scholarly journals Bestimmung des Elektronendichteprofils in Plasmen mit Hilfe von Hohlraumresonatoren / Determination of Plasma Electron Density Profiles by Means of Resonant Cavities

1969 ◽  
Vol 24 (10) ◽  
pp. 1496-1501
Author(s):  
G. Janzen

Abstract The shift of the resonant frequency of microwave cavities excited in TM0m0 (m=1, 2, 3), TMl10 (l=1, 2), TE01n (n>0 integer) modes under the influence of a plasma is calculated for arbitrary radii of plasma and cavity for Bessel profile and common parabolic profiles.In measuring the frequency shift for two of the cited cavity mode types an approximate electron density profile can be determined from the submitted diagrams.

1972 ◽  
Vol 27 (3) ◽  
pp. 491-499 ◽  
Author(s):  
G Janzen

AbstractThe eigenvalue equation of a plasma-discharge tube configuration in a cylindrical microwave cavity is derived and solved numerically by an exact theory for TMlm0 , TM0mn, and TE0mn resonance modes. The radial and axial electron density profiles are assumed to be homogeneous. The factors of proportionality between electron density and shift of the resonance frequency derived from the linear perturbation theory are compared with the exactly computed eigenvalues. Hence the range of validity of the linearly computed factors of proportionality (geometry factors) can be established. By considering the influence of the discharge tube the geometry factors are altered and consequently the sensitivity of the measurement. The influence of the discharge tube can be taken into account by means of suitable correction factors.


Nature ◽  
1978 ◽  
Vol 276 (5687) ◽  
pp. 530-532 ◽  
Author(s):  
N. P. FRANKS ◽  
T. ARUNACHALAM ◽  
E. CASPI

2021 ◽  
Vol 11 ◽  
pp. 18
Author(s):  
Iurii Cherniak ◽  
Irina Zakharenkova ◽  
John Braun ◽  
Qian Wu ◽  
Nicholas Pedatella ◽  
...  

The Constellation Observing System for Meteorology, Ionosphere, and Climate 2 (COSMIC-2) mission was launched into a low-inclination (24°) orbit on June 25, 2019. Six satellites, each with an advanced Tri-GNSS Radio-Occultation Receiver System (TGRS), provide a global and uniform data coverage of the equatorial region with several thousand electron density profiles daily. The COSMIC-2 electron density profiles, and specifically the derived ionospheric F2 peak parameters, are properly validated in this study with reliable “truth” observations. For this purpose, we used manually scaled ionograms from 29 ground-based ionosondes located globally at low and middle latitudes. For this validation campaign, we considered only geomagnetically quiet conditions in order to establish benchmark level of the new mission’s ionospheric observation quality and to evaluate the operational capability of the COSMIC-2 Radio Occultation (RO) payload at the background of normal day-to-day variability of the ionosphere. For reliable colocations between two independent techniques, we selected only COSMIC-2 RO profiles whose F2 peak point coordinates were within 5° of the closest ionosonde. Our comparison of the ionospheric F2 peak height (hmF2) derived from COSMIC-2 RO and ground-based ionosonde measurements showed a very good agreement, with a mean of ~5 and ~2 km at low and middle latitudes, respectively, while RMS error was of ~23 and ~14 km, respectively. That range corresponds to a deviation of only 6–9% from the reference, ionosonde observations. Examination of representative collocation events with multiple (2–5) simultaneous RO tracks near the same ionosonde with different RO geometry, multi-satellite and multi-GNSS combination give us observational evidence that COSMIC-2 RO-based EDPs derived from GPS and GLONAS links show good self-consistency in terms of the ionospheric F2 peak values and electron density profile shape. We can conclude that COSMIC-2 provides high quality data for specification the ionospheric electron density at the F2 peak region.


1979 ◽  
Vol 12 (3) ◽  
pp. 417-423
Author(s):  
J L Sebastian ◽  
V Colomer ◽  
M Rodriguez-Vidal ◽  
J Peon

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