Effect of the Magnetic Field on the Characteristics of a Pulsed Penning Ion Source

2020 ◽  
Vol 46 (2) ◽  
pp. 217-229 ◽  
Author(s):  
N. V. Mamedov ◽  
S. P. Maslennikov ◽  
A. A. Solodovnikov ◽  
D. I. Yurkov
2016 ◽  
Vol 35 (1) ◽  
pp. 53-57 ◽  
Author(s):  
T. Kanesue ◽  
S. Ikeda

AbstractA laser ion source (LIS) is a promising candidate as an ion source for heavy-ion inertial fusion (HIF), where a pulsed ultra-intense and low-charged heavy ion beam is required. It is a key development for a LIS to transport laser-produced plasma with a magnetic field to achieve a high-current beam. The effect of a tapered magnetic field on laser-produced plasma is demonstrated by comparing the results with a straight solenoid magnet. The magnetic field of interest is a wider aperture on a target side and narrower aperture on an extraction side. Based on the experimentally obtained results, the performance of a scaled LIS for HIF was estimated.


2021 ◽  
Vol 130 (5) ◽  
pp. 053303
Author(s):  
D. Wünderlich ◽  
I. M. Montellano ◽  
M. Lindqvist ◽  
A. Mimo ◽  
S. Mochalskyy ◽  
...  

2003 ◽  
Vol 42 (Part 1, No. 6A) ◽  
pp. 3656-3657 ◽  
Author(s):  
Yoshihide Higurashi ◽  
Takahide Nakagawa ◽  
Masanori Kidera ◽  
Toshimitsu Aihara ◽  
Masayuki Kase ◽  
...  

1967 ◽  
Vol 31 ◽  
pp. 375-380
Author(s):  
H. C. van de Hulst

Various methods of observing the galactic magnetic field are reviewed, and their results summarized. There is fair agreement about the direction of the magnetic field in the solar neighbourhood:l= 50° to 80°; the strength of the field in the disk is of the order of 10-5gauss.


1994 ◽  
Vol 144 ◽  
pp. 29-33
Author(s):  
P. Ambrož

AbstractThe large-scale coronal structures observed during the sporadically visible solar eclipses were compared with the numerically extrapolated field-line structures of coronal magnetic field. A characteristic relationship between the observed structures of coronal plasma and the magnetic field line configurations was determined. The long-term evolution of large scale coronal structures inferred from photospheric magnetic observations in the course of 11- and 22-year solar cycles is described.Some known parameters, such as the source surface radius, or coronal rotation rate are discussed and actually interpreted. A relation between the large-scale photospheric magnetic field evolution and the coronal structure rearrangement is demonstrated.


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