle levels of the atmosphere. These clouds are defined by having some vertical extent, meaning they grow upward. They are notably taller than the smaller cumulus humilis clouds. When the sun shines on them, they appear brilliantly white. However, the undersides of these clouds usually look dark.

Thermal column
Thermal column

The formation of these clouds relies on a process called convection. This process begins with thermal air columns. These are pockets of air that are warmer than the surrounding atmosphere. Because of ground surface irregularities, these air pockets become less dense. This lower density makes the air buoyant, so it floats upward. As these air pockets rise, the air begins to cool. Eventually, the air reaches its dew point. This is the point where water vapor condenses into liquid droplets. This condensation first creates small cumulus humilis clouds. If the thermals are powerful enough, they continue pushing upward. This extra growth transforms the small clouds into cumulus mediocris.

Thermal column
Thermal column

Cumulus mediocris clouds can also form through the transformation of other cloud types. They may result from a partial transformation of altocumulus or stratocumulus clouds. In some cases, they can form from a complete transformation of stratus or stratocumulus clouds. Scientists also look for specific features attached to these clouds. You might see a pileus, which is a cap cloud. Other features include a velum, or apron cloud, and an arcus, known as a shelf cloud. A tuba, or vertical column, can also appear.

There are specific varieties and patterns that observers can identify. One pattern-based variety is called Cumulus radiatus. In this variety, individual clouds arrange themselves into parallel rows. These formations are known as "cloud streets." These streets align themselves approximately parallel to the direction of the wind.

Weather forecasting often involves watching how these clouds behave. Cumulus mediocris are common in the advance of a cold front. They also appear during unstable atmospheric conditions, such as an area of low pressure. These clouds generally do not produce heavy precipitation. They might produce very light intensity rain or show features like virga. Virga refers to precipitation that falls but evaporates before hitting the ground. Some may even form Cumulus praecipitato clouds.

However, these clouds serve as a warning for more intense weather. They can further develop into much larger cloud types. They may grow into cumulus congestus or even cumulonimbus clouds. These larger clouds are capable of producing heavy precipitation and severe storms. If you see cumulus mediocris in the morning or early afternoon, pay attention. Their presence indicates significant atmospheric instability. This instability often leads to thunderstorms later in the afternoon or evening.

Organizations use standardized codes to classify these clouds for science. The World Meteorological Organization codes cumulus mediocris as CL2. Sometimes, a cloud might show a feature called pannus. This is a supplementary feature seen with precipitating clouds. Usually, the code CL7 is used to identify pannus. However, if the cloud has significant vertical development, the CL2 code is used instead. This helps meteorologists accurately track the growth and type of the cloud system.

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