Low‐Latitude Whistler‐Mode and Higher‐Latitude Z‐mode Emission at Jupiter Observed by Juno

2020 ◽  
Author(s):  
J. D. Menietti ◽  
T. F. Averkamp ◽  
M. Imai ◽  
W. S. Kurth ◽  
G. B. Clark ◽  
...  
Keyword(s):  
Low Latitude ◽  
Whistler Mode

scholarly journals Simulation of whistler mode propagation for low latitude stations

2004 ◽  
Vol 56 (10) ◽  
pp. 979-987 ◽  
Author(s):  
Kalpana Singh ◽  
R. P. Singh ◽  
Orsolya E. Ferencz
Keyword(s):  
Mode Propagation ◽  
Low Latitude ◽  
Whistler Mode

Doppler shifts of LF whistler-mode signal observed at a low-latitude (L = 1.54)

1989 ◽  
Vol 37 (7) ◽  
pp. 825-836 ◽  
Author(s):  
M. Nishino ◽  
Y. Tanaka ◽  
K.J.W. Lynn
Keyword(s):  
Low Latitude ◽  
Whistler Mode ◽  
Doppler Shifts

scholarly journals Very Low Latitude Whistler‐Mode Signals: Observations at Three Widely Spaced Latitudes

2019 ◽  
Vol 124 (11) ◽  
pp. 9253-9269
Author(s):  
Neil R. Thomson ◽  
Mark A. Clilverd ◽  
Craig J. Rodger
Keyword(s):  
Low Latitude ◽  
Whistler Mode

Progress report on 21-cm observations at low latitude between longitudes (l 11) 0° and 66°

1967 ◽  
Vol 31 ◽  
pp. 177-179
Author(s):  
W. W. Shane
Keyword(s):  
Preliminary Report ◽  
Progress Report ◽  
Galactic Centre ◽  
Low Latitude ◽  
The Third ◽  
Introductory Lecture ◽  
Centre Region

In the course of several 21-cm observing programmes being carried out by the Leiden Observatory with the 25-meter telescope at Dwingeloo, a fairly complete, though inhomogeneous, survey of the regionl11= 0° to 66° at low galactic latitudes is becoming available. The essential data on this survey are presented in Table 1. Oort (1967) has given a preliminary report on the first and third investigations. The third is discussed briefly by Kerr in his introductory lecture on the galactic centre region (Paper 42). Burton (1966) has published provisional results of the fifth investigation, and I have discussed the sixth in Paper 19. All of the observations listed in the table have been completed, but we plan to extend investigation 3 to a much finer grid of positions.

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