Global normal mode planetary wave activity: a study using TIMED/SABER observations from the stratosphere to the mesosphere-lower thermosphere

被引:23
作者
John, Sherine Rachel [1 ]
Kumar, Karanam Kishore [1 ]
机构
[1] Vikram Sarabhai Space Ctr, Space Phys Lab, Thiruvananthapuram 695022, Kerala, India
关键词
Middle atmospheric dynamics; Planetary waves; Interhemispheric propogation; TIMED/SABER; 5-DAY WAVE; LAMB WAVES; ESRANGE; 68-DEGREES-N; TRAVELING-WAVES; ROSSBY WAVES; TEMPERATURE; RADAR; PERIOD; WINTER; 21-DEGREES-E;
D O I
10.1007/s00382-016-3046-2
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
A comprehensive study of three normal mode travelling planetary waves, namely the quasi-16, -10 and -5 day waves, is carried out globally using 5 years (2003-2007) of TIMED/SABER temperature measurements from the stratosphere to the mesosphere-lower thermosphere (MLT) by employing the two dimensional Fourier decomposition technique. From preliminary analysis, it is found that significant amplitudes of normal modes are confined to wave numbers-2 (westward propagating modes) to 2 (eastward propagating modes). The westward propagating quasi 16-day waves with zonal wave number 1 (W1; W1 refers to westward propagating wave with zonal wave number 1) peaks over winter-hemispheric high latitudes with northern hemisphere (NH) having higher amplitudes as compared to their southern hemispheric (SH) counterpart. The W1 quasi 16-day waves exhibit a double peak structure in altitude over winter hemispheric high latitudes. The eastward propagating quasi 16-day waves with wave number 1 (E1; E1 refers to eastward propagating wave with zonal wave number 1) exhibits similar features as that of W1 waves in the NH. In contrast, the E1 quasi 16-day waves in the SH show larger amplitudes as compared to the W1 waves and they do not exhibit double peak structure in altitude. Similar to the quasi 16-day waves, the quasi 10- and 5-day wave amplitudes with respect to their wavenumbers are delineated. Unlike quasi-16 and -10 day waves, quasi-5 day waves peak during vernal equinox both in the SH and NH. The peak activity of the W1 quasi-5 day wave is centered around 40A degrees N and 40A degrees S exhibiting symmetry with respect to the equator. A detailed discussion on the height-latitude structure, interannual variability and inter-hemispheric propagation of quasi 16-, 10- and 5-day waves are discussed. The significance of the present study lies in establishing the 5-year climatology of normal mode planetary waves from the stratosphere to the MLT region including their spatial-temporal evolution, which are very important from the middle atmospheric dynamics standpoint.
引用
收藏
页码:3863 / 3881
页数:19
相关论文
共 55 条
  • [31] The 16-day planetary wave in the mesosphere and lower thermosphere
    Mitchell, NJ
    Middleton, HR
    Beard, AG
    Williams, PJS
    Muller, HG
    [J]. ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES, 1999, 17 (11): : 1447 - 1456
  • [32] MEAN ZONAL ACCELERATION AND HEATING OF THE 70-KM TO 100-KM REGION
    MIYAHARA, S
    PORTNYAGIN, YI
    FORBES, JM
    SOLOVJEVA, TV
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1991, 96 (A2) : 1225 - 1238
  • [33] Numerical simulation of the 5-day and 16-day waves in the mesopause region
    Miyoshi, Y
    [J]. EARTH PLANETS AND SPACE, 1999, 51 (7-8): : 763 - 772
  • [34] Miyoshi Y, 1999, J ATMOS SCI, V56, P1698, DOI 10.1175/1520-0469(1999)056<1698:ANEOEO>2.0.CO
  • [35] 2
  • [36] Climatology of the stationary planetary waves seen in the SABER/TIMED temperatures (2002-2007)
    Mukhtarov, P.
    Pancheva, D.
    Andonov, B.
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2010, 115
  • [38] Seasonal variation of the quasi 5 day planetary wave: Causes and consequences for polar mesospheric cloud variability in 2007
    Nielsen, K.
    Siskind, D. E.
    Eckermann, S. D.
    Hoppel, K. W.
    Coy, L.
    McCormack, J. P.
    Benze, S.
    Randall, C. E.
    Hervig, M. E.
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2010, 115
  • [39] Planetary wave coupling from the stratosphere to the thermosphere during the 2002 Southern Hemisphere pre-stratwarm period
    Palo, SE
    Forbes, JM
    Zhang, X
    Russell, JM
    Mertens, CJ
    Mlynczak, MG
    Burns, GB
    Espy, PJ
    Kawahara, TD
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2005, 32 (23) : 1 - 5
  • [40] Intra-seasonal oscillations observed in the MLT region above UK (52°N, 2°W) and ESRANGE (68°N, 21°E) -: art. no. 2084
    Pancheva, D
    Mitchell, NJ
    Younger, PT
    Muller, HG
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2003, 30 (21) : 2 - 1