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Investigation of the intraseasonal oscillations over a Brazilian equatorial station: a case study
© Guharay et al.; licensee Springer. 2014
- Received: 9 May 2014
- Accepted: 16 October 2014
- Published: 11 November 2014
Characteristics of the intraseasonal oscillations (ISO) in the mesosphere and lower thermosphere (MLT) are investigated using meteor radar wind observations from a South American, equatorial station, São João do Cariri (7.4°S, 36.5°W) during 2008. A prominent ISO signature is observed during January-May in the period band approximately 40 to 70 days in the MLT zonal wind. In the lower atmosphere, a dominant ISO is observed in the period band approximately 30 to 60 days in the outgoing longwave radiation (OLR) (a proxy for convection), total columnar water vapor (a proxy for tides), and zonal wind. Considerable high correlation of the ISO between the MLT and lower atmosphere indicates significant dynamical coupling between the lower and middle atmosphere during the observational period. The MLT-ISO shows conspicuous downward propagation of the peak amplitude indicating the role of the dissipating upward propagating waves for its generation. The amplitudes in the zonal wind of the dominant tidal components in the MLT exhibit conspicuous ISO modulation. The eastward propagating waves and tides are surmised to be responsible for communicating the ISO signature from the lower atmosphere to the MLT. The origin of the MLT-ISO is believed to take place in the lower troposphere, below 4 km. The MLT-ISO is believed to be the imprint of the lower atmospheric Madden-Julian oscillation which travels eastward from the Indian Ocean-western Pacific Ocean to the present location.
- Intraseasonal oscillations
- Lower and middle atmosphere coupling
- Meteor radar observations
The mean dynamical state of the equatorial middle atmosphere is significantly controlled by large-scale long period oscillations, i.e., semiannual oscillations (SAO) and quasi-biennial oscillations (QBO) (Burrage et al. ; Baldwin et al. ; Guharay et al. [2014a]). These oscillations show downward propagation of their phases with altitude since they are driven by deposition of energy from upward propagating gravity waves, Rossby waves, Kelvin waves, etc. due to wave-mean flow interaction. Convective processes are believed to be the most important mechanism for driving these waves which cause the strong SAO and QBO in the stratosphere and comparatively weak oscillations in the mesosphere.
In addition to the aforesaid long period oscillations, the equatorial lower and middle atmosphere wind exhibits significant oscillations in the period range 20 to 100 days which are termed as instraseasonal oscillations (ISO). The ISO was first observed by Eckermann and Vincent () in the mesosphere and lower thermosphere (MLT) zonal wind in the period range 10 to 100 days with dominant periodicities in the bands approximately 60, 35 to 40, 20 to 25 days using medium-frequency (MF) radar at Christmas Island (2°N, 157°W). They reported a striking similarity of the observed ISO in the MLT with their tropospheric counterpart, i.e., Madden-Julian oscillation (MJO) as described by the earlier investigators (Madden and Julian , ). Later, Eckermann et al. () furthered the work with nearly 5 years of long-term data and reported dominant ISO in the MLT zonal wind at Christmas Island with periods approximately 60, 40, and 20 days. They also found strong ISO modulation of the gravity waves and diurnal tide.
The MJO in the equatorial troposphere is observed in the zonal wind and rainfall which is driven by the convective anomalies transpiring in the regions near the Indian Ocean and western and central Pacific Ocean (Madden and Julian ). Large-scale convective anomalies are generated over the tropical Indian Ocean and slowly propagate with diminishing strength through the western and central Pacific Ocean and later disappear in the eastern Pacific Ocean (Madden and Julian ). The MJO can be interpreted as a mixed Kelvin and Rossby waves near the source region and an eastward propagating Kelvin wave away from the source (Madden and Julian ). The MJO feature in the zonal wind exhibits an out-of-phase relationship in the lower and upper troposphere, and it decays drastically above the tropopause (Madden and Julian , ). Signatures of the MJO were also observed in the ocean heat flux and sea surface temperature which was inferred as being a result of interaction between the convective processes and large-scale circulations in the troposphere (Jones et al. ).
Although the MJO is a large-scale feature in the equatorial tropospheric zonal wind, it cannot propagate vertically upward to the MLT region due to its low phase speed (Eckermann et al. ). Eckermann et al. () suggested that the MJO-modulated tropospheric convection causes similar modulation of the intensity of the upward propagating gravity waves and nonmigrating diurnal tide, and as these waves break/dissipate in the MLT region, they drive intraseasonal variation in the ambient wind. Kumar and Jain () inferred that the tropospheric Rossby waves responsible for the MJO in the troposphere can propagate directly to the upper atmosphere. On the other hand, with global geopotential height observations, Ziemke and Stanford () argued that the upward propagating Rossby waves from the tropical region travel towards midlatitude and refract back to the tropical latitude near the stratopause and imprint the ISO of 1- to 2-month periods over Indian Ocean-western Pacific region. Recently, Niranjankumar et al. () found a signature of refraction of the tropical ISO through subtropical stratosphere in course of propagation from the lower to the middle atmosphere over an Indian tropical station, Gadanki (13.5°N, 79.2°E) which was supported by the most recent study by Guharay et al. ([2014b]) utilizing observations from two low latitude Brazilian stations.
Using the satellite-based high-resolution Doppler imager (HRDI), Lieberman () studied the MLT-ISO in the zonal mean zonal wind at ±20° latitude region and found maxima at 121, 72, and 33 days. They reported significant modulation of the gravity waves and tides by the ISO supporting the earlier findings of Eckermann et al. (). Using radar wind observations over Jakarta (6°S, 107°E), Pontianak (0°N, 109°E) and Christmas Island, Isoda et al. () inferred that the mesospheric ISO is not a feature of propagating disturbances; rather, it is a variation of the zonal mean flow. They observed clear ISO modulation of the MLT zonal wind and diurnal tidal amplitude implying an appreciable contribution of the diurnal tide originating from the lower atmosphere to the MLT-ISO. They also found biennial variability in the ISO amplitude of the zonal wind and zonal amplitude of the diurnal tide. Using global circulation model study, Miyoshi and Fujiwara () showed important role of ultrafast Kelvin wave and diurnal tide (migrating and nonmigrating) on excitation of the MLT-ISO. Recently, Kumar et al. () reported ISO in the MLT zonal wind over the Indian sector, Tirunelveli (8.7°N, 77.8°E) in two period bands approximately 50 to 70 days and 20 to 40 days which were consistent with the observed ISO in the outgoing longwave radiation (OLR) and water vapor, respectively. Rokade et al. () carried out a comparative study with radar wind observations from two Indian low latitude stations and found influence of the deep tropical convection on the variability of the observed MLT-ISO. Most recently, using 3 years of observations, Guharay et al. () showed existence of a dominant ISO in the period range 20 to 100 days at Gadanki (13.5°N, 79.4°E) with intermittent behavior in the troposphere, insignificant amplitude in the stratosphere, and consistent variability in the mesosphere.
Although a number of investigations of the ISO carried out over Indian Ocean-western pacific sector (convective anomaly source region) are available, observations from the South American region (away from the sources) are scarce. Recently, Rao et al. () studied longitudinal variability of the ISO using measurements over four equatorial stations located at different longitudinal sectors over the globe including the present site, but the study did not investigate the generation mechanism in detail. Therefore, in our present paper, we have studied the characteristics of the MLT-ISO at São João do Cariri (hereafter referred to as Cariri) (7.4°S, 36.5°W), its correspondence with the lower atmospheric counterpart, i.e., MJO, as well as the possible generation mechanism for excitation in the lower and middle atmosphere. It should be mentioned that the most coherent ISO feature over various atmospheric regions at the present station is found during early 2008 (not observed in other years), and hence, we have selected the year 2008 for the present study.
Instruments and database
Meteor radar wind
The horizontal winds utilized for the present study are obtained from a SKiYMET-type meteor radar installed at Cariri. The radar operates at a frequency of 35.24 MHz with pulse width 13 μs, peak power 12 kW, and pulse repetition frequency 2,144 Hz. It employs one three-element Yagi antenna for transmission. For receiving the backscattered signal from the meteor trails, it uses five-phase coherent two-element Yagi antennas aligned along two orthogonal baselines with one center antenna common to both. The radar is able to detect about 5,000 meteor echoes per day to derive angular position, range, and wind velocity components. The details of the derivation algorithm for estimating the horizontal winds can be found in the paper of Hocking et al. (). For the present work, we have used zonal and meridional winds of temporal resolution 1 h and vertical resolution of 3 km within the vertical range 81 to 99 km for the year 2008. Daily mean winds estimated from the hourly values are used for determining the ISO characteristics in the MLT.
In order to estimate the ISO features in the stratosphere and troposphere, we have utilized the ERA-Interim reanalysis database (Berrisford et al. ) available at 0.5° × 0.5° latitude-longitude grid provided by the European Centre for Medium-range Weather Forecasts (ECMWF) during the observational period. For the present purpose, we have used daily zonal wind at 37 pressure levels (1 to 1,000 hPa), i.e., 0 to 48 km altitude range at grid point 7.5°S, 36.5°W nearest to the location of Cariri. Data of the total columnar water vapor (TCWV) at 7.5°S, 36.5°W during the observational period are also utilized for studying the ISO activity. Furthermore, 10-m zonal wind is used as a proxy for surface wind (Foltz and McPhaden ) for the latitude range 10°N to 10°S and longitude range 0 to 360°E.
To investigate the convective activity during the observational period, we have utilized OLR data available at 2.5° × 2.5° latitude-longitude grid provided by the National Centers for Environmental Prediction (NCEP) as a proxy in the year 2008. Details of the OLR data can be found in the available literature (Kalnay et al. ). OLR data for the latitude range 10°N to 10°S and longitude range 0 to 360°E are considered for the present work. The closest available OLR grid point to Cariri is found to be 7.5°S, 37.5°W.
For studying the ISO in the lower atmosphere and MLT, we utilized the standard wave analysis tools. These include Lomb-Scargle periodogram, wavelet analysis, digital filter, and cross-correlation analysis.
The present study from an equatorial South American station (away from the convective anomaly region) reveals a prominent ISO signature in the period range approximately 40 to 70 days in the MLT region during January-May of the year 2008. The detailed study of the ISO reveals its significant relationship with the lower atmospheric MJO suggesting its origin at lower troposphere, and it should be mentioned that such relationship is not prominent in the available limited dataset.
The ISO amplitude is found to be appreciable near the upper troposphere, stratopause, and mid-lower MLT. The ISO originating in the troposphere cannot propagate directly up to the mesosphere due to their small phase speed. The waves with higher phase speed originating from the lower atmosphere are modulated by the ISO and carry their signature to the middle atmosphere. As they break/dissipate in the middle atmosphere, the ISO signature reappears in the mean flow variability. In the MLT, we have found a shift of the peak period towards lower values with altitude. In general, the high frequency waves with higher phase speed can propagate to higher altitudes as compared to their low frequency counterpart before they deposit their energy due to breaking/dissipation causing the appearance of the high frequency ISO at higher altitudes.
In the MLT, wavelet (Figure 2) profiles show clear downward propagation of the ISO peak amplitude supporting the notion of its generation by dissipation of the upward propagating waves. With satellite-based HRDI observations, Lieberman () observed prominent downward propagation of the ISO in the MLT and he inferred significant role of gravity waves in driving the ISO. The observational results of the present study support the inference of Lieberman ().
Convection is the most important driver of the various atmospheric waves in the lower atmosphere (Manzini and Hamilton ; Hagan and Forbes ; Alexander et al. ). Since the convective activity is modulated by the ISO, the intensity of the convection-driven waves is also modulated by the ISO (Eckermann et al. ). Therefore, common intuition expects good correlation of the ISO between the MLT and OLR (a proxy for convection) since water vapor and surface zonal wind do exhibit such a correlation (Figure 5b). On the contrary, our observed result shows small correlation of the ISO between the MLT and OLR at Cariri. Such a discrepancy is possibly due to the distant location of the present site from the convective active source region and may imply its global domination over the local convective condition. Most recently, Guharay et al. () reported less correlation between the OLR and ISO activity during certain times of the three years observational span from an Indian station and indicated some complex mechanisms which might influence the ISO characteristics besides convection.
We have found an indication of the atmospheric tides to drive the ISO in terms of modulation of the water vapor in the TS and tidal amplitude in the MLT. Since the observed correlation between the MLT-ISO and water vapor ISO is high (>0.5), we can infer that the tides generated by water vapor heating and latent heat release are the possible communicators of the tropospheric ISO to the MLT at the present location. As the observed ISO is most likely driven by the eastward waves, it is believed that the nonmigrating tides are dominant in the present scenario. Eckermann et al. () concluded that the nonmigrating diurnal tide modulated by the lower atmospheric convectively generated ISO can carry the ISO signature to the mesosphere. Using numerical simulation, Lieberman et al. () showed that the nonmigrating diurnal tides generated by the water vapor heating might communicate the tropospheric variability to the upper mesosphere in the course of their propagation. Isoda et al. () found a dominant role of the convection-driven nonmigrating diurnal tide in the generation of the MLT-ISO. Kumar et al. () observed 20 to 40 day oscillations in the water vapor at an Indian equatorial station indicating an important role of the tides towards driving the MLT-ISO. Gurubaran et al. () concluded that the nonmigrating diurnal tide generated due to latent heat release of water vapor associated with convection could dominate over the migrating component to determine the long-term behavior under certain conditions.
The correlation analysis between the MLT-ISO at various altitudes in the radar zonal wind and TS-ISO in the ERA-Interim zonal wind (Figure 6) suggests that the source region of the MLT-ISO is below 4 km wherein correlation is found to be maximum. Considerable increase of the correlation coefficients at some altitudes in the TS can be interpreted as enhancement of the ISO activity due to vertically intermittent dissipation of the propagating waves possibly due to local ambient dynamical conditions which require further investigation and could be pursued in our future study.
The estimated mean phase speed of the MJO anomaly in the OLR and surface wind in the troposphere is found to be 4.7 m/s in the Indian Ocean-western Pacific region which is very similar to that demonstrated in previous studies. Using OLR, wind, and temperature observations, Hendon and Salby () estimated the eastward MJO anomaly phase speed approximately 5 m/s which is very close to the present result. Recently, using OLR and surface wind observations, Yu et al. () calculated the MJO anomaly phase speed to be approximately 4.7 m/s resembling the present finding. Yu et al. () investigated the global propagation properties of the MJO, and they showed eastward propagation of the MJO anomaly signature from the Indian Ocean-western Pacific region to the tropical Atlantic through Central America and Panama. However, they did not find any appreciable extension of the MJO over the South American region during the temporal span of 2000–2006 although we have found a very prominent ISO signature in the lower and middle atmosphere in 2008 which may indicate interannual variability of the MJO anomaly propagation extent and the associated dynamics. In the present study, we have found a plausible role of the eastward propagating waves for communicating the ISO signature from lower to middle atmosphere as the lower atmospheric background wind remains westward during January-May. It should be mentioned that during certain times of the year, there may be a possible role of the westward Rossby waves coming from the Indian Ocean region since the present observational location lies close to the western Atlantic. Yu et al. () suggested that the westward propagating Rossby waves could be strong enough due to interaction with the eastward propagating MJO over the tropical Atlantic region during boreal summer and fall. The westward propagating dominant oscillations of period approximately 25 to 60 days associated with the West African monsoon can influence the tropical Atlantic Ocean dynamics significantly (Thorncroft et al. ; Sultan and Janicot ).
The present investigation from an equatorial South American station, Cariri reveals a prominent feature of the ISO in the MLT zonal wind during January-May of 2008 as well as a conspicuous relationship with the lower atmospheric MJO signature indicating lower atmospheric origin. The dominant period of the ISO is found to be approximately 40 to 70 days in the MLT zonal wind and approximately 30 to 60 days in the lower atmospheric variables, i.e., OLR, TCWV, and tropospheric zonal wind. Significant correlation of the ISO between the TCWV and MLT zonal wind as well as modulation of the tidal amplitudes in the ISO period band may suggest a contribution of the atmospheric tides to the existing ISO coupling of the lower and middle atmosphere. The observed smaller correlation of the ISO between the MLT zonal wind and OLR is possibly due to distant location of the present site from the convective anomaly region where the MJO is excited. The ISO amplitude is observed to be significant in the upper troposphere, upper stratosphere, and mid-lower MLT. The MLT-ISO shows evident downward phase progression indicating upward propagation of the dissipating waves responsible for its generation. The high frequency waves with higher phase speeds are surmised to dissipate at higher altitudes. The eastward propagating gravity waves, Kelvin waves, and nonmigrating tides are possibly responsible for driving the ISO at Cariri. The eastward waves are supported by the westward background wind during the enhanced ISO activity period. The excitation of the MLT-ISO is believed to transpire in the lower atmosphere, below 4 km. There is an indication of the vertically intermittent dissipation of the ISO-modulated propagating waves at certain altitudes in the TS which may contribute to the MLT-ISO. The MJO anomaly signature in the lower atmosphere is found to propagate eastward from the Indian Ocean-western Pacific Ocean to reach the present longitude sector causing ISO activity in the tropical middle atmosphere.
AG sincerely acknowledges the support of the Fundação de Amparo a Pesquisa do Estado de São Paulo (FAPESP) to the present research work. The authors are thankful to the NCEP team for providing the OLR data. The authors are grateful to the ECMWF team for providing the ERA-interim dataset which is available at http://apps.ecmwf.int/datasets/data/interim_full_daily/. The wavelet software used in the present work is provided by C. Torrence and G. P. Compo and available at http://paos.colorado.edu/research/wavelets/.
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