Like most celestial objects, pulsars have poles, and when they’re faced towards Earth, we can see the rotating light pulses these mysterious objects emit, hence their given name. The first pulsar was discovered by Professor Dame Jocelyn Bell in 1967 when she was a PhD student at the Univers...
pulsarmicrostructureradio pulsestellar atmospheremagnetospherePSR 0833-45PSR 1749-28We present an analysis of pulsar observations carried out on two frequency channels at 1634 MHz and 1650 MHz with a time resolution of 62.5 ns on the 70-m radio telescope of the NASA Deep Space Network in Tidbin...
Space has real physical, electrical properties, called permittivity and permeability. We know this because the speed of light is determined by them. What gives properties to space must have a certain structure. There has been speculation about an aether, modelled as a fluid that fills all space ...
Pulsar Microstructure Quasi-Periodicity Polarization has been detected to preferentially change state at the edges of micropulses and subpulses. Finally, it is noted that data shows that quasi-periodicities have the same period at different radio frequencies in different pulsars... V Boriakoff,DC Fe...
In the early 1970s, a source that radiates short pulses of radio energy, called a pulsar (pulsating radio source), was discovered in the Crab Nebula. Visual inspection of this radio source revealed it to be a small star centered in the nebula. The first neutron star had been discovered. ...
It’s not the particles that move outwards but the pulses of light giving the misleading appearance of a “jet”. A pulsar, a star that rapidly pulsates, is very probably a “black hole” as seen from an exact polar perspective. A universe-wide electric network There are strong ...
More specifically, Sazhin [2] suggested that the arrival times of pulsar's pulses could be used for direct searches of gravitational radiation and shortly after Detweiler [3] made a similar point by deriving one of the first upper limits on the relic gravitational waves in the nHz range. ...
Using seven radio telescopes in Australia, the US and Europe, the researchers monitored the double pulsar system between its discovery in 2003 until 2019. They found that the radio pulses consistently arrived later than expected, and calculated this was because they were being deflected...
The formidable magnetic fields of these entities produce high-powered columns of radiation, which can sweep past the Earth like lighthouse beams, creating what's known as a pulsar. The properties of neutron stars are utterly out of this world — a single teaspoon of neutron-star material would...
stage. If they don’t explode, like novae, they degenerate to red giant status and fade out. As with stars, the color of the fireballs is probably an indication of their plasma temperature. Continuing the stellar analogy, instances of revolving sunspots and pulsar behavior were not uncommon....