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Training Guide in Surface Weather Observations - Multiple Choices

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1<br />

CU - Cumulus<br />

1<br />

Example 5-12. <strong>Multiple</strong> Layers Composed of CB and TCU.<br />

Layers composed of cumulonimbus or tower<strong>in</strong>g cumulus shall be identified by append<strong>in</strong>g the contraction<br />

CB or TCU, respectively. These are the only two cloud types appended to a sky condition layer. In the<br />

above example, if the CB and the TCU had been at the same level, only the CB would have been<br />

reported <strong>in</strong> the Sky Condition, that is, <strong>in</strong> column 10. However, a remark <strong>in</strong> column 14 would still be<br />

made to show the TCU’s location.<br />

5.2.3 Variable Sky Condition<br />

This term describes a condition when the reportable amount of a layer varies by one or more reportable<br />

values, e.g., SCT to BKN, OVC to BKN, FEW to SCT, etc.<br />

The variable sky condition remark is used to report two operationally significant sky conditions. A “V”<br />

is used to separate the variability between the two ranges. For example, a cloud layer vary<strong>in</strong>g between<br />

broken and overcast would be coded “BKN V OVC.” If there are several layers with the same sky<br />

condition amount, the layer height of the variable layer shall also be reported. For example, if there were<br />

two scattered layers reported, one at 500 feet, the other at 1,400 feet, and the layer at 1,400 feet is<br />

vary<strong>in</strong>g between scattered and broken the remark would be coded “SCT014 V BKN.”<br />

5.3 Cloud and Ceil<strong>in</strong>g Heights<br />

When it is possible to measure the height of clouds, determ<strong>in</strong><strong>in</strong>g the height is not much of a problem.<br />

However, you will have to estimate cloud heights quite often when the clouds are beyond the limits of<br />

the system available for measur<strong>in</strong>g them, when <strong>in</strong>struments are <strong>in</strong>operative, when clouds are scattered,<br />

etc. This estimation is especially difficult for the new observer.<br />

5-16

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