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ENCYCLOPEDIA OF RADIO ELECTRONICS AND ELECTRICAL ENGINEERING
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Op-amp capacitance meter. Encyclopedia of radio electronics and electrical engineering

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Encyclopedia of radio electronics and electrical engineering / Measuring technology

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The principle of operation of a capacitor capacitance meter from several picofarads to 5 μF is based on measuring the alternating current flowing through the capacitor under test.

Op-amp capacitance meter

An alternating current of a rectangular shape is generated by an oscillator on the operational amplifier A1. The repetition frequency of the pulses issued by the generator depends on the capacitance of one of the capacitors C1-C6 and the position of the variable resistor R5 slider. Depending on the measurement subrange, it varies from 100 Hz to 200 kHz. Trimmer resistor R1* symmetricalize the shape of rectangular oscillations at the output of the generator. In order for the measurement error in the very first subrange (50 pF) not to exceed 10%, the internal resistance of the device must be at least 3 kOhm.

The required measurement range is set by switch S1. The capacitance meter is powered by a stabilized bipolar source with a voltage of 8 ... 15 V. The values ​​​​of the frequency-setting capacitors C1-C6 may differ from those indicated in the diagram by 20%, but must have high temperature and time stability. The instrument is calibrated using reference capacitors. Since the alternating voltage at the output of the generator is bipolar, it is impossible to measure the capacitance of electrolytic capacitors with this device.

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New source of cosmic rays 31.10.2012

Researchers from the CNRS (French National Center for Scientific Research) and CEA have discovered a new source of cosmic rays while working with the European astronomical X-ray satellite XMM-Newton. It is located in close proximity to the Arches Star Cluster, not far from the center of our Milky Way galaxy.

Particles of this radiation are accelerated in a shock wave generated by tens of thousands of young Arch stars moving in roughly the same direction at about 700000 km/h. These cosmic rays, interacting with the atoms of the surrounding gas, produce characteristic X-rays. But the origin of these cosmic rays is different from the usual radiation that arises from supernova explosions. It was discovered exactly one hundred years ago by the Austrian physicist Victor Franz Hess. He discovered the existence of ionizing radiation of extraterrestrial origin, which he called cosmic rays. Modern astrophysicists understand their nature very well - when some stars explode and become supernovae at the end of their lives, their matter is ejected at supersonic speed, creating shock waves that accelerate particles. As a result, some atomic nuclei receive very high kinetic energy and enter the Earth's atmosphere.

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The authors of the article began by studying X-rays, which theoretically should generate low-energy cosmic rays in the interstellar medium. They then looked for signs of this emission in X-ray data collected by the XMM-Newton telescope over more than a decade of operation.

By analyzing the X-ray properties of interstellar iron from satellite records, they found traces of large, fast-moving ion populations. They come from the vicinity of the Arches star cluster, located at a distance of about a hundred light-years from the center of our Milky Way galaxy. In all likelihood, they occur when the stars of the Arch at high speed collide with a gas cloud on their way. In this particular region, the energy density of accelerated ions is thousands of times greater than that of cosmic rays in the vicinity of the solar system.

This is the first time that a major source of low-energy cosmic rays has been discovered outside the solar system. Everything points to the fact that gas and dust clouds, and not only shock waves of supernovae, as was thought until now, can give high speeds to ions.

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