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EHT Collaboration
At the time, all ingredients of the process were speculative, but the new observations confirm the Blandford-Znajek idea. “What we see in our image is ordered polarization in a spiral shape,” said Issaoun, who was involved in analyzing the polarization measurements. “And the shape of the magnetic field is also spiral … which means it’s able to launch a jet.”
“I’m very chuffed,” Znajek, now a retired Cambridge city councilor, said by email.
Moreover, the new observations point to one of two rival versions of the Blandford-Znajek process that have been developed and explored in hundreds of computer simulations in recent decades, known as the MAD and SANE jet-launching scenarios. These competing ideas paint opposing pictures of a black hole’s milieu and, in particular, the origin and strength of its magnetic field.

Related Keywords

Kyle Parfrey , Ramesh Narayan , Sasha Philippov , Harvard University , Princeton University , With Kerr , Andrew Chael , Event Horizon Telescope , Astrophysics , Black Holes , Computational Astrophysics , Galaxies , Physics , ரமேஷ் நாராயண் , ஹார்வர்ட் பல்கலைக்கழகம் , ப்ரிந்ஸ்டந் பல்கலைக்கழகம் , உடன் கெர் , ஆண்ட்ரூ சாயல் , நிகழ்வு அடிவானம் தொலைநோக்கி , வானியற்பியல் , கருப்பு துளைகள் , கணக்கீட்டு வானியற்பியல் , விண்மீன் திரள்கள் , இயற்பியல் ,

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