Evaluation of Second–Order Zeeman Frequency Shift in NTSC-F2

2021 ◽  
Author(s):  
Jun-Ru Shi ◽  
Xin-Liang Wang ◽  
Yang Bai ◽  
Fan Yang ◽  
Yong Guan ◽  
...  
Sensors ◽  
2021 ◽  
Vol 21 (24) ◽  
pp. 8333
Author(s):  
Yang Bai ◽  
Xinliang Wang ◽  
Junru Shi ◽  
Fan Yang ◽  
Jun Ruan ◽  
...  

Second-order Zeeman frequency shift is one of the major systematic factors affecting the frequency uncertainty performance of cesium atomic fountain clock. Second-order Zeeman frequency shift is calculated by experimentally measuring the central frequency of the (1,1) or (−1,−1) magnetically sensitive Ramsey transition. The low-frequency transition method can be used to measure the magnetic field strength and to predict the central fringe of (1,1) or (−1,−1) magnetically sensitive Ramsey transition. In this paper, we deduce the formula for magnetic field measurement using the low-frequency transition method and measured the magnetic field distribution of 4 cm inside the Ramsey cavity and 32 cm along the flight region experimentally. The result shows that the magnetic field fluctuation is less than 1 nT. The influence of low-frequency pulse signal duration on the accuracy of magnetic field measurement is studied and the optimal low-frequency pulse signal duration is determined. The central fringe of (−1,−1) magnetically sensitive Ramsey transition can be predicted by using a numerical integrating of the magnetic field “map”. Comparing the predicted central fringe with that identified by Ramsey method, the frequency difference between these two is, at most, a fringe width of 0.3. We apply the experimentally measured central frequency of the (−1,−1) Ramsey transition to the Breit-Rabi formula, and the second-order Zeeman frequency shift is calculated as 131.03 × 10−15, with the uncertainty of 0.10 × 10−15.


1999 ◽  
Vol 38 (Part 1, No. 10) ◽  
pp. 6174-6177 ◽  
Author(s):  
Sung Hoon Yang ◽  
Kwang Jae Baek ◽  
Taeg Yong Kwon ◽  
Young Bum Kim ◽  
Ho Seong Lee

Author(s):  
Toshihiro Konishi ◽  
Keisuke Okuno ◽  
Shintaro Izumi ◽  
Masahiko Yoshimoto ◽  
Hiroshi Kawaguchi

Author(s):  
В.В. Егоров ◽  
С.А. Лобов ◽  
М.Л. Маслаков ◽  
А.Н. Мингалев

Рассмотрена задача оценки доплеровского смещения несущей частоты информационного одночастотного фа- зоманипулированного сигнала, если информационная последовательность неизвестна. Приведено описание метода оценки с использованием разности фаз первого и второго порядков. Представлены результаты численного моделирования. The problem of Doppler frequency shift estimation of the single-tone information signal with phase-shiftkeying modulation under conditions when the information sequence is unknown is considered. The description of the estimation method using the firstand second-order phase difference is given. The results of the numerical simulation are presented.


2013 ◽  
Vol E96.C (4) ◽  
pp. 546-552 ◽  
Author(s):  
Toshihiro KONISHI ◽  
Keisuke OKUNO ◽  
Shintaro IZUMI ◽  
Masahiko YOSHIMOTO ◽  
Hiroshi KAWAGUCHI

Author(s):  
Keisuke OKUNO ◽  
Toshihiro KONISHI ◽  
Shintaro IZUMI ◽  
Masahiko YOSHIMOTO ◽  
Hiroshi KAWAGUCHI

1983 ◽  
Vol 30 (3) ◽  
pp. 423-461
Author(s):  
J. B. Ehrman

The nonlinear saturation of a resistive modified tearing mode in a toroidal plasma is calculated by Simon saturation theory for a weakly linearly unstable (over-stable) regime. The linearly unstable mode is a (1, 1) mode, where the first 1 indicates n, the toroidal mode number about an axisymmetric equilibrium and the second 1 indicates the multiple of the non-zero frequency at which the n = 1 mode oscillates when linearly marginally stable. The saturation amplitude is found to be proportional to (Δ – Δc)½ where Δ, a measure of the driving energy of the instability, is proportional to the difference between the logarithmic derivatives of the radial (i.e. perpendicular to the magnetic surface) perturbation magnetic field in the simplest case, and Δc measures toroidal stabilization due to average magnetic line curvature. To obtain the Simon saturation condition, one must go to third order in the small parameter (Δ –Δc)½. Starting with (1, 1), (1, – 1),( – 1, – 1), and( –1, 1 ) modes in first order in (Δ – Δc)½, the modes (0, 0), (0, 2), (2, 2), (2, 0) are obtained in second order, and these are driven with first-order modes to a third-order (1,1) mode which yields a saturation condition. In the quasi-linear approximation, only the near-zero frequency modes (0, 0) and (2, 0) are considered in the second order. In the present paper, only the axisymmetric perturbation (0,0) is used in second order. This gives a relation between nonlinear saturation amplitude and frequency shift, but does not determine either uniquely because of the undetermined parameter γ in the perturbation solutions. This parameter is determined exactly by the requirement of finiteness of the solutions when the (2, 0) non-axisymmetric near-zero frequency perturbation is taken into account in second order. However, magnetic island width at saturation can still be estimated taking only the (0,0) second order mode because this width depends so insensitively on γ, namely as γ–¼. Under this restriction to (0, 0) in second order, the frequency shift is found to be negative. Its absolute value is proportional to Δ – Δc, while the magnetic island width is proportional to (Δ – Δc)¼ and has a scale determined by t, the thickness of the resistive layer, proportional to η⅓, the cube root of the electrical resistivity.


1991 ◽  
Vol 44 (5) ◽  
pp. 459 ◽  
Author(s):  
BT McCann ◽  
RE Robson

A simplified, physically intuitive model of diffuse scattering of radio waves from a rough surface is used to present a self-contained derivation of first- and second-order cross sections, essentially in agreement with the standard expressions. Incoherent addition of the second-order contributions (electromagnetic and hydrodynamic) leads to a cross section which is slightly different from the more rigorously derived cross sections of Barrick (1972b) and Johnstone (1975). A surface current v has been incorporated in this model, with the main change to the cross section being a frequency shift of the entire spectrum by an amount Llw = -2ko . v.


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