J. Manninena, Yu. V. Fedorenkob, N. G. Kleimenovac, d, O. V. Kozyrevac, d, and A. S. Nikitenkob
a Sodankyla Geophysical Observatory, Finland
b Polar Geophysical Institute, Russian Academy of Sciences, Apatity, Murmansk region, Russia
c Schmidt Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia
d Institute of Space Research, Russian Academy of Sciences, Moscow, Russia
e-mail: jyrki.manninen@sgo.fi
Received July 2, 2013
AbstractFor the first time, simultaneous observations of very low frequency (VLF) emissions at auroral lat-
itudes (L = 5.3) are carried out at two points located at close geomagnetic latitudes and spaced in longitude by
400 km: the Finnish Kannuslehto station (
= 64.2
) and the Russian Lovozero observatory (
= 64.1
). A
recording equipment with similar frequency responses was used. The first results of a comparison of simulta-
neous observations showed that, in the overwhelming majority of cases, bursts of VLF emission appeared at
both points synchronously with an identical (more often right-handed) polarization of the magnetic field of VLF
waves, which can be evidence in favor of large dimensions of the ionosphere exit region of VLF waves. A simul-
taneous burst of quasi-periodic VLF emissions that occurred on February 02, 2013, during a substorm at 2324
UT is discussed in detail. Additionally, VLF bursts were recorded which were observed only at one point, e.g.,
the appearance of left-hand polarized periodic emissions (PEs) in band 2.54.0 kHz with a repetition period of
34 s.
10.1134/S0016793214010083
Pleiades Publishing home page | journal home page | top
If you have any problems with this server, contact webmaster.