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- ItemCharacteristics and sources of gravity waves observed in noctilucent cloud over Norway(München : European Geopyhsical Union, 2014) Demissie, T.D.; Espy, P.J.; Kleinknecht, N.H.; Hatlen, M.; Kaifler, N.; Baumgarten, G.Four years of noctilucent cloud (NLC) images from an automated digital camera in Trondheim and results from a ray-tracing model are used to extend the climatology of gravity waves to higher latitudes and to identify their sources during summertime. The climatology of the summertime gravity waves detected in NLC between 64 and 74° N is similar to that observed between 60 and 64° N by Pautet et al. (2011). The direction of propagation of gravity waves observed in the NLC north of 64° N is a continuation of the north and northeast propagation as observed in south of 64° N. However, a unique population of fast, short wavelength waves propagating towards the SW is observed in the NLC, which is consistent with transverse instabilities generated in situ by breaking gravity waves (Fritts and Alexander, 2003). The relative amplitude of the waves observed in the NLC Mie scatter have been combined with ray-tracing results to show that waves propagating from near the tropopause, rather than those resulting from secondary generation in the stratosphere or mesosphere, are more likely to be the sources of the prominent wave structures observed in the NLC. The coastal region of Norway along the latitude of 70° N is identified as the primary source region of the waves generated near the tropopause.
- ItemSolar 27-day signatures in standard phase height measurements above central Europe(Katlenburg-Lindau : EGU, 2019) von Savigny, Christian; Peters, Dieter H.W.; Entzian, GünterWe report on the effect of solar variability at the 27-day and the 11-year timescales on standard phase heightmeasurements in the ionospheric D region carried out in cen-tral Europe. Standard phase height corresponds to the re-flection height of radio waves (for constant solar zenith dis-tance) in the ionosphere near 80 km altitude, where NO isionized by solar Lyman-αradiation. Using the superposedepoch analysis (SEA) method, we extract statistically highlysignificant solar 27-day signatures in standard phase heights.The 27-day signatures are roughly inversely correlated to so-lar proxies, such as the F10.7 cm radio flux or the Lyman-αflux. The sensitivity of standard phase height change to so-lar forcing at the 27-day timescale is found to be in goodagreement with the sensitivity for the 11-year solar cycle,suggesting similar underlying mechanisms. The amplitude ofthe 27-day signature in standard phase height is larger duringsolar minimum than during solar maximum, indicating thatthe signature is not only driven by photoionization of NO. Weidentified statistical evidence for an influence of ultra-longplanetary waves on the quasi 27-day signature of standardphase height in winters of solar minimum periods.
- ItemQuantification of waves in lidar observations of noctilucent clouds at scales from seconds to minutes(Göttingen : Copernicus, 2013) Kaifler, N.; Baumgarten, G.; Fiedler, J.We present small-scale structures and waves observed in noctilucent clouds (NLC) by lidar at an unprecedented temporal resolution of 30 s or less. The measurements were taken with the Rayleigh/Mie/Raman lidar at the ALOMAR observatory in northern Norway (69 N) in the years 2008-2011. We find multiple layer NLC in 7.9% of the time for a brightness threshold of δ β 12 × 10-10 m-1 sr-1. In comparison to 10 min averaged data, the 30 s dataset shows considerably more structure. For limited periods, quasi-monochromatic waves in NLC altitude variations are common, in accord with ground-based NLC imagery. For the combined dataset, on the other hand, we do not find preferred periods but rather significant periods at all timescales observed (1 min to 1 h). Typical wave amplitudes in the layer vertical displacements are 0.2 km with maximum amplitudes up to 2.3 km. Average spectral slopes of temporal altitude and brightness variations are-2.01 ± 0.25 for centroid altitude,-1.41 ± 0.24 for peak brightness and-1.73 ± 0.25 for integrated brightness. Evaluating a new single-pulse detection system, we observe altitude variations of 70 s period and spectral slopes down to a scale of 10 s. We evaluate the suitability of NLC parameters as tracers for gravity waves.
- ItemModeling Antarctic tides in response to ice shelf thinning and retreat(Hoboken, NJ : Blackwell Publishing Ltd, 2014) Rosier, S.H.R.; Green, J.A.M.; Scourse, J.D.; Winkelmann, R.Tides play an important role in ice sheet dynamics by modulating ice stream velocity, fracturing, and moving ice shelves and mixing water beneath them. Any changes in ice shelf extent or thickness will alter the tidal dynamics through modification of water column thickness and coastal topography but these will in turn feed back onto the overall ice shelf stability. Here, we show that removal or reduction in extent and/or thickness of the Ross and Ronne-Filchner ice shelves would have a significant impact on the tides around Antarctica. The Ronne-Filchner appears particularly vulnerable, with an increase in M2 amplitude of over 0.5 m beneath much of the ice shelf potentially leading to tidally induced feedbacks on ice shelf/sheet dynamics. These results highlight the importance of understanding tidal feedbacks on ice shelves/streams due to their influence on ice sheet dynamics.
- ItemA linear model for amplitude modulation of Langmuir waves in weak electron-beam plasma interaction(Göttingen : Copernicus, 2013) Baumgärtel, K.A simple linear approach to the phenomenon of amplitude modulation of Langmuir waves in weak beam plasma interaction is presented. During the short growth phase of the instability and within the longer period after saturation, the waves are described by their linear kinetic dispersion properties.The amplitude modulation appears as result of the beating of waves with different wavelengths and amplitudes that have grown from noise in the initial phase. The Langmuir wave fields are calculated via FFT (fast Fourier transform) technique. The resulting waveforms in temporal representation are quite similar to those observed by spacecraft.
- ItemCoherent amplitude modulation of electron-beam-driven Langmuir waves(Göttingen : Copernicus, 2013) Baumgärtel, K.A linear approach to the phenomenon of irregular amplitude modulation of beam-driven Langmuir waves, developed in a previous paper, is extended to explain periodic modulation as well. It comes about by beating of the fastest growing mode of the instability with beam-aligned plasma oscillations. They are naturally generated in a uniform domain of beam-plasma interaction prior to the onset of the instability. Particle-in-cell (PIC) simulations support the results of the linear analysis.