Response of the mesopause region dynamics to the February 2001 stratospheric warming

https://doi.org/10.1016/S1364-6826(03)00086-5Get rights and content

Abstract

The response of the mesosphere/lower-thermosphere (MLT) region to a major stratospheric warming in Europe during winter 2000/2001 has been investigated using mesopause-region winds measured by meteor radar or the LF-D1 method over three stations (Castle Eaton, 52°N; Collm, 52°N; and Esrange 68°N). The vertical wind structure measured over the three sites, and its time evolution, are found to be quite similar despite the different techniques used in the measurements. The effects of stratospheric warming are very clear, and are similar over both the mid-latitude and high-latitude sites. The warming resulted in a reversal of both the zonal and meridional wind. In the zonal component, this reversal was apparently associated with a planetary-wave oscillation with a period of ∼10 days. The effect was most conspicuous in the vertical prevailing wind gradients. The mesopause-region effects thus seem to be the results of a superposition of an intensifying planetary wave and a slow overall decrease in the strength of the zonal prevailing winds.

Introduction

Stratospheric warmings can dramatically change the structure of the entire middle-atmosphere wind and temperature fields up to the height of the mesosphere/lower thermosphere (MLT) region. This is particularly so in the case of major warmings, which occur when the meridional temperature gradient in the winter high-latitude stratosphere actually reverses as part of a complete breakdown of the stratospheric polar vortex.

The effects of stratospheric warmings on the MLT region have been observed since the 1970s, when measurements of pressure and wind variations revealed a connection between these two levels of the atmosphere (e.g. Lysenko et al., 1975; Lauter and Schminder, 1976). These MLT-region reactions to stratospheric warmings have been interpreted as representing a breakdown of the winter circulation and a return to quasi-summer conditions (Lauter and Entzian, 1982; Von Cossart et al., 1982). A number of subsequent studies have examined the influence of stratospheric warmings on MLT-region circulation. Often, these have taken the form of case studies examining time series or selected profiles of mesopause-region mean winds measured during one or a few winters. These studies have frequently reported that stratospheric warmings lead to a decrease in the westerly zonal prevailing wind, or even to a wind reversal (Gregory and Manson, 1975; Schminder and Kürschner 1981a, Schminder and Kürschner 1981b, Schminder and Kürschner 1990; Greisiger et al., 1984; Muller et al., 1985; Lysenko et al., 1990; Kazimirowsky, 1994; Jacobi et al., 1997). Some studies have also reported changes in the meridional prevailing winds (Schminder and Kürschner, 1981b; Muller et al., 1985).

The semidiurnal tide is arguably the most conspicuous feature of the dynamics of the mid- and high-latitude MLT region. However, in contrast to the distinct response of the MLT-region mean winds to stratospheric warmings, the influence that such warmings have on the semidiurnal tide is less well understood. Lauter and Schminder (1976) reported that the amplitude of the semidiurnal tide increased during the periods when MLT-region pressure fluctuated in connection with stratospheric warmings. Schminder and Kürschner (1981b) presented examples when the semidiurnal tidal phase changed during stratospheric warmings, although in other years the tide seemed not to be influenced by the warming events (Schminder and Kürschner, 1981a; Manson and Meek, 1985).

Kazimirowsky (1994) reported measurements of winds over Siberia and showed that, in some years, the phase of the semidiurnal tide increased during the time when the MLT-region zonal winds decrease or reverse during a stratospheric warming. However, he also noted that the particular interaction between stratosphere and upper mesosphere during stratospheric warmings depends on the peculiarities of the specific warming event. Jacobi et al. (1997) also noted this effect in several case studies of the effect of major stratospheric warmings on the MLT-region winds measured over Collm. These latter authors considered simultaneous measurements of stratospheric temperature and mesopause region winds and reported that the stratospheric warmings regularly are indeed connected with a strongly disturbed zonal wind field in the MLT region, but that the breakdown of the stratospheric polar vortex is not necessarily connected with the observation of easterly zonal winds in the upper mesosphere and lower thermosphere.

At greater altitudes, strong westerly winds are measured during some stratospheric warmings—which may be called a “compensation” effect. This effect may result from the vertical structure of stratospheric warmings. In particular, an upward motion can occur above the level of the strongest poleward acceleration due to planetary-wave/mean-flow interaction, which may lead to a cooling of the lower thermosphere, and subsequently to strong westerlies. Alternatively, changes in the filtering of ascending gravity waves due to the reversed flow in the stratosphere may lead to easterly (westward) winds in the lower thermosphere. Jacobi et al. (2001) showed that during the occurrence of this compensation effect the stratospheric warming influence on the MLT region also varies with longitude.

In contrast to the behaviour of the stratosphere, the “compensation effect” during (and also after) stratospheric warmings may lead to a particularly cold upper mesosphere at high latitudes during stratospheric warmings (Labitzke, 1972). Thus, the easterly winds of the disturbed stratosphere may decrease with height, and particularly strong westerly winds in the mesopause region may actually be observed in some cases. In fact, a recent comprehensive study using radar measurements made over 12 years found that the particular response of the MLT-region to individual warming events differed notably from case to case, and moreover, varied significantly with latitude and longitude (Hoffmann et al., 2002). Hence, although in many cases the beginning of a stratospheric warming is marked by a decrease in the prevailing westerly zonal wind of the upper mesosphere, this observation probably cannot be used to indicate further development of the stratospheric warming event in the course of the following days or weeks.

In summary, while the basic behaviour of stratospheric warmings is reasonably well understood, their effect on the MLT region is still uncertain, and highlights the need for additional measurements and case studies. In the following work, we shall present MLT-region wind measurements made over three European sites during the February 2001 major stratospheric warming event.

Section snippets

Measurements and data evaluation

Investigations of the effects of stratospheric warmings on the MLT region have often been handicapped in the past by the fact that some meteor radar measurements did not have explicit height finding, and therefore the vertical structure of the warming evolution could not be monitored in detail. Detailed studies of the effects of warmings throughout the mesosphere and above have only very recently been undertaken (Hoffmann et al., 2002). Some modern meteor radars are now able to routinely

The MLT wind field during January and February 2001

A stratospheric warming, and the subsequent effects on the MLT region, consist of a strong interaction between planetary waves and the mean circulation, starting in the stratosphere. Therefore we begin with a short description of the February 2001 major stratospheric warming, before presenting the equivalent MLT-region wind fields. The latter, when measured by radar, are usually decomposed into tides, mean winds and long-period oscillations, and we shall follow this procedure—although it should

Long-period variations

Considering the zonal prevailing wind time series of Fig. 2, only a weak indication of wave activity (in terms of discernable regular oscillations) is found over Collm. A more pronounced oscillation is seen over Castle Eaton and over ESRANGE. Hoffmann et al. (2002) also reported larger amplitudes of planetary waves over the Arctic than over Central Europe during stratospheric warmings. This is further illustrated in the amplitude spectra presented in Fig. 5. The zonal prevailing wind spectra

Wave-tidal interaction

The time series of the semidiurnal tidal amplitudes are shown in Fig. 8. Very distinctive day-to-day variability can be seen at each height and over all three measuring sites. However, careful inspection of the figure suggests that the characteristic periods appear to be different. This is also visible in the amplitude spectra in Fig. 9 (i.e., spectra of the amplitude time series for the semidiurnal tide), again calculated from the data of days No. 15–55. Over Castle Eaton, a period of about

Conclusions

During winter 2000/2001, mesopause region horizontal winds have been measured over three European sites using two meteor radars and the LF D1 method. The measurements were carried out during a major stratospheric warming and the responses of the MLT region to this warming were monitored. The warming effect was slightly different at different latitudes. At middle latitudes, the zonal prevailing winds at fixed heights show a response near the major phase of the stratospheric warming. Starting

Acknowledgments

This research has been partly supported by the German Ministry of Education and Science under 07ATF10 within the AFO2000 programme.

References (28)

Cited by (44)

  • Arctic polar vortex dynamics during winter 2006/2007

    2020, Polar Science
    Citation Excerpt :

    SSWs are recorded over the Arctic almost every year (Ageyeva et al., 2017). The consequences of major SSWs resulting from the polar vortex splitting can appear in the mesosphere and even in the thermosphere (Jacobi et al., 2003; Pancheva et al., 2008a, 2008b; Pancheva and Mukhtarov, 2011; Jin et al., 2012). Minor SSWs are recorded as a result of the polar vortex displacement, which in some cases is short-term (with the PSC keeping inside the vortex) and may not affect the subsequent springtime ozone depletion.

  • On the variability of tides during a major stratospheric sudden warming in September 2002 at Southern hemispheric extra-tropical latitude

    2019, Advances in Space Research
    Citation Excerpt :

    The SSW is believed to be triggered by the wintertime large scale planetary waves through deceleration of the polar vortex wind resulting in a partial or full split of the vortex and associated warming of the ambient stratosphere (Matsuno, 1971; Schoeberl, 1978; Guharay et al., 2014). The impact of the stratospheric polar vortex weakening and reversal of the wintertime eastward wind flow on the mesosphere and lower thermosphere (MLT) was investigated by a handful of previous studies (Singer et al., 1992; Jacobi et al., 2003; Dowdy et al., 2004). The warming and associated disturbances due to the SSW event generally lasts for 4–6 weeks (Schoeberl, 1978).

  • Comparison of the dynamical response of low latitude middle atmosphere to the major stratospheric warming events in the Northern and Southern Hemispheres

    2016, Journal of Atmospheric and Solar-Terrestrial Physics
    Citation Excerpt :

    Using UKMO zonal mean winds, Sathishkumar et al. (2009) noted enhanced westward flow in the upper stratosphere and lower mesosphere and eastward flow in the lower stratosphere during the MSW events. A number of studies have examined the influence of MSW on high latitude Mesosphere and Lower Thermosphere (MLT) circulation and they reported that MSW events frequently led to a decrease of the eastward zonal prevailing wind, or even wind reversal (Gregory and Manson, 1975; Jacobi et al., 1997 and references therein), although in some cases, Jacobi et al. (2003) noted zonal wind reversal over middle and high latitude sites and the reversal was apparently associated with a planetary wave oscillation of ~10 day. Hoffmann et al. (2002) noted latitudinal dependence of the wind reversal of eastward directed winds with reduced magnitudes towards the equator during MSW in 1998–99.

  • An enhancement of the lunar tide in the MLT region observed in the Brazilian sector during 2006 SSW

    2012, Journal of Atmospheric and Solar-Terrestrial Physics
    Citation Excerpt :

    Frequently, studies have reported that SSW events lead to a decrease in the zonal wind, or even to a wind reversal (e.g., Muller et al., 1985; Schminder and Kuerschner, 1990; Hoffmann et al., 2002). Furthermore, changes in the meridional winds have also been observed (e.g., Muller et al., 1985; Hoffmann et al., 2002; Jacobi et al., 2003). Effects of stratospheric warming on tidal propagation have been reported in some studies.

  • Planetary wave coupling of the atmosphere-ionosphere system during the Northern winter of 2008/2009

    2012, Advances in Space Research
    Citation Excerpt :

    This basic feature of the stratosphere–mesosphere manifestation of the SSW has been supported by many observations. A small but representative recent subset includes those by Hoffmann et al. (2002, 2007), Jacobi et al. (2003), Dowdy et al. (2004), Cho et al. (2004), Palo et al. (2005), Espy et al. (2005), Chshyolkova et al. (2006), Shepherd et al. (2007), Pancheva et al. (2008a, 2008b, 2009a, 2009b), Mukhtarov et al. (2010a), Pancheva and Mukhtarov (2011a). Besides the above mentioned normal modes very frequently PWs with long period, ∼23 days, are observed by ground-based and satellite measurements in the winter middle atmosphere (Pancheva and Mitchell, 2004; Pancheva et al., 2008a; Pancheva et al., 2009a,b; Lu et al., 2012).

View all citing articles on Scopus
View full text