The mesosphere (/ˈmɛsəˌsfɪər,ˈmɛz-,ˈmiːsə-,-zə-/;[1] from Ancient Greekμέσος (mésos) 'middle', and -sphere) 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 its limits: it begins at the top of the stratosphere (sometimes called the stratopause), and ends at the mesopause, which is the coldest part of Earth's atmosphere, with temperatures below −143 °C (−225 °F; 130 K). The exact upper and lower boundaries of the mesosphere vary with latitude and with season (higher in winter and at the tropics, lower in summer and at the poles), but the lower boundary is usually located at altitudes from 50 to 65 km (31 to 40 mi; 164,000 to 213,000 ft) above sea level, and the upper boundary (the mesopause) is usually from 85 to 100 km (53 to 62 mi; 279,000 to 328,000 ft).[2][3][4][5]
Earth's atmosphere as it appears from space, as bands of different colours at the horizon. From the bottom, afterglow illuminates the troposphere in orange with silhouettes of clouds, and the stratosphere in white and blue. Next the mesosphere (pink area) extends to just below the edge of space at one hundred kilometers and the pink line of airglow of the lower thermosphere (dark), which hosts green and red aurorae over several hundred kilometers.
Diagram showing the five primary layers of the Earth's atmosphere: exosphere, thermosphere, mesosphere, stratosphere, and troposphere. From Earth's surface to the top of the stratosphere (50 km) is just under 1% of Earth's radius.
The stratosphere and mesosphere are sometimes collectively referred to as the "middle atmosphere",[6] which spans altitudes approximately between 12 and 80 km (7.5 and 49.7 mi) above Earth's surface. The mesopause, at an altitude of 80–90 km (50–56 mi), separates the mesosphere from the thermosphere—the second-outermost layer of Earth's atmosphere. This is the turbopause, below which different chemical species are well-mixed due to turbulent eddies. Above this level the atmosphere becomes non-uniform because the scale heights of different chemical species differ according to their molecular masses.
The term near space is also sometimes used to refer to altitudes within the mesosphere. This term does not have a technical definition, but typically refers to the region roughly between the Armstrong limit (about 62,000 ft or 19 km, above which humans require a pressure suit in order to survive) and the Kármán line (where astrodynamics must take over from aerodynamics in order to achieve flight); or, by another definition, to the space between the highest altitude commercial airliners fly at (about 40,000 ft (12.2 km)) and the lowest perigee of satellites being able to orbit the Earth (about 45 mi (73 km)). Some sources distinguish between the terms "near space" and "upper atmosphere", so that only the layers closest to the Kármán line are described as "near space".
Within the mesosphere, temperature decreases with increasing height, due to decreasing absorption of solar radiation by the rarefied atmosphere and increasing cooling by CO2radiative emission. The top of the mesosphere, called the mesopause, is the coldest part of Earth's atmosphere.[7] Temperatures in the upper mesosphere fall as low as about −100 °C (173 K; −148 °F),[8] varying according to latitude and season.
The main most important features in this region are strong zonal (East-West) winds, atmospheric tides, internal atmospheric gravity waves (commonly called "gravity waves"), and planetary waves. Most of these tides and waves start in the troposphere and lower stratosphere, and propagate to the mesosphere. In the mesosphere, gravity-wave amplitudes can become so large that the waves become unstable and dissipate. This dissipation deposits momentum into the mesosphere and largely drives global circulation.
Noctilucent clouds are located in the mesosphere. The upper mesosphere is also the region of the ionosphere known as the D layer, which is only present during the day when some ionization occurs with nitric oxide being ionized by Lyman series-alpha hydrogen radiation. The ionization is so weak that when night falls, and the source of ionization is removed, the free electron and ion form back into a neutral molecule.
A 5 km (3.1 mi; 16,000 ft) deep sodium layer is located between 80–105 km (50–65 mi; 262,000–344,000 ft). Made of unbound, non-ionized atoms of sodium, the sodium layer radiates weakly to contribute to the airglow. The sodium has an average concentration of 400,000 atoms per cubic centimetre. This band is regularly replenished by sodium sublimating from incoming meteors. Astronomers have begun utilizing this sodium band to create "guide stars" as part of the adaptive optical correction process used to produce ultra-sharp ground-based observations.[9] Other metal layers, e.g. iron and potassium, exist in the upper mesosphere/lower thermosphere region as well.
Beginning in October 2018,[10] a distinct type of aurora has been identified, originating in the mesosphere. Often referred to as 'dunes' due to their resemblance to sandy ripples on a beach, the green undulating lights extend toward the equator. They have been identified as originating about 96 km (60 mi; 315,000 ft) above the surface. Since auroras are caused by ultra-high-speed solar particles interacting with atmospheric molecules, the green color of these dunes has tentatively been explained by the interaction of those solar particles with oxygen molecules. The dunes therefore occur where mesospheric oxygen is more concentrated.[11]
Millions of meteors enter the Earth's atmosphere, averaging 40,000 tons per year.[12] The ablated material, called meteoric smoke, is thought to serve as condensation nuclei for noctilucent clouds.
Exploration
The mesosphere lies above altitude records for aircraft,[13] while only the lowest few kilometers are accessible to balloons, for which the altitude record is 53.0 kilometres (32.9 mi).[14] Meanwhile, the mesosphere is below the minimum altitude for orbitalspacecraft due to high atmospheric drag.[15][16][17] It has only been accessed through the use of sounding rockets, which are only capable of taking mesospheric measurements for a few minutes per mission.[18] As a result, it is the least-understood part of the atmosphere, resulting in the humorous moniker ignorosphere.[19][20] The presence of red sprites and blue jets (electrical discharges or lightning within the lower mesosphere), noctilucent clouds, and density shears within this poorly understood layer are of current scientific interest.
An astronaut onboard the International Space Station observes lightning at the horizon extending into the mesosphere as red sprite just below the line of airglow.
Noctilucent clouds (not to be mistaken with the slightly higher up airglow), at the upper edge of the mesosphere.
^"Middle atmosphere". www.antarctica.gov.au. Retrieved 17 June 2018.
^Venkat Ratnam, M.; Patra, A. K.; Krishna Murthy, B. V. (25 March 2010). "Tropical mesopause: Is it always close to 100 km?". Journal of Geophysical Research. 115 (D6): D06106. Bibcode:2010JGRD..115.6106V. doi:10.1029/2009jd012531. ISSN 0148-0227.
^"The Mesosphere - overview". scied.ucar.edu. UCAR Center for Science Education. Retrieved 17 June 2018.
^von Zahn, U.; Höffner, J.; Eska, V.; Alpers, M. (1 November 1996). "The mesopause altitude: Only two distinctive levels worldwide?". Geophysical Research Letters. 23 (22): 3231–34. Bibcode:1996GeoRL..23.3231V. doi:10.1029/96gl03041. ISSN 0094-8276.
^"Middle Atmosphere Meteorology". atmos.washington.edu. University of Washington. Retrieved 19 December 2018.
mesosphere, this, article, about, atmospheric, layer, other, uses, disambiguation, mesosphere, ɪər, from, ancient, greek, μέσος, mésos, middle, sphere, third, layer, atmosphere, directly, above, stratosphere, directly, below, thermosphere, mesosphere, temperat. This article is about the atmospheric layer For other uses see Mesosphere disambiguation The mesosphere ˈ m ɛ s e ˌ s f ɪer ˈ m ɛ z ˈ m iː s e z e 1 from Ancient Greek mesos mesos middle and sphere 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 its limits it begins at the top of the stratosphere sometimes called the stratopause and ends at the mesopause which is the coldest part of Earth s atmosphere with temperatures below 143 C 225 F 130 K The exact upper and lower boundaries of the mesosphere vary with latitude and with season higher in winter and at the tropics lower in summer and at the poles but the lower boundary is usually located at altitudes from 50 to 65 km 31 to 40 mi 164 000 to 213 000 ft above sea level and the upper boundary the mesopause is usually from 85 to 100 km 53 to 62 mi 279 000 to 328 000 ft 2 3 4 5 Earth s atmosphere as it appears from space as bands of different colours at the horizon From the bottom afterglow illuminates the troposphere in orange with silhouettes of clouds and the stratosphere in white and blue Next the mesosphere pink area extends to just below the edge of space at one hundred kilometers and the pink line of airglow of the lower thermosphere dark which hosts green and red aurorae over several hundred kilometers Diagram showing the five primary layers of the Earth s atmosphere exosphere thermosphere mesosphere stratosphere and troposphere From Earth s surface to the top of the stratosphere 50 km is just under 1 of Earth s radius The stratosphere and mesosphere are sometimes collectively referred to as the middle atmosphere 6 which spans altitudes approximately between 12 and 80 km 7 5 and 49 7 mi above Earth s surface The mesopause at an altitude of 80 90 km 50 56 mi separates the mesosphere from the thermosphere the second outermost layer of Earth s atmosphere This is the turbopause below which different chemical species are well mixed due to turbulent eddies Above this level the atmosphere becomes non uniform because the scale heights of different chemical species differ according to their molecular masses The term near space is also sometimes used to refer to altitudes within the mesosphere This term does not have a technical definition but typically refers to the region roughly between the Armstrong limit about 62 000 ft or 19 km above which humans require a pressure suit in order to survive and the Karman line where astrodynamics must take over from aerodynamics in order to achieve flight or by another definition to the space between the highest altitude commercial airliners fly at about 40 000 ft 12 2 km and the lowest perigee of satellites being able to orbit the Earth about 45 mi 73 km Some sources distinguish between the terms near space and upper atmosphere so that only the layers closest to the Karman line are described as near space Contents 1 Temperature 2 Dynamic features 3 Exploration 4 Phenomena in mesosphere and near space 5 See also 6 References 7 External linksTemperature EditWithin the mesosphere temperature decreases with increasing height due to decreasing absorption of solar radiation by the rarefied atmosphere and increasing cooling by CO2 radiative emission The top of the mesosphere called the mesopause is the coldest part of Earth s atmosphere 7 Temperatures in the upper mesosphere fall as low as about 100 C 173 K 148 F 8 varying according to latitude and season Dynamic features Edit Afterglow of the troposphere orange the stratosphere blue and the mesosphere dark at which atmospheric entry begins leaving smoke trails such as in this case of a spacecraft reentry The main most important features in this region are strong zonal East West winds atmospheric tides internal atmospheric gravity waves commonly called gravity waves and planetary waves Most of these tides and waves start in the troposphere and lower stratosphere and propagate to the mesosphere In the mesosphere gravity wave amplitudes can become so large that the waves become unstable and dissipate This dissipation deposits momentum into the mesosphere and largely drives global circulation Noctilucent clouds are located in the mesosphere The upper mesosphere is also the region of the ionosphere known as the D layer which is only present during the day when some ionization occurs with nitric oxide being ionized by Lyman series alpha hydrogen radiation The ionization is so weak that when night falls and the source of ionization is removed the free electron and ion form back into a neutral molecule A 5 km 3 1 mi 16 000 ft deep sodium layer is located between 80 105 km 50 65 mi 262 000 344 000 ft Made of unbound non ionized atoms of sodium the sodium layer radiates weakly to contribute to the airglow The sodium has an average concentration of 400 000 atoms per cubic centimetre This band is regularly replenished by sodium sublimating from incoming meteors Astronomers have begun utilizing this sodium band to create guide stars as part of the adaptive optical correction process used to produce ultra sharp ground based observations 9 Other metal layers e g iron and potassium exist in the upper mesosphere lower thermosphere region as well Beginning in October 2018 10 a distinct type of aurora has been identified originating in the mesosphere Often referred to as dunes due to their resemblance to sandy ripples on a beach the green undulating lights extend toward the equator They have been identified as originating about 96 km 60 mi 315 000 ft above the surface Since auroras are caused by ultra high speed solar particles interacting with atmospheric molecules the green color of these dunes has tentatively been explained by the interaction of those solar particles with oxygen molecules The dunes therefore occur where mesospheric oxygen is more concentrated 11 Millions of meteors enter the Earth s atmosphere averaging 40 000 tons per year 12 The ablated material called meteoric smoke is thought to serve as condensation nuclei for noctilucent clouds Exploration EditThe mesosphere lies above altitude records for aircraft 13 while only the lowest few kilometers are accessible to balloons for which the altitude record is 53 0 kilometres 32 9 mi 14 Meanwhile the mesosphere is below the minimum altitude for orbital spacecraft due to high atmospheric drag 15 16 17 It has only been accessed through the use of sounding rockets which are only capable of taking mesospheric measurements for a few minutes per mission 18 As a result it is the least understood part of the atmosphere resulting in the humorous moniker ignorosphere 19 20 The presence of red sprites and blue jets electrical discharges or lightning within the lower mesosphere noctilucent clouds and density shears within this poorly understood layer are of current scientific interest On February 1 2003 Space Shuttle Columbia broke up on reentry at about 62 km 39 mi altitude in the lower mesosphere killing all seven crew members Phenomena in mesosphere and near space Edit An astronaut onboard the International Space Station observes lightning at the horizon extending into the mesosphere as red sprite just below the line of airglow Noctilucent clouds not to be mistaken with the slightly higher up airglow at the upper edge of the mesosphere Airglow Atmospheric tides Ionosphere Meteors Noctilucent clouds Polar aurora Sprite lightning Upper atmospheric lightning Transient luminous event See also EditAeronomy Amateur radio high altitude ballooning Geospace High altitudeReferences Edit mesosphere Dictionary com Unabridged Online n d Middle atmosphere www antarctica gov au Retrieved 17 June 2018 Venkat Ratnam M Patra A K Krishna Murthy B V 25 March 2010 Tropical mesopause Is it always close to 100 km Journal of Geophysical Research 115 D6 D06106 Bibcode 2010JGRD 115 6106V doi 10 1029 2009jd012531 ISSN 0148 0227 The Mesosphere overview scied ucar edu UCAR Center for Science Education Retrieved 17 June 2018 von Zahn U Hoffner J Eska V Alpers M 1 November 1996 The mesopause altitude Only two distinctive levels worldwide Geophysical Research Letters 23 22 3231 34 Bibcode 1996GeoRL 23 3231V doi 10 1029 96gl03041 ISSN 0094 8276 Middle Atmosphere Meteorology atmos washington edu University of Washington Retrieved 19 December 2018 IUPAC Compendium of Chemical Terminology 2nd ed the Gold Book 1997 Online corrected version 2006 mesosphere doi 10 1351 goldbook M03855 Mesosphere Wayback Machine Archive Atmosphere Climate amp Environment Information ProgGFKDamme UK Department for Environment Food and Rural Affairs archived from the original on 1 July 2010 retrieved 14 November 2011 Martin Enderlein et al ESO s Very Large Telescope sees four times first light Laser Focus World July 2016 pp 22 24 The dunes were first spotted by photographers in Finland and Sweden Wu Katherine J A New Type of Aurora Ripples Across the Sky in Horizontal Green Dunes Smithsonian Magazine 29 January 2020 Leinert C Gruen E 1990 Interplanetary Dust Physics and Chemistry in Space R Schwenn and E Marsch eds Springer Verlag pp 204 275 Powered Aeroplanes World Records Federation Aeronautique Internationale Archived from the original on 11 September 2016 Retrieved 31 August 2016 Research on Balloon to Float over 50 km Altitude Institute of Space and Astronautical Science JAXA Retrieved 29 September 2011 IADC Space Debris Mitigation Guidelines PDF Inter Agency Space Debris Coordination Committee 15 October 2002 Archived from the original PDF on 3 December 2013 Retrieved 31 August 2016 NASA Safety Standard 1740 14 Guidelines and Assessment Procedures for Limiting Orbital Debris PDF Office of Safety and Mission Assurance 1 August 1995 Archived from the original PDF on 15 February 2013 100 km Altitude Boundary for Astronautics Federation Aeronautique Internationale NASA Sounding Rocket Program Overview NASA Sounding Rocket Program NASA 24 July 2006 Retrieved 10 October 2006 Reusable Rockets Set to Explore the Ignorosphere Discover Magazine 1 September 2016 Retrieved 2 April 2018 Upper atmosphere may hold clues in Columbia mystery 6 February 2003 External links EditDescription with links to other atmospheric topics Students And Teachers In Near Space Archived 4 January 2018 at the Wayback Machine Near Space Systems Space Data Corporation The B H A L D I Project Portals Weather Earth sciences Astronomy Stars Spaceflight Solar System Retrieved from https en wikipedia org w index php title Mesosphere amp oldid 1135643146, wikipedia, wiki, book, books, library,
