The 22-Pole Superconducting 7-Tesla Wiggler for the DELTA Storage Ring


Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

A superconducting wiggler with a magnetic field of 7 T is installed as an insertion device for three X-ray beamlines with photon energies of more than 30 keV used at the Dortmund Electron Accelerator (DELTA, Germany), a source of 1.5 GeV synchrotron radiation. Each of the two side beamlines is separated from the central one by 15 mrad and all three beamlines use a horizontal aperture of 5 mrad. To meet these requirements, the insertion device must have a period of 127 mm and a magnetic field of 7 T for the vertical aperture of a beam vacuum chamber 10 mm long and a flange-to-flange distance of 2.2 m. A superconducting 22-pole wiggler with a field of 7 T and a period of 127 mm operating in the zero boil-off mode is described. The concept and main approaches to designing the magnetic and the cryogenic systems are presented, along with the main parameters and results from testing the new 7-tesla superconducting wiggler for the DELTA storage ring.

About the authors

Ye. A. Gusev

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

S. Khan

Dortmund Technical University

Email: shkaruba@mail.ru
Germany, Dortmund, 244227

S. V. Khrushchev

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

V. Kh. Lev

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

N. A. Mezentsev

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

A. N. Safronov

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

V. A. Shkaruba

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Author for correspondence.
Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

O. A. Tarasenko

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

V. M. Tsukanov

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

S. S. Vasichev

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

A. A. Volkov

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

A. V. Zorin

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

A. V. Bragin

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

A. I. Erokhin

Budker Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences

Email: shkaruba@mail.ru
Russian Federation, Novosibirsk, 630090

Supplementary files

Supplementary Files
Action
1. JATS XML

Copyright (c) 2019 Allerton Press, Inc.