scholarly journals Measurements of electron density structure in striated barium clouds

1978 ◽  
Vol 5 (8) ◽  
pp. 723-726 ◽  
Author(s):  
K. D. Baker ◽  
J. C. Ulwick
1972 ◽  
Vol 2 (2) ◽  
pp. 98-100 ◽  
Author(s):  
A. C. Riddle

Scattering of radiation from solar radio sources by in homogeneities in the electron density structure of the corona can have marked effects on the observed time profile and the brightness distribution. These effects are appreciable for any localized source emitting a brief burst of radiation and are most pronounced when the radiation propagates close to the plasma level; it is such sources, illustrated here by those of type III bursts, that will be considered in this paper.


2020 ◽  
Vol 897 (2) ◽  
pp. 124 ◽  
Author(s):  
Stella Koch Ocker ◽  
James M. Cordes ◽  
Shami Chatterjee

2009 ◽  
Vol 114 (A2) ◽  
pp. n/a-n/a ◽  
Author(s):  
C. H. Lin ◽  
J. Y. Liu ◽  
C. Z. Cheng ◽  
C. H. Chen ◽  
C. H. Liu ◽  
...  

2015 ◽  
Vol 8 (8) ◽  
pp. 3069-3074 ◽  
Author(s):  
J. Y. Liu ◽  
C. Y. Lin ◽  
H. F. Tsai

Abstract. The FORMOSAT-7/COSMIC-2 (F7/C2) will ultimately place 12 satellites in orbit with two launches with 24–28.5° inclination and 520–550 km altitude in 2016 and with 72° inclination and 720–750 km altitude in 2018. It would be very useful for the community to construct the global three-dimensional electron density structure by simultaneously combining the two launch observations for studying ionospheric structure and dynamics. However, to properly construct the global electron density structure, it is essential to know and evaluate differences between the ionospheric electron densities probed by the two launches. To mimic the F7/C2 observations, we examine the electron density probed at the two satellite altitudes 500 and 800 km by means of FORMOSAT-3/COSMIC (F3/C) observations at the parking orbit 500 km altitude and mission orbit 800 km altitude, as well as a corresponding observing system simulation experiment (OSSE). Observation and OSSE results show that the sounding geometries by satellite orbiting at 500 and 800 km altitudes can cause the overall differences in the electron density, the F2 peak electron density, and the F2 peak height of about 18–24, 12–28 %, and 7–19 km, respectively. Results confirm that the discrepancies mainly result from the sounding geometry and the grid (contour) bias of the electron density.


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