论文标题
天线的射频发射源
Antenna source of radio-frequency emission in ion-proton pulsars
论文作者
论文摘要
在离子和质子的向外移动束中，纵向或准纵向的langmuir模式的生长形成了离子 - 普罗希望的脉冲星的开放扇区，作为一个终止喂养的高速赋予的高速公路水平水平直线的末期的类似物，是一整形的半波动的数量。辐射广泛地具有广泛观察到的能量通量，线性极化和光谱指数：另外，在某些集成的脉冲曲线中看到的缺口现象自然发生。低于100 MHz的PULSAR观测的新领域可能会导致无线电发射机制的生产性测试。
The growth of a longitudinal or quasi-longitudinal Langmuir mode in the outward-moving beam of ions and protons that forms the open sector of an ion-proton pulsar magnetosphere radiates as an analogue of an end-fed high-impedance horizontal straight-wire antenna an integral number of half-waves in length. The radiation has, broadly, the energy flux, linear polarization and spectral index that are widely observed: also, the notch phenomenon seen in some integrated pulse profiles occurs naturally. The new field of pulsar observations below 100 MHz may lead to productive tests of the radio emission mechanism.
