Slide 1 RF Cavity of CIS Xiaoying Pang Mar. 12 th, 2007 IUCF Slide 2 Present Design of CIS Energy=25MeV The Lowest frequency f=16.6MHz HARM=1(for the MPI cavity) We can choose…

Slide 1 Particle acceleration and plasma heating in the chromosphere Alexander Stepanov, Pulkovo Observatory, St.Petersburg, Russia Valery Zaitsev Institute of Applied Physics,…

Observational Evidence for Magnetic Reconnection in the Solar Corona Len Culhane Mullard Space Science Laboratory University College London SUMMARY Change in field connectivity…

Mini-research project Participants are divided into ≈6 teams. Each team includes 2-4 members and is supervised by Yokoyama or Isobe or ChenPF Each team works on a research…

PowerPoint Presentation The Sun 1 Solar Prominence Sun Fact Sheet The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. Diameter: 1,390,000 km (Earth…

Status of the Cold BPM Developments at CEA Saclay and Fermilab L-Band Cavity BPM: Nathan Eddy, Andrei Lunin, Eric Pirtle, Gennady Romanov, Nikolay Solyak, Seughwan Shin,…

Mini-research project Participants are divided into ≈6 teams. Each team includes 2-4 members and is supervised by Yokoyama or Isobe or ChenPF Each team works on a research…

PowerPoint Presentation The Sun 1 Solar Prominence Sun Fact Sheet The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. Diameter: 1,390,000 km (Earth…

Characterization of Heating and Cooling in Solar Flares Characterization of Heating and Cooling in Solar Flares Ryan Payne Advisor: Dana Longcope Solar Flares General Solar…

No. Name No. Name 1 Front cap 51 O-Ring 2 Backstop 52 Gear box 3 Sliding cover 53 oil cover 4 Steel ball 54 Tappered-gear shaft 5 Welle 55 Distance Welle 6 O-Rin 56 Bearing…