Talk:China Fusion Engineering Test Reactor

magnetic pressure shocks / magnetic pressure oscillations (push towards a small area and release repeatedly) are crucial for fusion

but it's hard to:

1. achieve enough pressure
2. find the optimal frequency

• some prefer the turbulent oscillations (4 different oscillative frequencies which are non harmonious and cause turbulence; an other technique is the combined "turbulent oscillations of many frequencies at different topologies" and then "harmonious altogether compression to merge that chaos" again and again "turbulent and harmonious oscillations alternatively" (you hope that chaos to cause few fusions, and it actually works)

edit made to main article

Hi I'm a student at sydney university , making an edit as part of a unit assignment. Please offer some feedback for the edit made. Thank you.TechnicolourKaleidoscope (talk) 07:59, 2 June 2021 (UTC)

A good edit. Thank you. Please check out the Fusion power page and copy/paste across relevant material from the CFETR page to that page, e.g., on the economics. So, as a top-level page, Fusion power should include the edits you have made on e.g., Economics and Safety, as well as a subsection on the CFETR. Also, sign your edits, like I have done.Johncdraper (talk) 12:59, 1 June 2021 (UTC)

Thank you so much for the feedback , i will get on to doing an edit on the fusion power page. would you be able to reassess this page by any chance, I completely understand if you aren't willing to do so. thank you.TechnicolourKaleidoscope (talk) 07:59, 2 June 2021 (UTC)

I have removed the stub class flags on the page but cannot edit the flags on this Talk page as I am not a member of the two groups - only members can edit. However, you could join the groups yourself on their pages and then edit the classes. Johncdraper (talk) 08:59, 2 June 2021 (UTC)

Future

150 MK is ten times the temperature of the sun's core, not three. google it! Wikkileaker (talk) 04:17, 1 August 2021 (UTC)