diff --git a/enter/.obsidian/plugins/recent-files-obsidian/data.json b/enter/.obsidian/plugins/recent-files-obsidian/data.json index 0621457..c078c83 100644 --- a/enter/.obsidian/plugins/recent-files-obsidian/data.json +++ b/enter/.obsidian/plugins/recent-files-obsidian/data.json @@ -1,5 +1,25 @@ { "recentFiles": [ + { + "basename": "Gitea .readme", + "path": "Gitea .readme.md" + }, + { + "basename": "Particle Terms", + "path": "Machine Tips (Quantum)/Physics/Particle Terms.md" + }, + { + "basename": "Ions", + "path": "Machine Tips (Quantum)/Physics/Ions.md" + }, + { + "basename": "Optics", + "path": "Machine Tips (Quantum)/Physics/Optics.md" + }, + { + "basename": "Anti Charm Meson", + "path": "Machine Tips (Quantum)/Physics/Anti Charm Meson.md" + }, { "basename": "Environments & Interfaces", "path": "Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md" @@ -120,10 +140,6 @@ "basename": "4. 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First Step is Matrix Math.md", - "Machine Tips (Quantum)/Math/Visualizing the Quantum Space.md", "Untitled", - "Machine Tips (Quantum)/Math/Algorithms/Alg Collection/Grover's Search Algorithm.md", - "Coding Tips (Classical)/Project Vault/hi.mainsite/Resume-ish - my occupations.md", "Machine Tips (Quantum)/Project Vault/Papers/Shwetha Jayaraj CV.pdf", - "Coding Tips (Classical)/Terminal Tips/Languages/Fortran.md", "Coding Tips (Classical)/Project Vault/Obsidian/imgFiles/Pasted image 20230828113948.png", "Coding Tips (Classical)/Project Vault/Comms/WRITTEN TEXT/E-Mail Settings", "Coding Tips (Classical)/Project Vault/Comms/RADIO/TALK WITH SOUND", diff --git a/enter/Gitea .readme.md b/enter/Gitea .readme.md new file mode 100644 index 0000000..a6baac3 --- /dev/null +++ b/enter/Gitea .readme.md @@ -0,0 +1,6 @@ +Gitea .readme profile + + +1. Make a repository named .profile + + diff --git a/enter/Machine Tips (Quantum)/Physics/Particle Terms.md b/enter/Machine Tips (Quantum)/Physics/Particle Terms.md index c35ad1c..116bdca 100644 --- a/enter/Machine Tips (Quantum)/Physics/Particle Terms.md +++ b/enter/Machine Tips (Quantum)/Physics/Particle Terms.md @@ -65,3 +65,16 @@ +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) \ No newline at end of file diff --git a/enter/Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md b/enter/Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md index 1919e5e..f37189e 100644 --- a/enter/Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md +++ b/enter/Machine Tips (Quantum)/Resources/Code & Circuit Operations/Environments & Interfaces.md @@ -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. - - +