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PROBLEMS OF GEOCOSMOS

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Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008)<br />

ANALYSIS <strong>OF</strong> CLUSTER AND IRIS RIOMETER DATA OBTAINED<br />

DURING EXPERIMENTS ON IONOSPHERIC MODIFICATION CARRIED<br />

OUT 16 FEBRUARY 2003<br />

A.L. Maulini 1 , A.L.Kotikov 1 , A.Gavrasov 2 , V.I. Odintsov 3<br />

1 Institute of Physics, St.Petersburg University, St.Petersburg, 198504, Russia, e-mail:<br />

maulini@geo.phys.spbu.ru; 2 Kostroma State University, Kostroma,Russia; 3 Institute of Terrestrial<br />

Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN), Moscow, Russia<br />

Abstract. This article is dedicated to one of the actively developing line of investigation in space<br />

plasma physics such as artificial modification of the ionosphere. Experiments carried out using<br />

Tromso heating facility with pump wave frequency of transmitter 4.04 MHz with square<br />

modulation period 10 minutes in 16 February 2003 is considered. This event was selected because<br />

of orbits projections of CLUSTER satellites along magnetic field lines went nearby disturbed<br />

region in ionosphere according to Tsyganeko model (T96). Electric, magnetic field and electron<br />

density data from CLUSTER satellites and IRIS imaging riometer data using wavelet, short time<br />

Fourier transform and spectral time analysis developed in IZMIRAN are analyzed. It is shown that<br />

effect is clearly observed in IRIS imaging riometer data (16 February 2003) right in the beam<br />

where the heating spot is. Also effect of heating is observed in CLUSTER data when satellites<br />

cross magnetic field lines conjugated with disturbed region. Thus it is experimentally shown that<br />

functioning of heating facility affects not only ionosphere but also the coupled ionosphericmagnetospheric<br />

interaction system.<br />

Introduction<br />

Aim of the experiment maid on 16 February 2003 by EISCAT heating facility in Tromso was the study of<br />

magnetospheric disturbances originated from modified ionosphere. The pump wave of 4.04 MHz had been<br />

used for ionospheric conductivity modification from 19:55:00 to 23:59:59 UT. The heating wave in<br />

eXtraordinary polarization (X-mode) and square modulation regime with 5 minutes ON and 5 minutes <strong>OF</strong>F<br />

cycle was employed.<br />

Generation of the disturbances made by enhancement of ionospheric conductivity in presence of the<br />

background electric field was considered theoretically by Maltsev et al. (1974), Stubbe and Kopka, (1977),<br />

Oguti and Hayashi (1984). Maltsev et al. (1974) have found analytical solution for some kinds of<br />

conductivity inhomogeneities, for more general cases numerical modeling should be used. The process can<br />

be described shortly as follows: in the region with enhanced conductivity electrical field can be considered as<br />

homogenous, at the border of the region appear field aligned currents, out of the disturbed region electric<br />

field diminishes as two-dimensional dipole. Disturbances of the electric field and related field-aligned<br />

currents propagate into magnetosphere with Alfven speed. This propagation is supposed to provide<br />

disturbances in coupled magnetospheric-ionospheric system much stronger than initial ones. And this work<br />

tries to check this supposition using different kind of experimental data.<br />

Satellite observations and analysis<br />

We used data from Cluster – satellites of European Space Agency. This is a group of four satellites<br />

forming a tetrahedron what make possible to measure different parameters of cosmic plasma not only from<br />

one point in space but from a volume. Orbits of satellites were calculated down to the ionosphere ( about 100<br />

km above the Earth surface) along magnetic field lines using Tsyganenko model (T96) with follows<br />

parameters: DST = -27, By = 2.9 nT, Bz = 2.3 nT, pressure<br />

of solar wind Psw = 2.5 nPa. According to calculation the<br />

disturbed spot at high of ionosphere has about 25 km in<br />

diameter.<br />

.<br />

along magnetic field lines.<br />

Fig.1 Results of calculation of disturbed magnetic tube<br />

and projection of clusters’ orbits down to the Earth surface<br />

168

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