John M.C. Plane | |
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Born | South Africa |
Alma mater | University of Cambridge |
Known for | Chemistry of troposphere and mesosphere |
Awards |
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Scientific career | |
Fields | Atmospheric chemistry |
Institutions | |
Website | Official website |
John Maurice Campbell Plane, FRAS , FRSC , FRS is a British atmospheric chemist, currently Professor of Atmospheric Chemistry at the University of Leeds. His research investigates planetary atmospheres using a range of theoretical and experimental techniques. [1]
Plane was born in South Africa. He took an MA (1979) and a PhD (1983) at the University of Cambridge, where he also held a research fellowship. Later, he held academic appointments at the University of Miami and the University of East Anglia, before moving to the University of Leeds. [2]
Plane's research focuses on understanding the chemistry of planetary atmospheres (including Earth's) involving a combination of laboratory techniques (kinetics and photochemistry), atmospheric measurements (in situ and satellite remote sensing), and modelling at different scales. His research group studies four main areas: Earth's mesosphere (middle and upper atmosphere) and troposphere (lower atmosphere), the atmospheres of other planets, and interstellar chemistry (such as the formation of stardust). [1] Plane is particularly noted for his work on the chemistry of metals that ablate ("erode") from cosmic dust particles, such as meteoroids, as they enter the atmosphere. He is an expert on mesospheric metal chemistry, a pioneer of Differential Optical Absorption Spectroscopy (DOAS), and one of the developers of tropospheric iodine chemistry - a means of studying the composition of Earth's atmosphere. [3] He has authored over 240 peer-reviewed papers. [4]
Plane has received numerous honors and awards, including the Royal Society of Chemistry prize in Reaction Kinetics and Mechanisms (2005), a Royal Society of Chemistry Tilden Prize Lectureship (2006) ("for his outstanding contributions to our understanding of the chemistry of the troposphere and mesosphere through field measurements, laboratory experiments and theory"), [5] the National Science Foundation CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Lecture Prize (2007), and the European Geosciences Union Vilhelm Bjerknes Medal (2017) ("in recognition of his groundbreaking work in atmospheric chemistry"). [6] He was elected a Fellow of the American Geophysical Union in 2017. He is also a Fellow of the Royal Society of Chemistry and a Fellow of the Royal Astronomical Society, and was elected a Fellow of the Royal Society in 2020. [2] [4] In 2022, he was elected a member of the Academia Europaea. [7]
The stratosphere is the second-lowest layer of the atmosphere of Earth, located above the troposphere and below the mesosphere. The stratosphere is composed of stratified temperature zones, with the warmer layers of air located higher and the cooler layers lower. The increase of temperature with altitude is a result of the absorption of the Sun's ultraviolet (UV) radiation by the ozone layer, where ozone is exothermically photolyzed into oxygen in a cyclical fashion. This temperature inversion is in contrast to the troposphere, where temperature decreases with altitude, and between the troposphere and stratosphere is the tropopause border that demarcates the beginning of the temperature inversion.
The mesosphere is the third layer of the atmosphere, directly above the stratosphere and directly below the thermosphere. In the mesosphere, temperature decreases as altitude increases. This characteristic is used to define limits: it begins at the top of the stratosphere, and ends at the mesopause, which is the coldest part of Earth's atmosphere, with temperatures below −143 °C. The exact upper and lower boundaries of the mesosphere vary with latitude and with season, but the lower boundary is usually located at altitudes from 47 to 51 km above sea level, and the upper boundary is usually from 85 to 100 km.
The atmosphere of Earth is composed of a layer of gas mixture that surrounds the Earth's planetary surface, known collectively as air, with variable quantities of suspended aerosols and particulates, all retained by Earth's gravity. The atmosphere serves as a protective buffer between the Earth's surface and outer space, shields the surface from most meteoroids and ultraviolet solar radiation, keeps it warm and reduces diurnal temperature variation through heat retention, redistributes heat and moisture among different regions via air currents, and provides the chemical and climate conditions allowing life to exist and evolve on Earth.
An atmosphere is a layer of gasses that envelop an astronomical object, held in place by the gravity of the object. A planet retains an atmosphere when the gravity is great and the temperature of the atmosphere is low. A stellar atmosphere is the outer region of a star, which includes the layers above the opaque photosphere; stars of low temperature might have outer atmospheres containing compound molecules.
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