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Программа и тезисы докладов - Институт космических ...

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field recordings for detailed analysis. Applying our real full wave (UWB) propagation<br />

code, and utilizing the high sensibility of the satellite sensors, proper interpretation<br />

of amplitude modulated character of trans-ionospheric whistlers was possible<br />

as closely spaced oblique propagated impulses. This technique provides more accurate<br />

information about the generation (lightning flash) mechanism. Results of UWB<br />

modeling of lightning excited impulse propagation in the anisotropic ionosphere<br />

confirmed the conlusions of earlier studies, performed in higher altitude satellite recordings.<br />

Swallow tailed whistler (STW) occurrences has been demostrated in Chibis<br />

records. Unlike to already known, published character of STWs, these cases were<br />

coupled to 0 + whistler types. With the analysis of newly found STW occurrences<br />

their source region, exciting process may be better described.<br />

The iniTial reSulTS oF MagneTic-Wave coMplex<br />

daTa proceSSing (MicroSaTelliTe “chibiS-M”)<br />

S. M. Belyaev, D. F. Dudkin<br />

Lviv Centre of Institute for Space Research (LC ISR) of the National Academy<br />

of Sciences of Ukraine and National Space Agency of Ukraine, Lviv, Ukraine<br />

Scientific equipment complex “Groza” of “Chibis-M” includes magneticwave<br />

complex (MWC) consisting of 2 combined wave probes (CWP1, CWP2), an<br />

induction magnetometer and a spectral analysis processor (SAP). MWC is meant<br />

for measuring and examining space weather electromagnetic parameters within the<br />

band of 1 Hz — 20 kHz.<br />

MWC detectors are set on the micro-satellite in such a way that the induction<br />

magnetometer and magnetic field measurers, belonging to wave probes, form<br />

orthogonal coordinate system, and the plates of space plasma current measurers<br />

of both wave probes are mutually perpendicular. This configuration allows for measuring<br />

3 components of magnetic field induction, 2 components of space current<br />

density and electric field intensity.<br />

Analogue output voltages of detectors are transformed into a digital form<br />

and undergo primary treatment in the spectral analysis processor. Resulting data<br />

streams are transmitted to the ground contact points.<br />

During data processing intense disturbance coming from the onboard equipment<br />

of the micro-satellite were registered. This was caused by the proximity of<br />

detectors to other devices of the scientific equipment complex. After the onboard<br />

disturbance examination new methods and algorithms of digital data filtering were<br />

elaborated and tested. The onboard recordings demonstrated great effectiveness<br />

of these algorithms.<br />

The analysis of telemetry packets received from MWC in contingency (power<br />

shortage) has indicated the sufficient stability of equipment and modes adopted in<br />

such situations.<br />

In the process of filtered data analysis whistler waves illustrating ionosphere<br />

electromagnetic processes were detected. The most qualitative results were obtained<br />

on the examination of measurements of magnetic field induction and electric field<br />

intensity. Least informative were the channels of current measuring.<br />

27

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