Timeline for Determining the size of a light source
Current License: CC BY-SA 4.0
17 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Jun 24, 2020 at 17:52 | vote | accept | Akerai | ||
| S Jun 24, 2020 at 17:52 | history | bounty ended | Akerai | ||
| S Jun 24, 2020 at 17:52 | history | notice removed | Akerai | ||
| Jun 24, 2020 at 2:16 | answer | added | mmesser314 | timeline score: 2 | |
| Jun 23, 2020 at 1:18 | answer | added | S. McGrew | timeline score: 3 | |
| Jun 23, 2020 at 1:03 | answer | added | Adam V. Steele | timeline score: 0 | |
| Jun 23, 2020 at 0:00 | history | tweeted | twitter.com/StackPhysics/status/1275217078153248768 | ||
| Jun 17, 2020 at 14:07 | comment | added | Akerai | @JoséAndrade It is a 4pi emitter in vacuum, among the available spatial-resolving diagnostics are only radiographs of different objects, large pinholes, slits, USAF targets. | |
| Jun 17, 2020 at 13:55 | comment | added | José Andrade | Can you provide more details about the experimental conditions? Is this in vacuum? What is available to you (ie cameras, scintillators, etc.)? Is the source directional or is it spherical? | |
| Jun 17, 2020 at 12:56 | comment | added | Akerai | @JoséAndrade In principle. In reality, in the COVID-19 world I currently don't. | |
| Jun 17, 2020 at 12:56 | history | edited | Akerai | CC BY-SA 4.0 |
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| S Jun 17, 2020 at 12:51 | history | bounty started | Akerai | ||
| S Jun 17, 2020 at 12:51 | history | notice added | Akerai | Canonical answer required | |
| Jun 13, 2020 at 13:49 | comment | added | José Andrade | That is macrosized when compared to the wavelength. I guess that if you are dealing with such sources you also have access to x-ray imaging optics. Can't you just image it via grazing incidence toroidal mirrors? | |
| Jun 13, 2020 at 12:37 | comment | added | Akerai | @Pieter 0.1 to 0.01nm, or 1-10keV | |
| Jun 13, 2020 at 12:37 | history | edited | Akerai | CC BY-SA 4.0 |
added 107 characters in body
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| Jun 13, 2020 at 12:12 | history | asked | Akerai | CC BY-SA 4.0 |