Sentence examples for emissions shock from inspiring English sources
The SC also caused an impulsive enhancement of dayside auroral emissions (shock aurora) as observed by the hyperspectral all-sky imager NORUSCA II at Barentsburg and the meridian scanning photometer at Longyearbyen (both at Svalbard).
This was attributed to emission of shock-heated plasma in the wind wind interaction zone located between the stars.
Here we used the high photosensitive and spatiotemporal resolution images to detect the diffuse auroral emissions during the shock compression.
This emission is thought to be synchrotron emission from electrons shock accelerated to hundreds of TeV, and thus represents strong evidence that cosmic rays are accelerated in SNR shocks.
We analyzed the emission through comparison with the H2 line emission of several shock models.
These include the evolution of solar radio emissions associated with shocks driven by coronal mass ejections and searches for coherent radio emission from supernova remnants and relativistic jets.
The temperature dependence of the measured peak OH∗ emission from the shock tube and the peak OH∗ concentration from a homogeneous closed reactor model are compared.
Using ground-based high temporal and spatial optical aurora observations, we investigated one fortuitous event to illustrate the direct responses of the fine structure auroral emission to interplanetary shock on 7 January 2005.
We modelled their broadband behaviour as the sum of the standard forward shock emission due to the interaction of a fireball with the circum-burst medium and an additional component.
Exponential fit on the intensity maxima of the harmonic emission provided a shock speed of ∼580 990 km s−1, consistent with the average speed of the associated EUV wave front of 626 km s−1.
