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CRAB PULSAR (PSR B0531+21) sound - YouTube
https://www.youtube.com/watch?v=ewCApzryDho
The Crab Pulsar (PSR B0531+21) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which...
Crab Pulsar | StarDate Online
https://stardate.org/radio/program/2020-02-11
The pulsar produces a “wind” of charged particles that sculpts the interior of the surrounding cloud. And it causes the pulsar to slow down — but only by about ten millionths of a second per year. So the Crab Pulsar will keep spinning for a long time to come. More about pulsars tomorrow. Script by Damond Benningfield
Pulsar Audio | High-end audio software
Pulsar Mu is way more than a vari-mu compressor/limiter to my ears. It’s instant character on everything it touches, just running audio through it. It’s sculpting audio information to their very core. It’s pure fun to use on literally every source material, with the most powerful side chain section you can think of today and one hell of a sound.
Pulsars I.
https://www.naic.edu/~astro/School/Talks/cordes_pulsar1.pdf
Pulsar Sounds Radio signals demodulated into audio signals B1937+21 1.56 642 J0437-4715 5.7 174 33 30.2 B0531+21 (Crab) 89 11.2 B0833-45 (Vela) B0950+08 253 3.9 B0329+54 714 1.4 f=1/P (Hz) P (ms) Pulsar sound file J0437 -4715 profile
Audio files - Astrosurf
http://www.astrosurf.com/luxorion/audiofiles-pulsar.htm
Here are audio files related to pulsars. They were recorded at Jodrell Bank Observatory. You will find on this page recordings of QSOs worked by radio amateurs, including with ISS, the sound of different transmission modes and interferences, as well as recordings of historical events. You will find on this page recordings related to astronautic events, transmissions from satellite and …
Crab Pulsar - Wikipedia
https://en.wikipedia.org/wiki/Crab_Pulsar
The period of the pulsar's rotation is increasing by 38 nanoseconds per day due to the large amounts of energy carried away in the pulsar wind. The Crab Nebula is often used as a calibration source in X-ray astronomy. It is very bright in X-rays, and the flux density and spectrum are known to be constant, with the exception of the pulsar itself. The pulsar provides a strong periodic …
Multifrequency Radio Observations of the Crab Pulsar ...
https://ui.adsabs.harvard.edu/abs/1996ApJ...468..779M/abstract
Previously unseen profile components of the Crab pulsar have been discovered in a study of the frequency-dependent behavior of its average pulse profile between 0.33 and 8.4 GHz. One new component, 36° ahead of the main pulse at 1.4 GHz, is not coincident with the position of the precursor at lower frequencies. Two additional, fiat-spectrum components appear after the …
CRABTIME - Crab Pulsar Timing - NASA
https://heasarc.gsfc.nasa.gov/W3Browse/all/crabtime.html
The Declination of the Crab Pulsar. The assumed pulsar position used in the reductions is as follows: RA (1950.0) 05 31 31.406 DEC (1950.0) +21 58 54.391 RA (J2000) 05 34 31.973 DEC (2000.0) +22 00 52.061 LII The Galactic Longitude of the Crab Pulsar. BII The Galactic Latitude of the Crab Pulsar. Day The day of the ephemeris entry. Month
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