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Lecture notes

Commercial Pilot Licence (CPL) Meteorology - CMET

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PDF of typed notes of key terms and concepts required for the exam, as expressed in the Manual of Standards (MoS). Very convenient to carry around on the go! I passed all of my CPL, IREX and ATPL subject exams in the past 12 months first-time, with an average of 90. My lowest score through CPL w...

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  • February 13, 2021
  • 48
  • 2020/2021
  • Lecture notes
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COMMERCIAL PILOT LICENCE (CPL)
METEOROLOGY - CMET


THERMAL ENERGY
● Feeling of heat is the transfer of thermal energy
● Contained within any object with a temperature above absolute zero
● Transfer of energy flows from hot to cold


CONDUCTION
● Flow of heat via contact between two objects


CONVECTION
● Vertical movement of hot and cold due its buoyancy relative to the
surrounds
● Hot air is lighter than the surrounding air, and therefore rises
● Cold air is denser than the surrounding air, and therefore sinks


ADVECTION
● Horizontal movement of hot and cold
● Wind


RADIATION
● Flow of heat via electromagnetic radiation, without contact
● Can travel without an atmosphere


LATENT HEAT
● Flow of heat via phase change of an object
● Either absorbed into the object or released into the environment

,SPECIFIC HEAT
● Energy required to change its temperature by 1 degree
● High specific heat means a large amount of energy is required to
change its temperature
● Low specific heat means only a small amount of energy is required to
change its temperature


HEIGHT
● Vertical distance above a datum, usually above ground level


ALTITUDE
● Vertical distance above mean sea level


ELEVATION
● Vertical distance of some point on the ground, above mean sea level


QNH
● Air pressure at any point on the earth, measured at mean sea level


QFE
● Air pressure at field elevation, measured at some point on the ground


PRESSURE HEIGHT
● Vertical distance above the international standard atmosphere mean
sea level, 1013.25 hPA
● 1 hPA is lost for every 30 ft of height gained


ISA TEMPERATURE
● 15 degrees at mean sea level
● 2 degrees is lost for every 1,000 ft of height gained

,THE ATMOSPHERE
● 78% nitrogen, 20% oxygen, 2% carbon dioxide and other gases
● Broken up into layers defined by the behaviour of temperature with
increasing height
● Water vapour present in lower level of atmosphere in amounts
varying from trace to 3% of total mass


TROPOSPHERE
● First layer of the atmosphere
● Temperature decreases as height increases
● About 60,000 ft (18 km) over the equator and 30,000 ft (8 km) over
the poles
● Contains virtually all convection, water vapour, weather and clouds


TROPOPAUSE
● Boundary between the troposphere and stratosphere
● Marked by the change to an isothermal temperature lapse rate
● Convection of air weakens due to the converging buoyancy of the
surrounding air


STRATOSPHERE
● Second layer of the atmosphere
● Temperature is constant as height increases to a point, and then
temperature increases as height increases given the proximity to the
ozone
● Little to no vertical mixing of air due to the increase in the ambient
temperature preventing convection
● Only towering cumulus or cumulonimbus may be found here due to
very strong convection


ISOTHERMAL LAYER
● Temperature is constant as height increases

, SOLAR RADIATION
● Ozone gas absorbs large amounts of solar radiation, producing
temperatures similar to that on the ground
○ Concentrated at 50 km above ground

● Remaining can be reflected back to space from cloud tops
● Some is scattered by air particles, producing the blue colour of the
sky
● What’s left is arrives at the surface and may be absorbed or
reflected
● Equatorial regions receive radiation at a greater intensity than the
poles
○ Therefore equatorial regions have higher surface temperatures

○ During summer in the southern hemisphere, due to the tilt, the

most intense solar heating occurs south of the equator
○ During winter in the southern hemisphere, due to the tilt, the

most intense solar heating occurs north of the equator


TROPICAL CELL
● Equatorial regions with high surface temperatures heat the air via
conduction
● Hot air rises due to convection until it can rise no further
● Air moves laterally towards the poles
● Air begins to cool (not at the poles) and sinks to the surface


POLAR CELL
● Polar regions with low surface temperatures cool the air via
conduction
● Sinking cold air pushes air below it towards the equator
● Transversing air warms as it moves to lower latitudes
● Once warm enough, it rises and returns to the polar regions where it
then sinks

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