Influence of heating of the ionosphere by high-power radio emission on the sporadic E layer

1975 ◽  
Vol 18 (9) ◽  
pp. 1010-1013 ◽  
Author(s):  
Yu. A. Ignat'ev
Author(s):  
Kamil Yusupov ◽  
Nataliya Bakhmetieva ◽  
Vladimir Frolov ◽  
Takashi Maruyama ◽  
Adel Akchurin ◽  
...  

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pp. 653-663 ◽  
Author(s):  
T. D. Borisova ◽  
N. F. Blagoveshchenskaya ◽  
V. A. Kornienko ◽  
A. S. Yanzhura ◽  
A. S. Kalishin ◽  
...  

2017 ◽  
Vol 122 (12) ◽  
pp. 12,517-12,533 ◽  
Author(s):  
J. Moro ◽  
L. C. A. Resende ◽  
C. M. Denardini ◽  
J. Xu ◽  
I. S. Batista ◽  
...  

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Vol 11 (9) ◽  
pp. 756-759
Author(s):  
Yu. A. Ignat'ev

2008 ◽  
Vol 26 (9) ◽  
pp. 2929-2936 ◽  
Author(s):  
K.-I. Oyama ◽  
K. Hibino ◽  
T. Abe ◽  
R. Pfaff ◽  
T. Yokoyama ◽  
...  

Abstract. The electron temperature (Te), electron density (Ne), and two components of the electric field were measured from the height of 90 km to 150 km by one of the sounding rockets launched during the SEEK-2 campaign. The rocket went through sporadic E layer (Es) at the height of 102 km–109 km during ascent and 99 km–108 km during decent, respectively. The energy density of thermal electrons calculated from Ne and Te shows the broad maximum in the height range of 100–110 km, and it decreases towards the lower and higher altitudes, which implies that a heat source exists in the height region of 100 km–110 km. A 3-D picture of Es, that was drawn by using Te, Ne, and the electric field data, corresponded to the computer simulation; the main structure of Es is projected to a higher altitude along the magnetic line of force, thus producing irregular structures of Te, Ne and electric field in higher altitude.


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