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Updated: Wednesday, August 30,2023-08-30 17:06:51

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shwetha729 2023-08-30 17:06:54 -04:00
parent f947d8d680
commit 052cb5ad34
5 changed files with 65 additions and 32 deletions
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40
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enter/Gitea .readme.md 100644
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Gitea .readme profile
1. Make a repository named .profile

13
enter/Machine Tips (Quantum)/Physics/Particle Terms.md
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The term quasar - Quasi stellar radio telescope - The term "quasar" was first used in an article by [astrophysicist](https://en.wikipedia.org/wiki/Astrophysicist "Astrophysicist") [Hong-Yee Chiu](https://en.wikipedia.org/wiki/Hong-Yee_Chiu "Hong-Yee Chiu") in May 1964, in _[Physics Today](https://en.wikipedia.org/wiki/Physics_Today "Physics Today")_, to describe certain astronomically puzzling objects:[[14]](https://en.wikipedia.org/wiki/Quasar#cite_note-14)
> So far, the clumsily long name "quasi-stellar radio sources" is used to describe these objects. Because the nature of these objects is entirely unknown, it is hard to prepare a short, appropriate nomenclature for them so that their essential properties are obvious from their name. For convenience, the abbreviated form "quasar" will be used throughout this paper.
Now we know them as black holes.
E-VLBI -
VLBI has traditionally operated by recording the signal at each telescope on [magnetic tapes](https://en.wikipedia.org/wiki/Magnetic_tape_data_storage "Magnetic tape data storage") or [disks](https://en.wikipedia.org/wiki/Hard_disk_drive "Hard disk drive"), and shipping those to the correlation center for replay. In 2004 it became possible to connect VLBI radio telescopes in close to real-time, while still employing the local time references of the VLBI technique, in a technique known as e-VLBI. In Europe, six [radio telescopes](https://en.wikipedia.org/wiki/Radio_telescopes "Radio telescopes") of the [European VLBI Network (EVN)](https://en.wikipedia.org/wiki/European_VLBI_Network "European VLBI Network") were connected with Gigabit per second links via their National Research Networks and the Pan-European research network [GEANT2](https://en.wikipedia.org/wiki/GEANT2 "GEANT2"), and the first astronomical experiments using this new technique were successfully conducted.[[15]](https://en.wikipedia.org/wiki/Very-long-baseline_interferometry#cite_note-JIVE2004-15)
The image to the right shows the first science produced by the European VLBI Network using e-VLBI. The data from each of the telescopes were routed through the [GÉANT2](https://en.wikipedia.org/wiki/G%C3%89ANT2 "GÉANT2") network and on through [SURFnet](https://en.wikipedia.org/wiki/SURFnet "SURFnet") to be the processed in real time at the European Data Processing centre at [JIVE](https://en.wikipedia.org/wiki/Joint_Institute_for_VLBI_in_Europe "Joint Institute for VLBI in Europe").[[15]](https://en.wikipedia.org/wiki/Very-long-baseline_interferometry#cite_note-JIVE2004-15)

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enter/Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md
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@ -35,4 +35,4 @@ There are several competing quantum computing platforms and environments in the
- view the quick start pdf
- used for QX Quantum Code - a different assembly language
- The [QX Simulator](http://quantum-studio.net/) is a universal quantum circuit simulator developed at QuTech by Nader Khammassi. The QX allows quantum algorithm designers to simulate the execution of their quantum circuits on a quantum computer. The simulator defines a low-level quantum assembly language namely Quantum Code which allows the users to describe their circuits in a simple textual source code file. The source code file is then used as the input of the simulator which executes its content.
-