相关实验视频
Updated: Jan 13, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
5.3K
在无线电干扰测量中的白.
E Paul Boven1,2,3, Jeroen C J Koelemeij4,5, Chantal van Tour4,5
1JIVE - Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, Dwingeloo, 7991PD the Netherlands.
概括
白协议精确地将时间和频率信号分布在光纤上,证明它适合无线电干扰计时钟同步. 这项技术支持高达15 GHz的观测频率,增强望远镜的连贯性.
科学领域:
- 天文学和天体物理学
- 网络工程 网络工程
- 信号处理 信号处理
背景情况:
- 无线电干扰测量需要精确的时间和频率同步以实现连贯的操作.
- 高速通信网络为分发这些信号提供了潜力.
- 白协议是为了在光纤上准确地分配时间和频率而设计的.
研究的目的:
- 评估用于同步无线电干扰仪的白协议的定量极限.
- 开发一种方法来量化由于白相位噪声而导致的敏感性损失.
- 为了评估白适合用于无线电天文学中的时钟分布.
主要方法:
- 开发了一种方法来量化白相位噪声的连贯性损失,包括闪相位噪声的新表达式.
- 设计了一个校准程序来测量部署光纤网络中的分散.
- 将白集成到具有共存数据流量的生产网络中,并对35公里和169公里光纤连接进行了非常长基线干扰测量 (VLBI) 实验.
主要成果:
- 由于白阶段噪声而导致的量化连贯性损失,显示预测值和测量值之间的良好一致.
- 证明了白信号与同一光纤上的数据流量成功共存.
- 确定标准的White Rabbit v3开关支持高达3.5 GHz,而低的版本支持高达15 GHz.
结论:
- 白是用于无线电干扰测量的时钟分布的可行解决方案.
- 开发的用于量化连贯性损失和测量分散的方法是有效的.
- 白通过精确的时间和频率同步,使无线电天文学中的高频观测成为可能.
相关概念视频
Atomic Emission Spectroscopy: Interference
589
In atomic emission spectroscopy (AES), high-temperature atomizers excite a broad range of elements and molecules that generate complex emissions from sources such as oxides, hydroxides, and flame combustion products in the flame or plasma. Several strategies can be employed to minimize spectral interferences caused by overlapping emission lines or bands. These include increasing instrument resolution, choosing alternative emission lines, optimally placing the detector in low-background regions,...
589
Infrared (IR) Spectroscopy: Overview
4.6K
When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
Different compounds display unique properties due to their...
4.6K
IR Spectrum
2.0K
When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0%...
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0%...
2.0K
Interference and Diffraction
51.6K
Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.
51.6K
IR Spectrometers
2.3K
There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
2.3K
IR Frequency Region: X–H Stretching
1.4K
In IR spectroscopy, signals produced by the X−H bonds (such as C−H, O−H, or N−H) can be observed in the frequency range of 2700–4000 cm–1. The C−H stretching vibration forms sharp bands in the region 2850–3000 cm–1. The presence of the O−H stretching vibration leads to the forming of an absorption band in the frequency range 3650–3200 cm−1. At the same time, N−H stretching can be confirmed by absorption bands in...
1.4K

