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

enter/.obsidian/plugins/recent-files-obsidian/data.json

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@@ -139,14 +159,8 @@
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enter/Gitea .readme.md

@@ -0,0 +1,6 @@
+Gitea .readme profile 
+
+
+1. Make a repository named .profile
+
+

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)

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.
-	- 
+