Convection of Moist Saturated Air: Analytical Study. Robert Zakinyan, Arthur Zakinyan *, Roman Ryzhkov and Kristina Avanesyan
|
|
- Eileen Maxwell
- 6 years ago
- Views:
Transcription
1 atmosphere Article Convection of Moist Saturated Air: Analytical Study Robert Zakinyan, Arthur Zakinyan *, Roman Ryzhkov and Kristina Avanesyan Received: 9 October 015; Accepted: 30 December 015; Published: 5 January 016 Academic Editor: Robert W. Talbot Department of General and Theoretical Physics, Institute of Mamatics and Natural Sciences, North Caucasus Federal University, 1 Pushkin Street, Stavropol , Russia; zakinyan@mail.ru (R.Z.); romandesignllc@gmail.com (R.R.); awan.kristina@yandex.ru (K.A.) * Correspondence: zakinyan.a.r@mail.ru; Tel.: Abstract: In present work, steady-state stationary rmal convection of moist saturated air in a lower atmosphere has been studied oretically. Thermal convection was considered without accounting for Coriolis force, and with only temperature The analytical solution of geophysical fluid dynamics equations, which generalizes formulation of moist convection problem, is obtained in two-dimensional case. The stream function is derived in Boussinesq approximation with velocity divergence taken as zero. It has been shown that stream function is asymmetrical in direction contrary to dry and moist unsaturated air convection. It has been demonstrated that convection in moist atmosphere strongly depends on Keywords: rmal convection; Rayleigh Benard convection; moist air; stream function; analytical model 1. Introduction Atmospheric convection is involved in many of central problems in meteorology and climate science [1,]. Investigation and understanding of atmospheric convection is of great importance for development and improvement of global wear and climate prediction [3,4]. Convection interacts with larger-scale dynamics of planetary atmospheres in ways that remain poorly represented in global models [5,6]. The important role in convective instability is played by release of latent heat of condensation during phase transitions of water in moist saturated air [7]. Many experimental and oretical works, reviews and textbooks have been devoted to rmal convection [8 1]. Even so, we currently have not a complete understanding of this phenomenon. According to Alekseev and Gusev [13], free convection can be of two main types: The Rayleigh convection conditioned by hypercritical temperature gradient, and lateral convection resulting from temperature heterogeneity in horizontal plane. The interlatitude and monsoonal type air circulations belong to lateral convection. As for classic Rayleigh convection, examples are convection resulting in formation of clouds distributed in space in form of ular structures (Benard s). Here, convection will be studied. For analysis of a convective stability, linearized system of equations describing rmal convection in a plane has been solved by Rayleigh [14]. It is valid to say that Rayleigh ory is non-stationary two-dimensional linear analytical model of convection. The study of nonhydrostatic models commonly involves extensive numerical integrations. Such an approach was used by Ogura [15], who studied development of an axially symmetric moist convective toward steady state. The numerical studies have been furr developed by many authors (as, for example, in [16,17]). Much insight into problem can be gained by using highly truncated models. Saltzman [18] and Lorenz [19] studied dry convection by only taking a few spectral components of motion and temperature fields into Atmosphere 016, 7, 8; doi: /atmos
2 Atmosphere 016, 7, 8 of 10 account. They have developed Rayleigh ory by considering system of non-linear equations. However, y solved obtained system of equations numerically. These studies have been followed by many ors [0 ]. When moist processes are considered, formulation of a low-order model presents some special difficulties. These are due to complex expressions for latent heat release and asymmetric properties of condensation with respect to upward and downward motion. One simplified approach of physics of condensation has been proposed by Shirer and Dutton [3]. In ir model, condensation processes have effect of modifying critical Rayleigh number, i.e., critical temperature gradient needed for onset of convection. This model has been developed by Huang and Källén [4] by considering hysteretic effects. The effect of moisture is only introduced via condensational heating in [4]. Low-order models of atmosphere were also used to study specific problems such as blocking [5]. Several particular solutions for inviscid non-heat-conducting atmosphere have been analyzed in [6 8]. Currently, numerical methods of analysis of nonstationary two- and three-dimensional non-linear models of convection with use of high-performance computers are widely applicable in oretical studies. On or hand, because of ir relative simplicity, low-order models present considerably more qualitative insight into problem than complicated numerical computations. In spite of this, it is of interest to obtain analytical solution of stationary two-dimensional model of convection. It will allow us to understand better fundamental nature of atmospheric structures and dynamics. The obtained solution can be an effective tool at forecasting of convection parameters. Previously we have reported on two-dimensional analytical model of dry air rmal convection [9]. Here we present furr development of two-dimensional analytical convection model which takes into account atmospheric humidity. Hence, purpose of this article is to define conditions of moist saturated air free convection occurrence within framework of two-dimensional convection model. Here we extend classical parcel-based linear stability analysis to case with a finite displacement.. Basic Equations of Moist Saturated Air Convection Consider ideal fluid equation of motion, in x z plane, in Eulerian form, in inertial reference system, neglecting Earth rotation, in projections onto coordinates axes [30 3]: In equilibrium (statics): Bu Bt ` u Bu Bx ` w Bu Bz 1 ρ i Bw Bt ` u Bw Bx ` w Bw Bz 1 ρ i v 0, Bp Bx 0, 1 ρ e ˆBp Bx (1) ˆBp g () Bz ˆBp g 0 (3) Bz Here ρ i is moist air parcel density; ρ e air parcel surrounding atmosphere density; and g free fall acceleration. We accept parameters of surrounding atmosphere as an undisturbed state. Hence, pressure may be written as: p p ` p 1, here p 1 is pressure disturbance relative to statics state. In moist atmosphere air density equation in Boussinesq approximation will be [13] ρ i ρ e p1 α T β sq (4) where α = 1/T 0 is air rmal expansion coefficient; T 0 = 73 K; T(z) = T i (z) T e (z); T(z) overheat function; T i, T e air parcel internal and external temperatures; s water (also called specific humidity or moisture content); s=s i s e supersaturation function; β M d /M v 1 = 0.608; M d = 9 g/mol dry air molar ; M v = 18 g/mol water molar
3 Atmosphere 016, 7, 8 3 of 10. In or words, we assume that density depends on temperature and and not depends on pressure [33]. Here we do not consider water loading. The temperature change of surrounding atmosphere will be considered to follow law: T e pzq T ec γ pz z c q (5) where γ is surrounding air temperature gradient; and T ec surrounding air temperature at condensation level (z c ). The moist saturated air temperature gradient is determined by [34] γ ma dt i γ a ` L c p (6) where γ a is dry-adiabatic temperature gradient; L specific heat of condensation; c p specific heat capacity at constant pressure; s m saturated. The quantity / appearing in Equation (6) is a complicated function of temperature and pressure [34]; this is why Equation (6) is usually analyzed numerically. To obtain an analytical solution, we should propose an adequate parametrization for quantity /. We specify saturated change with altitude parametrically by expanding in a Taylor series: ˇ ` K pz z c q, K d s m ˇ (7) here K is some function of saturated at condensation level (s mc ). Then for moist-adiabatic temperature gradient we have parametrical form: «γ ma γ a ` L c p ff ˇ ` K pz z c q γ mac ` εpz z c q, γ mac γ a ` L c p ˇ (8) here γ mac is moist-adiabatic temperature gradient at condensation level [34] (this is known function of temperature and pressure). Note that Equation (8) presents a linear approximation to lapse rate. Analyzing and approximating table values of moist-adiabatic temperature gradient [34], for quantity ε we can get: ε = LK/c p « C/m. Then we have that temperature of adiabatically rising moist saturated air parcel follows law: T i pzq T ic γ mac pz z c q ε pz z cq (9) where T ic is rising air parcel temperature at condensation level. The function T i (z) graph presents state curve ; family of such curves is displayed on aerological diagrams. The table values of air temperature obtained from state curve demonstrates satisfactory agreement with values calculated by Equation (9) within convection layer of interest z w z c ď 5 km. Here z w is convection level. Taking into account Equations (5) and (9) overheat function will be: T pzq c T ` γ mac pz z c q ε pz z cq (10) where c T is overheat function at condensation level; γ mac = γ γ mac is difference of ambient air temperature gradient and rising air parcel temperature gradient at condensation level. The quantity γ mac determines angle between state curve and stratification curve at condensation level on aerological diagram.
4 Atmosphere 016, 7, 8 4 of 10 For adiabatically rising air parcel saturated follows law: s m pzq s mc ` ˇ pz z c q ` K pz z cq (11) Assume that decreases linearly with altitude in surrounding atmosphere: s e pzq s ec b pz z c q (1) where s ec is water in surrounding atmosphere at condensation level; b Then for supersaturation function we get s pzq c s ` ˇ ` b pz z c q ` K pz z cq (13) where c s = s mc s ec is supersaturation at condensation level. Taking into account Equations (10) and (13), Equation (4) for air parcel density will be written as: ρ i ρ e 1 α 0 α 1 pz z c q ` α pz z c q ı (14) where α 0 α c T ` β c s, α 1 α γ mac ` β ˇ ` b, α 1 pαε βkq (15) From here level of equalization of densities of rising air parcel and surrounding air can be found: b z ρ z c α 1 ` α 1 ` pαε βkq pα ct ` β c sq. (16) αε βk The level of equalization of temperatures ( level of neutral buoyancy) is determined by b z t z c γ mac ` p γ mac q ` ε c T. (17) ε The steady motion of air parcel is described by set of equations of moist saturated air convection: u Bu Bx ` w Bu Bz 1 Bp 1 (18) ρ e Bx u Bw Bx ` w Bw g pα T ` β sq Bz (19) T pzq c T ` γ mac pz z c q ε pz z cq (0) s pzq c s ` ˇ ` b In Equation (19) following assumption has been made: pz z c q ` K pz z cq (1) Bu Bx ` Bw Bz 0 () ˇ ˇ 1 Bp 1 ρ e Bz ˇ! g pα T ` β sq (3)
5 Atmosphere 016, 7, 8 5 of 10 To satisfy Equation (3), in present study we seek analytical solution for pressure disturbance in form: p 1 1 pxq p1 px, zqˇˇz z (4) where z is some level determined below. Substituting Equations (0) and (1) into Equation (19), we finally get set of equations of moist saturated air free convection in form: u Bu Bx ` w Bu Bz 1 Bp 1 ρ e Bx (5) u Bw Bx ` w Bw Bz g α 0 ` α 1 pz z c q α pz z c q ı (6) Bu Bx ` Bw Bz 0 (7) Furr we will find solution of obtained system of equations. 3. Solution of Moist Saturated Air Convection Equations It follows from continuity Equation (7) that for shallow convection condition stream function ψ may be introduced [30 3]: u Bψ Bz, w Bψ Bx (8) Substituting Equation (8) into Equations (5) and (6), we get: Bψ Bz Bψ B ψ Bz Bx ` Bψ Bx Equation (30) can be written as Bψ B ψ Bz Bx ` Bψ Bx B ψ BxBz Bψ Bx B ψ Bz 1 Bp 1 ρ e Bx (9) B ψ BzBx g α 0 ` α 1 pz z c q α pz z c q ı (30) B ψ BzBx N r mac rz ` pz z c q k 1 pz z c q ı (31) where rn mac g «α γ mac ` β ff ˇ ` b (3) is square of Brunt Väisälä frequency for moist saturated air; α c T ` β c s αε βk rz, k 1 «ff (33) α γ mac ` β ˇ ` b α γ mac ` β ˇ ` b We seek solution of resulting equations set in following form: Substituting Equation (34) into Equation (9), we get: ψ px, zq X pxq Z pzq (34) Z XX 1 1 ZZ 1 Bp 1 ρ e Bx (35)
6 Atmosphere 016, 7, 8 6 of 10 Substituting Equation (34) into Equation (31), we obtain: X ZZ 1 1 XX N r mac rz ` pz z c q k 1 pz z c q From Equation (36), separating variables, it follows that: ZZ 1 k r N mac rz ` pz z c q k 1 pz z c q (36) (37) Atmosphere 016, 7, 8 6 of 10 X 1 XX 1 k (38) ZZ = k N ( ) ( ) where k is constant requiring determination. mac ( z + z z The Equation c k 1 z z (37) c solution ) has form: (37) 1 Z kn r X XX mac d pz z c q rz ` pz = z j k cq k1 3 pz z cq (38) where k is constant requiring determination. The Equation (37) solution has form: It follows from here: ( z z ( ) c ) k 1 ( ) Z = kn mac z zc z + z z Z 1 kn r rz ` pz z c q k 1 pz z c q c (39) 3 mac d pz z c q rz ` pz z j (40) It follows from here: cq k1 3 pz z cq z + ( z zc) k1( z zc) Z = kn mac We seek Equation (38) solution with following ( z zc ) form: k1 (40) ( z zc) z + ( z zc) 3 X 1 cos kx (41) We seek Equation (38) solution with kfollowing form: Substituting Equation (41) directly into Equation 1 Х = cos (38), kx we see that solution is valid. Hence, for (41) stream function, we have expression: k Substituting Equation (41) directly N ψ ZX r d into Equation (38), we see that solution is valid. Hence, mac pz z c q rz ` pz z j for stream function, we have expression: cq k1 k 3 pz z cq cos kx (4) N ( ) mac z z ( ) c k 1 ( ) ψ = ZX = z zc z + z zc cos kx (4) 1 shows this function graph. k As is seen, stream 3 function is symmetrical in horizontal direction and asymmetrical 1 shows this in function graph. direction. As is seen, The level stream of maximal function is symmetrical velocities in horizontal is in upper part of direction convective and asymmetrical contrary in to direction. dry and moist The level unsaturated of maximal air convection velocities [9]. is in upper part of convective contrary to dry and moist unsaturated air convection [9]. (39) 1. Stream function at b = 10 6 m 1, ΔcT = 0.5 C, Δcs = 0, Δγmac = C/m, ε C/m, 1. Stream function at b = k = 10 3 m 1, d d 10 6 m 1 = m,. c T = 0.5 C, c s = 0, γ mac = 5 ˆ 10 4 C/m, ε = 3 ˆ 10 7 C/m, k = 10 3 m 1, { z zc 1.6 ˆ 10 6 m 1. From Equations (8) velocity projections can be written: z + ( z zc) k1( z zc) ( c ) 1 ( z z ) z + ( z z ) N mac u = ZX = cos kx k z z k c c 3 (43)
7 From here one can see that maximal velocities level is not in center of convective as it has been for dry air convection. The maximal velocities level for moist saturated air is at /3 of of convection. Substituting expression for zmax zc into Equation (44), we get for ascending moist Atmosphere 016, 7, 8 7 of 10 From Equations (8) velocity projections can be written: u Z 1 X rn mac rz ` pz z c q k 1 pz z c q d k pz z c q rz ` pz z jcos kx (43) Atmosphere 016, 7, 8 cq k1 3 pz z cq 7 of 10 ( ) z z ( ) w ZX 1 N r mac d pz z c q rz ` pz z c k cq 1 ( ) w= ZX = N j mac z zc z + k1 z z 3 pz c z sin kx 3 cq (44) sin kx (44) From here, using condition w = 0, we get expression for of convection From here, using condition w = 0, we get expression for of convection (or cloud ): (or cloud ): z w z c 3 c ` ` 16 c4k k zw z = 1 1 k z1rz 4k (45) shows shows dependence dependence of of convection convection on on water water As As is is seen, seen, convection convection rises rises monotonically monotonically with with.. Convection Convection vs. vs. water water The The atmospheric atmospheric parameters parameters are are same same as as in in Analysis and Discussion of Obtained Solution 4. Analysis and Discussion of Obtained Solution We find maximal velocities level from condition: w/ z 0. Taking derivative of We find maximal velocities level from condition: Bw/Bz = 0. Taking derivative of Equation (44) with respect to z, we get: Equation (44) with respect to z, we get: kz 1 zmax zc = (46) z max z c 1 ` a1 ` 4k k 1 rz 1 (46) k 1 If =0 ( overheat ΔcT and oversaturation Δcs are equal to zero at condensation level), If rz 0 ( overheat n for convection level c T and oversaturation and for maximal velocities c s are equal to zero at condensation level), level we have n for convection level and for maximal velocities level we have d s αδγ m mac + β ds + b 3 m z= zc zw zc = = 3 (47) z w z c 3 α γ mac ` β ˇ ` b k k 3 1 αε βk (47) 1 αε βk ds αδγ m mac + β + b 1 z= zc (48) zmax zc = = k1 αε βk
8 Atmosphere 016, 7, 8 8 of 10 z max z c 1 k 1 «α γ mac ` β αε βk ff ˇ ` b From here one can see that maximal velocities level is not in center of convective as it has been for dry air convection. The maximal velocities level for moist saturated air is at /3 of of convection. Substituting expression for z max z c into Equation (44), we get for ascending moist saturated air maximal velocity equation: w max r N mac k 1 g f e 1 ` a1 «` 4k 1 rz k 1 rz ` 1 ` a1 ` 4k 1 rz 4 (48) 1 1 ` a1 ff ` 4k 1 1 rz sin kx. (49) If rz 0, n we have w max r N mac? 3k1 sin kx (50) Let us find pressure spatial distribution. For this, integrating Equation (35), we get: p 1 px, zq 1 ρ ex Z 1 ZZ ` const (51) The constant of integration can be found from condition that at maximal velocities level pressure disturbance is equal to zero at points meeting condition cos kx = 1. From here we have Here we take into account that if rz 0, n const ρ e r N mac k (5) Z 1 3 kk 1N r k 1 pz z c q mac 1 j 3{, z max z c 1 (53) 3 k k 1 1 pz z c q From here, taking into account Equation (4) and assuming z z max, for pressure disturbance we get p 1 1 pxq p1 px, z max q ρ e r N mac k sin kx (54) It should be noted that analytical solution Equation (4) is obtained by integrating only one Equation (36); in so doing we neglected term 1 ρ e Bp 1 {B z in accordance with condition Equation (3). In such an approach to problem, Equation (18) plays a role of auxiliary equation for pressure disturbance determination. To make Equations (18) and (19) agree with condition Equation (3) we were compelled to consider Equation (18) at point z z max of maximal velocities where pressure disturbance is equal to zero. 5. Conclusions Hence, we have obtained new solution of equations of moist saturated air convection in atmospheric cloud layer. The solution is obtained within framework of stationary D analytical model. It has been shown that convection parameters in moist atmosphere strongly depend on water The expression for convective is obtained. The obtained solutions can be valuable in convection parameters forecasting practice. As it can be seen from obtained equations, important convection parameters, such as convection level,
9 Atmosphere 016, 7, 8 9 of 10 level of neutral buoyancy, maximal velocities level, and maximal velocity itself, are determined by characteristics which can be calculated from aerological diagrams using radiosounding data. These characteristics are angle between state curve and stratification curve at condensation level and water Acknowledgments: This work was supported by Ministry of Education and Science of Russian Federation in framework of base part of governmental ordering for scientific research works (order No 014/16, project 653). Author Contributions: Robert Zakinyan planned and supervised research, co-wrote paper; Arthur Zakinyan co-performed oretical analysis, co-wrote paper; Roman Ryzhkov and Kristina Avanesyan co-performed oretical analysis. Conflicts of Interest: The authors declare no conflict of interest. References 1. Emanuel, K.A. Atmospheric Convection; Oxford University Press: New York, NY, USA, Stevens, B. Atmospheric moist convection. Annu. Rev. Earth Planet. Sci. 005, 33, [CrossRef] 3. Sherwood, S.C.; Bony, S.; Dufresne, J.-L. Spread in model climate sensitivity traced to atmospheric convective mixing. Nature 014, 505, [CrossRef] [PubMed] 4. Bluestein, H.B. Severe Convective Storms and Tornadoes; Springer: Chichester, UK, Lambaerts, J.; Lapeyre, G.; Zeitlin, V. Moist versus dry barotropic instability in a shallow-water model of atmosphere with moist convection. J. Atmos. Sci. 011, 68, [CrossRef] 6. Yano, J.; Geleyn, J.-F.; Köhler, M.; Mironov, D.; Quaas, J.; Soares, P.M.M.; Phillips, V.T.J.; Plant, R.S.; Deluca, A.; Marquet, P.; et al. Basic concepts for convection parameterization in wear forecast and climate models: COST action ES0905 final report. Atmosphere 015, 6, [CrossRef] 7. Shmerlin, B.Y.; Kalashnik, M.V. Rayleigh convective instability in presence of phase transitions of water. The formation of large-scale eddies and cloud structures. Phys. Uspekhi 013, 56, [CrossRef] 8. Chandrasekhar, S. Hydrodynamic and Hydromagnetic Stability; Clarendon Press: Oxford, UK, Martynenko, O.G.; Khramtsov, P.P. Free-Convective Heat Transfer; Springer: Berlin, Germany, Ogura, Y. A review of numerical modeling research on small-scale convection in atmosphere. Meteorol. Monogr. 1963, 5, Arakawa, A.; Jung, J.-H. Multiscale modeling of moist-convective atmosphere A review. Atmos. Res. 011, 10, [CrossRef] 1. Derbyshire, S.H.; Beau, I.; Bechtold, P.; Grandpeix, J.-Y.; Piriou, J.-M.; Redelsperger, J.-L.; Soares, P.M.M. Sensitivity of moist convection to environmental humidity. Q. J. R. Meteorol. Soc. 004, 130, [CrossRef] 13. Alekseev, V.V.; Gusev, A.M. Free convection in geophysical processes. Sov. Phys. Uspekhi 1983, 6, [CrossRef] 14. Rayleigh, L. On convective currents in a horizontal layer of fluid when higher temperature is on underside. Philos. Mag. 1916, 3, [CrossRef] 15. Ogura, Y. The evolution of a moist convective element in a shallow, conditionally unstable atmosphere: A numerical calculation. J. Atmos. Sci. 1963, 0, [CrossRef] 16. Van Delden, A.; Oerlemans, J. Grouping of clouds in a numerical cumulus convection model. Contrib. Atmos. Phys 198, 56, Asai, T.; Nakasuji, I. A furr study of preferred mode of cumulus convection in a conditionally unstable atmosphere. J. Meteorol. Soc. Jpn. 198, 60, Saltzman, B. Finite amplitude free convection as an initial value problem I. J. Atmos. Sci. 196, 19, [CrossRef] 19. Lorenz, E.N. Deterministic nonperiodic flow. J. Atmos. Sci. 1963, 0, [CrossRef] 0. Van Delden, A. Scale selection in low-order spectral models of two-dimensional rmal convection. Tellus 1984, 36, [CrossRef] 1. Schlesinger, R.E.; Young, J.A. On transient behavior of Asai s model of moist convection. Mon. Wear Rev. 1970, 98, [CrossRef]
10 Atmosphere 016, 7, 8 10 of 10. Brerton, C.S. A ory for nonprecipitating moist convection between two parallel plates. Part I: Thermodynamics and linear solutions. J. Atmos. Sci. 1987, 44, [CrossRef] 3. Shirer, H.N.; Dutton, J.A. The branching hierarchy of multiple solutions in a model of moist convection. J. Amos. Sci. 1979, 36, [CrossRef] 4. Huang, X.-Y.; Källén, E. A low-order model for moist convection. Tellus 1986, 38, [CrossRef] 5. Charney, J.G.; Devore, J.G. Multiple flow equilibria in atmosphere and blocking. J. Atmos. Sci. 1979, 36, [CrossRef] 6. Kuo, H.L. Convection in a conditionally unstable atmosphere. Tellus 1961, 13, [CrossRef] 7. Lilly, D.K. On ory of disturbances in a conditionally unstable atmosphere. Mon. Wear Rev. 1960, 88, [CrossRef] 8. Gill, A.E. Spontaneously growing hurricane-like disturbances in a simple baroclinic model with latent: Heat release. In Intense Atmospheric Vortices; Springer: Berlin, Germany, Zakinyan, R.G.; Zakinyan, A.R.; Lukinov, A.A. Two-dimensional analytical model of dry air rmal convection. Meteorol. Atmos. Phys. 015, 17, [CrossRef] 30. Drazin, P.G. Introduction to Hydrodynamic Stability; Cambridge University Press: Cambridge, UK, Monin, A.S. Theoretical Geophysical Fluid Dynamics; Kluwer Academic Publishers: Dordrecht, The Nerlands, Zdunkowski, W.; Bott, A. Dynamics of Atmosphere: A Course in Theoretical Meteorology; Cambridge University Press: Cambridge, UK, Smith, R.K. The physics and parameterization of moist atmospheric convection. In Nato Science Series C; Kluwer Academic Publishers: Dordrecht, The Nerlands, 1997; Volume Matveev, L.T. Fundamentals of General Meteorology: Physics of Atmosphere; Israel Program for Scientific Translations: Jerusalem, Israel, by authors; licensee MDPI, Basel, Switzerland. This article is an open access article distributed under terms and conditions of Creative Commons by Attribution (CC-BY) license (
Conference Proceedings Paper Vortex Motion State of the Dry Atmosphere with Nonzero Velocity Divergence
1 3 4 5 6 7 8 9 10 11 1 13 14 15 16 17 18 19 0 1 3 4 5 6 7 8 9 30 31 3 33 34 35 36 37 38 39 40 41 Conference Proceedings Paper Vortex Motion State of the Dry Atmosphere with Nonzero Velocity Divergence
More informationProceedings Vortex Motion State of the Dry Atmosphere with Nonzero Velocity Divergence
Proceedings Vortex Motion State of the Dry Atmosphere with Nonzero Velocity Divergence Robert Zakinyan, Arthur Zakinyan *, Roman Ryzhkov and Julia Semenova Department of General and Theoretical Physics,
More informationPrototype Instabilities
Prototype Instabilities David Randall Introduction Broadly speaking, a growing atmospheric disturbance can draw its kinetic energy from two possible sources: the kinetic and available potential energies
More informationVortex Motion State of the Dry Atmosphere with Nonzero Velocity Divergence
atmosphere Article Vortex Motion State of Dry Atmosphere with Nonzero Velocity Divergence Robert Zakinyan, Arthur Zakinyan * ID, Roman Ryzhkov Julia Semenova Department of General Theoretical Physics,
More informationModeling Large-Scale Atmospheric and Oceanic Flows 2
Modeling Large-Scale Atmospheric and Oceanic Flows V. Zeitlin known s of the Laboratoire de Météorologie Dynamique, Univ. P. and M. Curie, Paris Mathematics of the Oceans, Fields Institute, Toronto, 3
More informationRadiative equilibrium Some thermodynamics review Radiative-convective equilibrium. Goal: Develop a 1D description of the [tropical] atmosphere
Radiative equilibrium Some thermodynamics review Radiative-convective equilibrium Goal: Develop a 1D description of the [tropical] atmosphere Vertical temperature profile Total atmospheric mass: ~5.15x10
More informationHurricanes are intense vortical (rotational) storms that develop over the tropical oceans in regions of very warm surface water.
Hurricanes: Observations and Dynamics Houze Section 10.1. Holton Section 9.7. Emanuel, K. A., 1988: Toward a general theory of hurricanes. American Scientist, 76, 371-379 (web link). http://ww2010.atmos.uiuc.edu/(gh)/guides/mtr/hurr/home.rxml
More informationLecture 3: Convective Heat Transfer I
Lecture 3: Convective Heat Transfer I Kerry Emanuel; notes by Paige Martin and Daniel Mukiibi June 18 1 Introduction In the first lecture, we discussed radiative transfer in the climate system. Here, we
More informationReferences: Parcel Theory. Vertical Force Balance. ESCI Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr.
References: ESCI 340 - Cloud Physics and Precipitation Processes Lesson 3 - Stability and Buoyancy Dr. DeCaria Glossary of Meteorology, 2nd ed., American Meteorological Society A Short Course in Cloud
More information2.1 Effects of a cumulus ensemble upon the large scale temperature and moisture fields by induced subsidence and detrainment
Atmospheric Sciences 6150 Cloud System Modeling 2.1 Effects of a cumulus ensemble upon the large scale temperature and moisture fields by induced subsidence and detrainment Arakawa (1969, 1972), W. Gray
More informationBoundary layer equilibrium [2005] over tropical oceans
Boundary layer equilibrium [2005] over tropical oceans Alan K. Betts [akbetts@aol.com] Based on: Betts, A.K., 1997: Trade Cumulus: Observations and Modeling. Chapter 4 (pp 99-126) in The Physics and Parameterization
More informationMoist Convection. Chapter 6
Moist Convection Chapter 6 1 2 Trade Cumuli Afternoon cumulus over land 3 Cumuls congestus Convectively-driven weather systems Deep convection plays an important role in the dynamics of tropical weather
More informationOn the effect of forward shear and reversed shear baroclinic flows for polar low developments. Thor Erik Nordeng Norwegian Meteorological Institute
On the effect of forward shear and reversed shear baroclinic flows for polar low developments Thor Erik Nordeng Norwegian Meteorological Institute Outline Baroclinic growth a) Normal mode solution b) Initial
More informationA Further Study of Dynamics of the Four-Day Circulation. By Yoshihisa Matsuda
February 1982 Y. Matsuda 245 A Further Study of Dynamics of the Four-Day Circulation in the Venus Atmosphere By Yoshihisa Matsuda Department of Astronomy and Earth Sciences, Tokyo Gakugei University, Koganei
More informationDynamics and Kinematics
Geophysics Fluid Dynamics () Syllabus Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3,
More informationGeophysics Fluid Dynamics (ESS228)
Geophysics Fluid Dynamics (ESS228) Course Time Lectures: Tu, Th 09:30-10:50 Discussion: 3315 Croul Hall Text Book J. R. Holton, "An introduction to Dynamic Meteorology", Academic Press (Ch. 1, 2, 3, 4,
More informationModel description of AGCM5 of GFD-Dennou-Club edition. SWAMP project, GFD-Dennou-Club
Model description of AGCM5 of GFD-Dennou-Club edition SWAMP project, GFD-Dennou-Club Mar 01, 2006 AGCM5 of the GFD-DENNOU CLUB edition is a three-dimensional primitive system on a sphere (Swamp Project,
More informationGoals of this Chapter
Waves in the Atmosphere and Oceans Restoring Force Conservation of potential temperature in the presence of positive static stability internal gravity waves Conservation of potential vorticity in the presence
More information196 7 atmospheric oscillations:
196 7 atmospheric oscillations: 7.4 INTERNAL GRAVITY (BUOYANCY) WAVES We now consider the nature of gravity wave propagation in the atmosphere. Atmospheric gravity waves can only exist when the atmosphere
More information( ) = 1005 J kg 1 K 1 ;
Problem Set 3 1. A parcel of water is added to the ocean surface that is denser (heavier) than any of the waters in the ocean. Suppose the parcel sinks to the ocean bottom; estimate the change in temperature
More informationThermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic]
Thermodynamics Review [?] Entropy & thermodynamic potentials Hydrostatic equilibrium & buoyancy Stability [dry & moist adiabatic] Entropy 1. (Thermodynamics) a thermodynamic quantity that changes in a
More informationParameterization of effects of unresolved clouds and precipitation
Parameterization of effects of unresolved clouds and precipitation eas471_cumparam.odp JDW, EAS, U. Alberta Last modified: 29 Mar. 2016 (from Physical Parameterizations in Canadian Operational Models,
More informationAtmospheric Dynamics: lecture 2
Atmospheric Dynamics: lecture 2 Topics Some aspects of advection and the Coriolis-effect (1.7) Composition of the atmosphere (figure 1.6) Equation of state (1.8&1.9) Water vapour in the atmosphere (1.10)
More informationProject 3 Convection and Atmospheric Thermodynamics
12.818 Project 3 Convection and Atmospheric Thermodynamics Lodovica Illari 1 Background The Earth is bathed in radiation from the Sun whose intensity peaks in the visible. In order to maintain energy balance
More informationINTERNAL GRAVITY WAVES
INTERNAL GRAVITY WAVES B. R. Sutherland Departments of Physics and of Earth&Atmospheric Sciences University of Alberta Contents Preface List of Tables vii xi 1 Stratified Fluids and Waves 1 1.1 Introduction
More informationEliassen-Palm Theory
Eliassen-Palm Theory David Painemal MPO611 April 2007 I. Introduction The separation of the flow into its zonal average and the deviations therefrom has been a dominant paradigm for analyses of the general
More informationDraft Chapter from Mesoscale Dynamic Meteorology By Prof. Yu-lang Lin, North Carolina State University
Draft Chapter from Mesoscale Dynamic Meteorology By Prof. Yu-lang Lin, North Carolina State University Chapter 1 Overview 1.1 Introduction The so-called mesometeorology or mesoscale meteorology is defined
More informationEnhanced summer convective rainfall at Alpine high elevations in response to climate warming
SUPPLEMENTARY INFORMATION DOI: 10.1038/NGEO2761 Enhanced summer convective rainfall at Alpine high elevations in response to climate warming Filippo Giorgi, Csaba Torma, Erika Coppola, Nikolina Ban, Christoph
More informationLecture 10a: The Hadley Cell
Lecture 10a: The Hadley Cell Geoff Vallis; notes by Jim Thomas and Geoff J. Stanley June 27 In this short lecture we take a look at the general circulation of the atmosphere, and in particular the Hadley
More informationDynamic Meteorology: lecture 2
Dynamic Meteorology: lecture 2 Sections 1.3-1.5 and Box 1.5 Potential temperature Radiatively determined temperature (boxes 1.1-1.4) Buoyancy (-oscillations) and static instability, Brunt-Vaisala frequency
More informationBALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere. Potential temperature θ. Rossby Ertel potential vorticity
BALANCED FLOW: EXAMPLES (PHH lecture 3) Potential Vorticity in the real atmosphere Need to introduce a new measure of the buoyancy Potential temperature θ In a compressible fluid, the relevant measure
More informationGravity Waves. Lecture 5: Waves in Atmosphere. Waves in the Atmosphere and Oceans. Internal Gravity (Buoyancy) Waves 2/9/2017
Lecture 5: Waves in Atmosphere Perturbation Method Properties of Wave Shallow Water Model Gravity Waves Rossby Waves Waves in the Atmosphere and Oceans Restoring Force Conservation of potential temperature
More informationGeneralizing the Boussinesq Approximation to Stratified Compressible Flow
Generalizing the Boussinesq Approximation to Stratified Compressible Flow Dale R. Durran a Akio Arakawa b a University of Washington, Seattle, USA b University of California, Los Angeles, USA Abstract
More informationFloquet Theory for Internal Gravity Waves in a Density-Stratified Fluid. Yuanxun Bill Bao Senior Supervisor: Professor David J. Muraki August 3, 2012
Floquet Theory for Internal Gravity Waves in a Density-Stratified Fluid Yuanxun Bill Bao Senior Supervisor: Professor David J. Muraki August 3, 212 Density-Stratified Fluid Dynamics Density-Stratified
More informationPALM - Cloud Physics. Contents. PALM group. last update: Monday 21 st September, 2015
PALM - Cloud Physics PALM group Institute of Meteorology and Climatology, Leibniz Universität Hannover last update: Monday 21 st September, 2015 PALM group PALM Seminar 1 / 16 Contents Motivation Approach
More informationChapter 2. The continuous equations
Chapter. The continuous equations Fig. 1.: Schematic of a forecast with slowly varying weather-related variations and superimposed high frequency Lamb waves. Note that even though the forecast of the slow
More informationAn Introduction to Physical Parameterization Techniques Used in Atmospheric Models
An Introduction to Physical Parameterization Techniques Used in Atmospheric Models J. J. Hack National Center for Atmospheric Research Boulder, Colorado USA Outline Frame broader scientific problem Hierarchy
More informationTropical Cyclone Intensification
Tropical Cyclone Intensification Theories for tropical cyclone intensification and structure CISK (Charney and Eliassen 1964) Cooperative Intensification Theory (Ooyama 1969). WISHE (Emanuel 1986, Holton
More informationOnset of convection of a reacting fluid layer in a porous medium with temperature-dependent heat source
AMERICAN JOURNAL OF SCIENTIFIC AND INDUSTRIAL RESEARCH 2011, Science Huβ, http://www.scihub.org/ajsir ISSN: 2153-649X doi:10.5251/ajsir.2011.2.6.860.864 Onset of convection of a reacting fluid layer in
More informationChapter 1. Introduction
Chapter 1. Introduction In this class, we will examine atmospheric phenomena that occurs at the mesoscale, including some boundary layer processes, convective storms, and hurricanes. We will emphasize
More information4. Atmospheric transport. Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017
4. Atmospheric transport Daniel J. Jacob, Atmospheric Chemistry, Harvard University, Spring 2017 Forces in the atmosphere: Gravity g Pressure-gradient ap = ( 1/ ρ ) dp / dx for x-direction (also y, z directions)
More information2. Conservation laws and basic equations
2. Conservation laws and basic equations Equatorial region is mapped well by cylindrical (Mercator) projection: eastward, northward, upward (local Cartesian) coordinates:,, velocity vector:,,,, material
More informationChapter 5. Atmospheric Moisture
Chapter 5 Atmospheric Moisture hydrologic cycle--movement of water in all forms between earth & atmosphere Humidity: amount of water vapor in air vapor pressure saturation vapor pressure absolute humidity
More informationSAMPLE CHAPTERS UNESCO EOLSS WAVES IN THE OCEANS. Wolfgang Fennel Institut für Ostseeforschung Warnemünde (IOW) an der Universität Rostock,Germany
WAVES IN THE OCEANS Wolfgang Fennel Institut für Ostseeforschung Warnemünde (IOW) an der Universität Rostock,Germany Keywords: Wind waves, dispersion, internal waves, inertial oscillations, inertial waves,
More informationCondensation of Water Vapor in the Gravitational Field 1
ISSN 063-776, Journal of Experimental and Theoretical Physics, 202, Vol. 5, No. 4, pp. 723 728. Pleiades Publishing, Inc., 202. Original Russian Text V.G. Gorshkov, A.M. Makarieva, A.V. Nefiodov, 202,
More informationClouds and turbulent moist convection
Clouds and turbulent moist convection Lecture 2: Cloud formation and Physics Caroline Muller Les Houches summer school Lectures Outline : Cloud fundamentals - global distribution, types, visualization
More informationSEVERE AND UNUSUAL WEATHER
SEVERE AND UNUSUAL WEATHER Basic Meteorological Terminology Adiabatic - Referring to a process without the addition or removal of heat. A temperature change may come about as a result of a change in the
More informationIn two-dimensional barotropic flow, there is an exact relationship between mass
19. Baroclinic Instability In two-dimensional barotropic flow, there is an exact relationship between mass streamfunction ψ and the conserved quantity, vorticity (η) given by η = 2 ψ.the evolution of the
More informationNWP Equations (Adapted from UCAR/COMET Online Modules)
NWP Equations (Adapted from UCAR/COMET Online Modules) Certain physical laws of motion and conservation of energy (for example, Newton's Second Law of Motion and the First Law of Thermodynamics) govern
More informationTransient/Eddy Flux. Transient and Eddy. Flux Components. Lecture 7: Disturbance (Outline) Why transients/eddies matter to zonal and time means?
Lecture 7: Disturbance (Outline) Transients and Eddies Climate Roles Mid-Latitude Cyclones Tropical Hurricanes Mid-Ocean Eddies (From Weather & Climate) Flux Components (1) (2) (3) Three components contribute
More informationGFD 2012 Lecture 1: Dynamics of Coherent Structures and their Impact on Transport and Predictability
GFD 2012 Lecture 1: Dynamics of Coherent Structures and their Impact on Transport and Predictability Jeffrey B. Weiss; notes by Duncan Hewitt and Pedram Hassanzadeh June 18, 2012 1 Introduction 1.1 What
More informationEliassen-Palm Cross Sections Edmon et al. (1980)
Eliassen-Palm Cross Sections Edmon et al. (1980) Cecily Keppel November 14 2014 Eliassen-Palm Flux For β-plane Coordinates (y, p) in northward, vertical directions Zonal means F = v u f (y) v θ θ p F will
More informationarxiv: v1 [physics.ao-ph] 18 Jul 2007
GEOPHYSICAL RESEARCH LETTERS, VOL.???, XXXX, DOI:10.1029/, arxiv:07.2750v1 [physics.ao-ph] 18 Jul 2007 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 Multiple Equilibria in a Single-Column Model of the Tropical Atmosphere
More informationToday s Lecture: Atmosphere finish primitive equations, mostly thermodynamics
Today s Lecture: Atmosphere finish primitive equations, mostly thermodynamics Reference Peixoto and Oort, Sec. 3.1, 3.2, 3.4, 3.5 (but skip the discussion of oceans until next week); Ch. 10 Thermodynamic
More informationSymmetry methods in dynamic meteorology
Symmetry methods in dynamic meteorology p. 1/12 Symmetry methods in dynamic meteorology Applications of Computer Algebra 2008 Alexander Bihlo alexander.bihlo@univie.ac.at Department of Meteorology and
More information1/18/2011. Conservation of Momentum Conservation of Mass Conservation of Energy Scaling Analysis ESS227 Prof. Jin-Yi Yu
Lecture 2: Basic Conservation Laws Conservation Law of Momentum Newton s 2 nd Law of Momentum = absolute velocity viewed in an inertial system = rate of change of Ua following the motion in an inertial
More informationContents. Parti Fundamentals. 1. Introduction. 2. The Coriolis Force. Preface Preface of the First Edition
Foreword Preface Preface of the First Edition xiii xv xvii Parti Fundamentals 1. Introduction 1.1 Objective 3 1.2 Importance of Geophysical Fluid Dynamics 4 1.3 Distinguishing Attributes of Geophysical
More informationOrographic Precipitation II: Effects of Phase Change on Orographic Flow. Richard Rotunno. National Center for Atmospheric Research, USA
Orographic Precipitation II: Effects of Phase Change on Orographic Flow Richard Rotunno National Center for Atmospheric Research, USA Condensation D Dt vs w( x, ) vs U Large-Scale Flow 0 H L Dynamics w
More information1. Static Stability. (ρ V ) d2 z (1) d 2 z. = g (2) = g (3) T T = g T (4)
NCAR (National Center for Atmospheric Research) has an excellent resource for education called COMET-MetEd. There you can find some really great tutorials on SkewT-LogP plots: visit http://www.meted.ucar.edu/mesoprim/skewt/index.htm.
More informationThermodynamics of a Global-Mean State of the Atmosphere A State of Maximum Entropy Increase
1 Thermodynamics of a Global-Mean State of the Atmosphere A State of Maximum Entropy Increase HISASHI OZAWA* AND ATSUMU OHMURA Department of Geography, Swiss Federal Institute of Technology (ETH), Zurich,
More informationBuoyancy and Coriolis forces
Chapter 2 Buoyancy and Coriolis forces In this chapter we address several topics that we need to understand before starting on our study of geophysical uid dynamics. 2.1 Hydrostatic approximation Consider
More informationNotes and Correspondence Higher-order corrections for Rossby waves in a zonal channel on the β-plane
QUARTERLY JOURNAL OF THE ROYAL METEOROLOGICAL SOCIETY Q. J. R. Meteorol. Soc. 33: 893 898 (7 Published online 4 October 7 in Wiley InterScience (www.interscience.wiley.com DOI:./qj.44 Notes and Correspondence
More informationCan a Simple Two-Layer Model Capture the Structure of Easterly Waves?
Can a Simple Two-Layer Model Capture the Structure of Easterly Waves? Cheryl L. Lacotta 1 Introduction Most tropical storms in the Atlantic, and even many in the eastern Pacific, are due to disturbances
More information10 Shallow Water Models
10 Shallow Water Models So far, we have studied the effects due to rotation and stratification in isolation. We then looked at the effects of rotation in a barotropic model, but what about if we add stratification
More informationIsentropic Analysis. Much of this presentation is due to Jim Moore, SLU
Isentropic Analysis Much of this presentation is due to Jim Moore, SLU Utility of Isentropic Analysis Diagnose and visualize vertical motion - through advection of pressure and system-relative flow Depict
More informationChapter 1. Governing Equations of GFD. 1.1 Mass continuity
Chapter 1 Governing Equations of GFD The fluid dynamical governing equations consist of an equation for mass continuity, one for the momentum budget, and one or more additional equations to account for
More informationPHYS 432 Physics of Fluids: Instabilities
PHYS 432 Physics of Fluids: Instabilities 1. Internal gravity waves Background state being perturbed: A stratified fluid in hydrostatic balance. It can be constant density like the ocean or compressible
More information2. Baroclinic Instability and Midlatitude Dynamics
2. Baroclinic Instability and Midlatitude Dynamics Midlatitude Jet Stream Climatology (Atlantic and Pacific) Copyright 26 Emily Shuckburgh, University of Cambridge. Not to be quoted or reproduced without
More informationAccurate computation of moist available potential energy with the Munkres algorithm
Quarterly Journal of the Royal Meteorological Society Q. J. R. Meteorol. Soc. 143: 288 292, January 2017 A DOI:10.1002/qj.2921 Accurate computation of moist available potential energy with the Munkres
More informationMEA 716 Exercise, BMJ CP Scheme With acknowledgements to B. Rozumalski, M. Baldwin, and J. Kain Optional Review Assignment, distributed Th 2/18/2016
MEA 716 Exercise, BMJ CP Scheme With acknowledgements to B. Rozumalski, M. Baldwin, and J. Kain Optional Review Assignment, distributed Th 2/18/2016 We have reviewed the reasons why NWP models need to
More informationChapter 4. Gravity Waves in Shear. 4.1 Non-rotating shear flow
Chapter 4 Gravity Waves in Shear 4.1 Non-rotating shear flow We now study the special case of gravity waves in a non-rotating, sheared environment. Rotation introduces additional complexities in the already
More informationAtmosphere, Ocean and Climate Dynamics Fall 2008
MIT OpenCourseWare http://ocw.mit.edu 12.003 Atmosphere, Ocean and Climate Dynamics Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. Contents
More informationModel equations for planetary and synoptic scale atmospheric motions associated with different background stratification
Model equations for planetary and synoptic scale atmospheric motions associated with different background stratification Stamen Dolaptchiev & Rupert Klein Potsdam Institute for Climate Impact Research
More informationDynamics Rotating Tank
Institute for Atmospheric and Climate Science - IACETH Atmospheric Physics Lab Work Dynamics Rotating Tank Large scale flows on different latitudes of the rotating Earth Abstract The large scale atmospheric
More informationLecture 7. Science A-30 February 21, 2008 Air may be forced to move up or down in the atmosphere by mechanical forces (wind blowing over an obstacle,
Lecture 7. Science A-30 February 21, 2008 Air may be forced to move up or down in the atmosphere by mechanical forces (wind blowing over an obstacle, like a mountain) or by buoyancy forces. Air that is
More informationThe Effect of Sea Spray on Tropical Cyclone Intensity
The Effect of Sea Spray on Tropical Cyclone Intensity Jeffrey S. Gall, Young Kwon, and William Frank The Pennsylvania State University University Park, Pennsylvania 16802 1. Introduction Under high-wind
More informationScienceDirect. Numerical modeling of atmospheric water content and probability evaluation. Part I
Available online at www.sciencedirect.com ScienceDirect Procedia Engineering 70 ( 2014 ) 321 329 12th International Conference on Computing and Control for the Water Industry, CCWI2013 Numerical modeling
More information2σ e s (r,t) = e s (T)exp( rr v ρ l T ) = exp( ) 2σ R v ρ l Tln(e/e s (T)) e s (f H2 O,r,T) = f H2 O
Formulas/Constants, Physics/Oceanography 4510/5510 B Atmospheric Physics II N A = 6.02 10 23 molecules/mole (Avogadro s number) 1 mb = 100 Pa 1 Pa = 1 N/m 2 Γ d = 9.8 o C/km (dry adiabatic lapse rate)
More informationConvection and buoyancy oscillation
Convection and buoyancy oscillation Recap: We analyzed the static stability of a vertical profile by the "parcel method"; For a given environmental profile (of T 0, p 0, θ 0, etc.), if the density of an
More informationDynamic Meteorology (Atmospheric Dynamics)
Lecture 1-2012 Dynamic Meteorology (Atmospheric Dynamics) Lecturer: Aarnout van Delden Office: BBG, room 615 a.j.vandelden@uu.nl http://www.staff.science.uu.nl/~delde102/index.php Students (background
More informationQuasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States
Quasi-equilibrium Theory of Small Perturbations to Radiative- Convective Equilibrium States See CalTech 2005 paper on course web site Free troposphere assumed to have moist adiabatic lapse rate (s* does
More informationThe Effective Static Stability Experienced by Eddies in a Moist Atmosphere
JANUARY 2011 O G O R M A N 75 The Effective Static Stability Experienced by Eddies in a Moist Atmosphere PAUL A. O GORMAN Massachusetts Institute of Technology, Cambridge, Massachusetts (Manuscript received
More information1/27/2010. With this method, all filed variables are separated into. from the basic state: Assumptions 1: : the basic state variables must
Lecture 5: Waves in Atmosphere Perturbation Method With this method, all filed variables are separated into two parts: (a) a basic state part and (b) a deviation from the basic state: Perturbation Method
More informationTraveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability
GEOPHYSICAL RESEARCH LETTERS, VOL. 39,, doi:10.1029/2012gl053684, 2012 Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability Daniela I. V. Domeisen
More informationUnderstanding inertial instability on the f-plane with complete Coriolis force
Understanding inertial instability on the f-plane with complete Coriolis force Abstract Vladimir Zeitlin Laboratory of Dynamical Meteorology, University P. and M. Curie and Ecole Normale Supérieure, Paris,
More informationAtmospheric dynamics and meteorology
Atmospheric dynamics and meteorology B. Legras, http://www.lmd.ens.fr/legras III Frontogenesis (pre requisite: quasi-geostrophic equation, baroclinic instability in the Eady and Phillips models ) Recommended
More information8/21/08. Modeling the General Circulation of the Atmosphere. Topic 4: Equatorial Wave Dynamics. Moisture and Equatorial Waves
Modeling the General Circulation of the Atmosphere. Topic 4: Equatorial Wave Dynamics D A R G A N M. W. F R I E R S O N U N I V E R S I T Y O F W A S H I N G T O N, D E P A R T M E N T O F A T M O S P
More informationThe general circulation of the atmosphere
Lecture Summer term 2015 The general circulation of the atmosphere Prof. Dr. Volkmar Wirth, Zi. 426, Tel.: 39-22868, vwirth@uni-mainz.de Lecture: 2 Stunden pro Woche Recommended reading Hartmann, D. L.,
More informationFor the operational forecaster one important precondition for the diagnosis and prediction of
Initiation of Deep Moist Convection at WV-Boundaries Vienna, Austria For the operational forecaster one important precondition for the diagnosis and prediction of convective activity is the availability
More informationGEF2200 atmospheric physics 2018
GEF2200 atmospheric physics 208 Solutions: thermodynamics 3 Oppgaver hentet fra boka Wallace and Hobbs (2006) er merket WH06 WH06 3.8r Unsaturated air is lifted (adiabatically): The first pair of quantities
More informationEdward Lorenz: Predictability
Edward Lorenz: Predictability Master Literature Seminar, speaker: Josef Schröttle Edward Lorenz in 1994, Northern Hemisphere, Lorenz Attractor I) Lorenz, E.N.: Deterministic Nonperiodic Flow (JAS, 1963)
More informationKelvin Helmholtz Instability
Kelvin Helmholtz Instability A. Salih Department of Aerospace Engineering Indian Institute of Space Science and Technology, Thiruvananthapuram November 00 One of the most well known instabilities in fluid
More informationA Proposed Test Suite for Atmospheric Model Dynamical Cores
A Proposed Test Suite for Atmospheric Model Dynamical Cores Christiane Jablonowski (cjablono@umich.edu) University of Michigan, Ann Arbor PDEs on the Sphere Workshop Monterey, CA, June/26-29/2006 Motivation
More informationStability of meridionally-flowing grounded abyssal currents in the ocean
Advances in Fluid Mechanics VII 93 Stability of meridionally-flowing grounded abyssal currents in the ocean G. E. Swaters Applied Mathematics Institute, Department of Mathematical & Statistical Sciences
More informationMixing and Turbulence
Mixing and Turbulence November 3, 2012 This section introduces some elementary concepts associated with mixing and turbulence in the environment. 1 Conserved Variables Studies of mixing of different airmasses
More information( u,v). For simplicity, the density is considered to be a constant, denoted by ρ 0
! Revised Friday, April 19, 2013! 1 Inertial Stability and Instability David Randall Introduction Inertial stability and instability are relevant to the atmosphere and ocean, and also in other contexts
More informationRobert J. Trapp Purdue University, West Lafayette, Indiana
10.6 DO SUPERCELL THUNDERSTORMS PLAY A ROLE IN THE EQUILIBRATION OF THE LARGE-SCALE ATMOSPHERE? Robert J. Trapp Purdue University, West Lafayette, Indiana Charles A. Doswell, III Cooperative Institute
More informationp = ρrt p = ρr d = T( q v ) dp dz = ρg
Chapter 1: Properties of the Atmosphere What are the major chemical components of the atmosphere? Atmospheric Layers and their major characteristics: Troposphere, Stratosphere Mesosphere, Thermosphere
More information2.1 Temporal evolution
15B.3 ROLE OF NOCTURNAL TURBULENCE AND ADVECTION IN THE FORMATION OF SHALLOW CUMULUS Jordi Vilà-Guerau de Arellano Meteorology and Air Quality Section, Wageningen University, The Netherlands 1. MOTIVATION
More informationGoal: Use understanding of physically-relevant scales to reduce the complexity of the governing equations
Scale analysis relevant to the tropics [large-scale synoptic systems]* Goal: Use understanding of physically-relevant scales to reduce the complexity of the governing equations *Reminder: Midlatitude scale
More information