electron density peak
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Author(s):  
А.Ю. Тельнова ◽  
Г.С. Курскиев ◽  
Н.Н. Бахарев ◽  
В.К. Гусев ◽  
Е.О. Киселев ◽  
...  

AbstractThe results of experiments and simulations of the transport of heat and particles in the Globus-M spherical tokamak are presented. Investigations were carried out in the ohmic mode in hydrogen and deuterium plasma. It is shown that in the phase of current growth under the same initial conditions, as long as the condition is met at which the minimum of the safety factor exceeds unity, two scenarios of discharge development are possible: with an electron temperature dive or with an electron density peak. After the safety factor reaches the value of 1, the differences are no longer observed. Modeling of transport processes using the ASTRA code showed that the dive of the electron temperature and density is a consequence of the decrease in the transport of heat and particles in the plasma core (i.e., the presence of internal transport barriers).


2015 ◽  
Vol 5 ◽  
pp. A21 ◽  
Author(s):  
Marco Limberger ◽  
Manuel Hernández-Pajares ◽  
Angela Aragón-Ángel ◽  
David Altadill ◽  
Denise Dettmering

2004 ◽  
Vol 22 (6) ◽  
pp. 2015-2022 ◽  
Author(s):  
C. Stolle ◽  
N. Jakowski ◽  
K. Schlegel ◽  
M. Rietveld

Abstract. To obtain a comprehensive view on high latitude processes by applying different observation techniques, the SIRCUS campaign was initiated in 2001/2002. This paper compares electron density profiles derived from CHAMP radio occultation data and those measured with the EISCAT facility. Since ionospheric profiling with the help of space-based received GPS is a relatively new technique, validations with established independent instruments are of crucial need. We present 28 profiling events for quasi-statistical analyses, which occurred during the SIRCUS campaigns and describe some of them in more detail. We found out that the majority of profile comparisons in electron density peak value and height, as well as in TEC, lie within the error ranges of the two methods. Differences in the ionospheric quantities do not necessarily occur when the locations of the occultation and of the radar site show considerable distances. Differences are more pronounced when the ionosphere is remarkably structured.


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