scholarly journals A Precipitation Seesaw Mode between Northeast Asia and Siberia in Summer Caused by Rossby Waves over the Eurasian Continent

2008 ◽  
Vol 21 (11) ◽  
pp. 2401-2419 ◽  
Author(s):  
Koki Iwao ◽  
Masaaki Takahashi
Keyword(s):  
Rossby Waves ◽  
Northeast Asia ◽  
Low Frequency ◽  
Northern Eurasia ◽  
The North ◽  
Meridional Winds ◽  
Low Pass ◽  
Precipitation Anomalies ◽  
The Difference ◽  
Stretching Effect

Abstract There is a dominant seesaw pattern in summertime precipitation between northeast Asia and Siberia. Examined here is a mechanism of the seesaw mode, focusing on quasi-stationary Rossby waves propagating on two upper-tropospheric waveguides along the Asian jet and over northern Eurasia. Empirical orthogonal function (EOF) analysis to the low-frequency (10-day low-pass filtered) variation during summer reveals wave-propagation patterns on both of the waveguides. The time evolution of the two composite fields, constructed using the obtained EOF modes for each phase of the seesaw mode, was investigated by the wave-activity flux. In both composite fields, eastward-propagating Rossby waves originating from the North Atlantic–European sector branch off around eastern Europe onto the two waveguides, which become out of phase toward the east because of the difference in longitudinal wavelengths along them. This results in opposite phase anomalies of meridional winds over northeast Asia and Siberia. Budget analyses of vorticity, heat, and water vapor on a day with significant wave patterns along the two waveguides revealed the main balances; the zonal advection of vorticity anomalies around the tropopause was partly balanced by an anomalous stretching effect over these two regions, and the adiabatic heating anomalies in the midtroposphere associated with the stretching effect around the tropopause were balanced with diabatic heating anomalies, explained by condensation heating related to the precipitation anomalies. These events occur frequently in July, when the climatological precipitation is the largest, particularly over northeast Asia.

RESULTS OF A DIFFERENTIAL OMEGA TEST IN THE MACKENZIE RIVER DELTA

Geophysics ◽  
1970 ◽  
Vol 35 (3) ◽  
pp. 514-520
Author(s):  
L. W. Sobczak ◽  
G. J. Taylor
Keyword(s):  
New York ◽  
Navigation System ◽  
Low Frequency ◽  
Department Of Energy ◽  
The Arctic ◽  
The North ◽  
Radio Navigation System ◽  
The Difference ◽  
Area North ◽  
North Atlantic Area

In 1969 the Gravity Division of the Observatories Branch, Department of Energy, Mines and Resources, Ottawa, in cooperation with the Research, Development, and Programming Division of the Telecommunications and Electronics Branch of the Department of Transport, undertook an evaluation of the worldwide Omega Navigation System in the Arctic for the Polar Continental Shelf Project. Omega is a long‐range, very low frequency radio navigation system. It consists of 4 (Norway, Trinidad, Hawaii, and New York) of the planned 8 transmitters and provides navigational coverage for the North Atlantic area, North America, and parts of South America (Scull, 1969 and Dick‐Peddie, 1968). These stations presently transmit two frequencies (10.2 kHz and 13.6 kHz) in a sequential pattern synchronized in phase by means of atomic clocks (Tracor, 1968 and Findlay, 1968). The Omega receiver measures the difference of phase of received signals from a pair of transmitters. This measurement defines one line of position (LOP) in a family of hyperbolic lines. Lines of positions defined by the zero phase difference are the lines of position that are numbered on an Omega chart, and the distance between two such lines is known as a lane. A position is determined by the intersection of two lines of position within known lanes.

Energy Transmission by Barotropic Rossby Waves Revisited

2005 ◽  
Vol 35 (11) ◽  
pp. 2228-2236 ◽  
Author(s):  
R. P. Matano ◽  
E. D. Palma
Keyword(s):  
Cross Section ◽  
Rossby Waves ◽  
Bottom Topography ◽  
Low Frequency ◽  
Energy Transmission ◽  
Low Pass ◽  
Mid Atlantic Ridge ◽  
High Frequency Waves ◽  
The Individual ◽  
Matching Techniques

Abstract This article presents a semianalytic method to investigate the properties of energy transmission across bottom topography by barotropic Rossby waves. The method is first used to revisit the analytical estimates derived from wave-matching techniques and Wentzel–Kramers–Brillouin (WKB) approximations. The comparison between the semianalytic method and WKB indicates that the results of the latter are valid for waves with periods longer than a month and ridges taller than ∼1000 m and wider than ∼500 km. For these parameter values both methods predict the passage of low-frequency waves and the reflection of high-frequency waves. The semianalytic method is then used to discuss the energy transmission properties of a cross section of the Mid-Atlantic Ridge. It is shown that the filtering characteristics of realistic bottom topographies depend not only on the spatial scale set by the cross-section envelope, but also on the scales of the individual peaks. This dependence is related to the fact that topographies narrower than ∼400 km (e.g., peaks) are high-pass filters of incoming waves, while topographies wider than that (e.g., cross-section envelopes) are low-pass filters. In the particular case of the Mid-Atlantic Ridge the neglect of the contribution of individual peaks leads to an erroneous estimate of the filtering properties of the massif.

scholarly journals Investigating Nonlinear Dependence between Climate Fields

2017 ◽  
Vol 30 (14) ◽  
pp. 5547-5562
Author(s):  
Matt J. Fischer
Keyword(s):  
Kernel Methods ◽  
Low Frequency ◽  
Kernel Functions ◽  
Nonlinear Dependence ◽  
Directional Derivatives ◽  
Nonlinear Coupling ◽  
Low Pass ◽  
Gradient Based ◽  
The Difference ◽  
Response Field

The Earth’s ice–ocean–atmosphere system exhibits nonlinear responses, such as the difference in the magnitude of the atmospheric response to positive or negative ocean or sea ice anomalies. Two classes of methods that have previously been used to investigate the nonlinear dependence between climate fields are kernel methods and neural network methods. In this paper, a third methodology is introduced: gradient-based kernel dimension reduction. Gradient-based kernel methods are an extension of conventional kernel methods, but gradient-based methods focus on the directional derivatives of the regression surface between two fields. Specifically, a new gradient-based method is developed here: gradient kernel canonical correlation analysis (gKCCA). In gKCCA, the canonical directions maximize the directional derivatives between the predictor field and the response field, while the canonical components of the response field maximize the correlation with a nonlinear augmentation of the predictor canonical components. Gradient-based kernel methods have several advantages: their components can be directly related to the original fields (unlike in conventional kernel methods), and the projection vectors are determined by analytical solution (unlike in neural networks). Here gKCCA is applied to the question of nonlinear coupling between high-frequency (2–3 years) and low-frequency (4–6 years) modes in the Pacific Ocean. The leading gKCCA subspace shows a significant nonlinear coupling between the low-pass and high-pass fields. The paper also shows that the results of gKCCA are robust to different levels of noise and different kernel functions.

scholarly journals Northward Propagation, Initiation, and Termination of Boreal Summer Intraseasonal Oscillations in a Zonally Symmetric Model

2019 ◽  
Vol 76 (2) ◽  
pp. 639-668 ◽  
Author(s):  
Qiu Yang ◽  
Boualem Khouider ◽  
Andrew J. Majda ◽  
Michèle De La Chevrotière
Keyword(s):  
Warm Pool ◽  
Hadley Cell ◽  
Boreal Summer ◽  
Symmetric Model ◽  
The North ◽  
Beta Effect ◽  
Northward Propagation ◽  
Meridional Winds ◽  
Intraseasonal Oscillations ◽  
Precipitation Anomalies

AbstractA simple multilayer zonally symmetric model, using a multicloud convective parameterization and coupled to a dynamical bulk atmospheric boundary layer, is used here to simulate boreal summer intraseasonal oscillations (BSISO) in the summer monsoon trough and elucidate the underlying main physical mechanisms responsible for their initiation, propagation, and termination. Northward-moving precipitating events initiated near the equator propagate northward at roughly 1° day−1 and terminate near 20°N. Unlike earlier findings, the northward propagation of precipitation anomalies in this model is due to the propagation of positive moisture anomalies in the northward direction, resulting from an asymmetry in the meridional velocity induced by the beta effect. From a moisture-budget perspective, advection constitutes a biased intrusion of dry air into the convection center, forcing new convection events to form north of the wave disturbance, while moisture convergence supplies the precipitation sink. The BSISO events are initiated near the equator when the competing effects between first-baroclinic divergence and second-baroclinic convergence, induced by the descending branch of the Hadley cell and in situ congestus heating, respectively, become favorable to convective intensification. The termination often near 20°N and halfway stalling of these precipitating events occur when the asymmetry in the first-baroclinic meridional winds weakens and when the negative moisture gradient to the north of the convection center becomes too strong as the anomaly exits the imposed warm pool domain.

scholarly journals An Analysis of Low- and High-Frequency Summer Climate Variability around the Caribbean Antilles

2012 ◽  
Vol 25 (11) ◽  
pp. 3942-3952 ◽  
Author(s):  
Isabelle Gouirand ◽  
Mark R. Jury ◽  
Bernd Sing
Keyword(s):  
Climate Variability ◽  
North Atlantic ◽  
High Frequency ◽  
Low Frequency ◽  
Late Summer ◽  
Summer Climate ◽  
The North ◽  
Tropical North Atlantic ◽  
Low Pass ◽  
The Caribbean

This study contrasts the pattern of low-frequency (LF) and high-frequency (HF) climate variability in the eastern Caribbean. A low-pass Butterworth filter is used to study oscillations in rainfall and regional SST on time scales of greater and less than 8 yr in the period 1901–2002. The results show that the southern and northern Antilles are dominated by HF variability, whereas rainfall fluctuations in the eastern Antilles oscillate at quasi-decadal periods over the 102-yr record. In the southern Antilles, the HF rainfall signal derives from a late-summer response to the ENSO phase: warm and dry versus cool and wet. In the northern Antilles, the HF signal relates to a combination of an ENSO and North Atlantic Oscillation (NAO) phase: a warm ENSO and a negative NAO bring wetter conditions, while a cool ENSO and a positive NAO bring drier conditions. The early rainfall LF signal in SST is characterized by a dipole between the North Atlantic and South Atlantic and is associated with cross-equatorial winds that promote convection in the Caribbean. The study analyzes the upper-ocean structure—in particular, a low (high) salinity signal in the tropical North Atlantic (North Pacific) that relates to LF (HF) climate variability.

scholarly journals Influence of the Barotropic Mean Flow on the Width and the Structure of the Atlantic Equatorial Deep Jets

2014 ◽  
Vol 44 (9) ◽  
pp. 2485-2497 ◽  
Author(s):  
Martin Claus ◽  
Richard J. Greatbatch ◽  
Peter Brandt
Keyword(s):  
Rossby Waves ◽  
Current System ◽  
Low Frequency ◽  
Water Model ◽  
Kelvin Wave ◽  
Mean Flow ◽  
The North ◽  
Basin Mode ◽  
The Mean ◽  
Equatorial Rossby Waves

Abstract A representation of an equatorial basin mode excited in a shallow-water model for a single high-order baroclinic vertical normal mode is used as a simple model for the equatorial deep jets. The model is linearized about both a state of rest and a barotropic mean flow corresponding to the observed Atlantic Equatorial Intermediate Current System. It was found that the eastward mean flow associated with the North and South Intermediate Counter Currents (NICC and SICC, respectively) effectively shields the equator from off-equatorial Rossby waves. The westward propagation of these waves is blocked, and focusing on the equator due to beta dispersion is prevented. This leads to less energetic jets along the equator. On the other hand, the westward barotropic mean flow along the equator reduces the gradient of absolute vorticity and hence widens the cross-equatorial structure of the basin mode. Increasing lateral viscosity predominantly affects the width of the basin modes’ Kelvin wave component in the presence of the mean flow, while the Rossby wave is confined by the flanking NICC and SICC. Independent of the presence of the mean flow, the application of sufficient lateral mixing also hinders the focusing of off-equatorial Rossby waves, which is hence an unlikely feature of a low-frequency basin mode in the real ocean.

Realization of Enhanced LMS Filter Using Carry Skip Adder And Quantum Dot Cellular Automation In VLSI For Removing Impulse Noises In Medical Image

2019 ◽  
Vol 14 ◽  
Author(s):  
K.R. Shankarkumar ◽  
Gokul Kumar
Keyword(s):  
Adaptive Filtering ◽  
Adaptive Filters ◽  
Pass Band ◽  
Least Mean Square ◽  
Low Pass ◽  
Parallel Prefix ◽  
Loop Feedback ◽  
Band Pass ◽  
The Difference ◽  
Prefix Adder

: Filtering is an important step in the field of image processing to suppress the required parts or to remove any artifacts present in it. There are different types of filters like low pass, high pass, Band pass, IIR, FIR and adaptive filtering etc.., in these filters adaptive filters is an important filter because it is used to remove the noisy signal and images. Least Mean Square filter is a type of an adaptive filtering which is used to remove the noises present in the medical images. The working of LMS is based on the minimization of the difference between the error images using a closed loop feedback. Therefore presented technique called as Q-CSKA. Here the CSKA performs its operation in stages which is based on the nucleus stage. In the traditional CSKA the nucleus stage is depend on the parallel prefix adder in this work it is replaced by the QCA adder. The QCA adder utilizes the less area compared to PPA and it can be realized in Nanometer range also. For multiplexers, And OR Invert, OR and Invert logic is used to reduce the area and delay. Due to these advantages of the QCA, AOI-OAI logic the proposed method outperformed the LMS implementation in area, power, and accuracy and delay, this based five type image noise of medical pictures related to the best technique is out comes. It helps to medicinal practitioner to resolve the symptoms of patient with ease.

scholarly journals A Low frequency Southern Sky Survey Using the Mauritius Radio Telescope

2002 ◽  
Vol 199 ◽  
pp. 25-31
Author(s):  
N. Udaya Shankar
Keyword(s):  
Radio Telescope ◽  
Low Frequency ◽  
Fourier Synthesis ◽  
North East ◽  
The North ◽  
Sky Survey ◽  
Correlation Receiver ◽  
Complex Correlation ◽  
Right Ascension ◽  
East West

The Mauritius Radio Telescope (MRT) is a Fourier synthesis instrument which has been built to fill the gap in the availability of deep sky surveys at low radio frequencies in the southern hemisphere. It is situated in the north-east of Mauritius at a southern latitude of 20°.14 and an eastern longitude of 57°.73. The aim of the survey with the MRT is to contribute to the database of southern sky sources in the declination range −70° ≤ δ ≤ −10°, covering the entire 24 hours of right ascension, with a resolution of 4' × 4'.6sec(δ + 20.14°) and a point source sensitivity of 200 mJy (3σ level) at 151.5 MHz.MRT is a T-shaped non-coplanar array consisting of a 2048 m long East-West arm and a 880 m long South arm. In the East-West arm 1024 fixed helices are arranged in 32 groups and in the South arm 16 trolleys, with four helices on each, which move on a rail are used. A 512 channel, 2-bit 3-level complex correlation receiver is used to measure the visibility function. At least 60 days of observing are required for obtaining the visibilities up to the 880 m spacing. The calibrated visibilities are transformed taking care of the non-coplanarity of the array to produce an image of the area of the sky under observation.This paper will describe the telescope, the observations carried out so far, a few interesting aspects of imaging with this non-coplanar array and present results of a low resolution survey (13' × 18') covering roughly 12 hours of right ascension, and also present an image with a resolution of 4' × 4'.6sec(δ + 20.14°) made using the telescope.

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