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相关概念视频

Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Phasors01:12

Phasors

Phasors are a powerful mathematical tool used to analyze alternating current (AC) circuits. They provide a complex number representation of sinusoids, with the magnitude of the phasor equating to the amplitude of the sinusoid and the angle of the phasor representing the phase measured from the positive x-axis.
One of the significant benefits of using phasors is that they simplify the analysis of AC circuits by eliminating the time dependence of the current and voltage. This transformation...
Doppler Effect - II01:05

Doppler Effect - II

The Doppler effect has several practical, real-world applications. For instance, meteorologists use Doppler radars to interpret weather events based on the Doppler effect. Typically, a transmitter emits radio waves at a specific frequency toward the sky from a weather station. The radio waves bounce off the clouds and precipitation and travel back to the weather station. The radio frequency of the waves reflected back to the station appears to decrease if the clouds or precipitation are moving...
Doppler Effect - I00:56

Doppler Effect - I

The Doppler effect and Doppler shift were named after the Austrian physicist and mathematician Christian Johann Doppler in 1842, who conducted experiments with both moving sources and moving observers. Consider an observer standing on a street corner, observing an ambulance with a siren sound passing by at a constant speed. The observer experiences two characteristic changes in the sound of the siren. Initially, the sound increases in loudness as the ambulance approaches and decreases in...
IR Frequency Region: Fingerprint Region01:03

IR Frequency Region: Fingerprint Region

IR spectra are divided into two main regions: the diagnostic region and the fingerprint region. The diagnostic region of the spectrum lies above 1500 cm−1. The absorptions resulting from single-bond vibrations of the N–H, C–H, and O–H stretch at higher wavenumbers and appear on the left side of the spectrum. The stretching absorptions of the C≡C and C≡N occur between 2100–2300 cm−1. In contrast, those arising from stretching absorptions of the C=O, C=N, and C=C occur between 1600–1850 cm−1.
The...
Gas Chromatography: Types of Detectors-II01:19

Gas Chromatography: Types of Detectors-II

In gas chromatography, different detectors are employed to meet specific analytical needs. These detectors are often categorized based on their detection mechanisms and the types of compounds they are best suited to analyze. Thermal Conductivity Detectors (TCD), Flame Ionization Detectors (FID), and Electron Capture Detectors (ECD) represent common categories, each with unique operating principles and applications. However, beyond these, several other detectors are designed for more specialized...

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相关实验视频

Updated: Jul 11, 2026

Time Multiplexing Super Resolving Technique for Imaging from a Moving Platform
06:25

Time Multiplexing Super Resolving Technique for Imaging from a Moving Platform

Published on: February 12, 2014

雷达检测恐惧症的雷达检测

S J Ostro, R F Jurgens, D K Yeomans

    Science (New York, N.Y.)
    |March 24, 1989
    PubMed
    概括

    雷达研究揭示了Phobos的存在.

    科学领域:

    • 行星科学 行星科学
    • 雷达天文学 雷达天文学
    • 小人体的特征描述

    背景情况:

    • 火星最大的卫星博斯是了解太阳系中小型天体的关键目标.
    • 之前对博的表面特性进行的研究是有限的.
    • 雷达观测提供了一种独特的方法来探测地下特征.

    研究的目的:

    • 用雷达回声来调查博斯的表面特性.
    • 为了确定博星的 regolith 的物理特征.
    • 为了比较福博斯的雷达信号与其他小型太阳系天体.

    主要方法:

    • 分析了来自博斯3.5厘米波长的雷达回声.
    • 测量了福博斯的雷达阿尔贝多,极化比和回声光谱形状.
    • 与小行星和月球的数据比较福博斯的雷达信号.

    主要成果:

    • 在厘米到十米的尺度上,博斯表现出比月球更光滑的表面.
    • 博的最上层规流体的平均体积密度大约为2.0gcm(-3).
    • 博斯的雷达信号与接近地球的物体不同,但与大型C类小行星相似.

    结论:

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    Tracking Infiltration Front Depth Using Time-lapse Multi-offset Gathers Collected with Array Antenna Ground Penetrating Radar

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    Last Updated: Jul 11, 2026

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    Published on: February 12, 2014

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    Published on: February 12, 2013

    Tracking Infiltration Front Depth Using Time-lapse Multi-offset Gathers Collected with Array Antenna Ground Penetrating Radar
    07:14

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    Published on: May 1, 2018

    • 福博斯的表面和浅地底与主带小行星有共同的特征.
    • 雷达数据表明,福博斯的起源或进化路径可能不同于以前的假设.
    • 进一步的雷达研究可以完善我们对福博斯的组成和历史的理解.