This paper summarizes the the activities carried out by Working Group 4 of COST 271 Action. The structure of this Working Group included four Working packages that were dealing with different aspects of the same overall problem related to space plasma variability and irregularities effects
on advanced satellite systems. General comments about the most relevant achievements and possible future lines of research are given

Radicella, S. M.

Tulunay, E.

Earth-prints Repository

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ANNALS  OF  GEOPHYSICS, SUPPLEMENT TO VOL.  47, N.  2/3, 2004
4
Space plasma effects on Earth-space 
and satellite-to-satellite communications:
Working Group 4 overview 
SANDRO M. RADICELLA (1) and ERSIN TULUNAY (2) (3) 
(1) The Abdus Salam International Centre for Theoretical Physics (ICTP),
Aeronomy and Radiopropagation Laboratory, Trieste, Italy
(2) Department of Electrical and Electronics Engineering, Middle East Technical University,
Balgat, Ankara, Turkey
(3) TUBITAK Marmara Research Center, Information Technologies Research Institute, Gebze, Kocaeli, Turkey 
This paper summarizes the the activities carried out by Working Group 4 of COST 271 Action.
The structure of this Working Group included four Working packages that were dealing with differ-
ent aspects of the same overall problem related to space plasma variability and irregularities effects
on advanced satellite systems. General comments about the most relevant achievements and possible
future lines of research are given.
4.1. INTRODUCTION
At present to assess the effect of space plasma variability and irregularities on satellite systems is
becoming an important part of planning of advanced applications of such systems. This aim was cho-
sen as the key objective of Working Group 4 of the COST 271 Action. The structure of this Working
Group included four Working Packages dealing with different aspects of the same overall problem
covering ionospheric scintillations observations and modelling, development of algorithms for the
forecasting and nowcasting of Total Electron Content (TEC), study of ionospheric disturbances gen-
erated by natural and anthropogenic processes, and the effects of electron density and TEC gradients
on Earth-space and satellite-to-satellite communications. The details of these investigations and the
results achieved can be found in the respective papers that correspond to each of the Working Pack-
ages of WG 4. General comments about the major achievements and possible future lines of research
dealing with the same topics are given below.
4.2. EFFECTS OF SPACE PLASMA VARIABILITY AND IRREGULARITIES ON EARTH-SPACE
AND SATELLITE-TO-SATELLITE COMMUNICATION CHANNELS
The propagation of satellite signals through ionospheric irregularities generates modifications
of the signals like intensity and phase fluctuations and rapid variations of angle of arrival. These
phenomena are known as ionospheric scintillations and are observed particularly at low and high
latitudes. 
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Sandro M. Radicella and Ersin Tulunay
The GISM model has been further developed (Beniguel, 2002). It uses the Multiple Phase
Screen technique and gives statistical characteristics of transmitted signals, fade duration and oth-
er parameters like signal loss of lock probability. Maps of scintillation index S4 and phase standard
deviations can be produced. 
A new hybrid propagation model to describe ionospheric scintillations has been developed
that includes generating a 2D random screen by means of the complex phase method (Gherm et
al., 2002). This can result in a full shaped model able to extract not only scintillation indices, but
also additional spectral information and model time series particularly suited for system-oriented
problems. 
Both GISM and the new model use as background ionosphere the 3D and time dependent
NeQuick model of electron density that is one of the ionospheric models developed in the framework
of the previous COST 251 Action (Radicella and Leitinger, 2001). 
At present, it is widely accepted that at high latitudes phase scintillation activity is high and dom-
inant while intensity scintillation is low and negligible. This scenario is based on several scintillation
experiments done by means of GPS scintillation monitors. 
Forte and Radicella (2002) have shown that data detrending, when the separation of determinis-
tic and stochastic components is done using a fixed cut-off frequency, can lead to a misleading data
interpretation. An experiment for measuring these effects on ionospheric scintillation information
pointed out from GPS signals has been set up at auroral latitudes being run at the Sodankyla Geo-
physical Observatory (University of Oulu). A GPS receiver with a sufficiently high sampling rate has
been used to measure the carrier phase and signal-to-noise ratios at L1. The preliminary result of the
experiment seems to confirm the theoretical mechanism suggested as an explanation for the occur-
rence at high latitudes of high phase scintillation against low intensity scintillation. With these results
new ways of describing scintillation effects at system level can be determined. 
An effort was also made by Forte et al. (2002) to interpret experimental scintillations intensity da-
ta in a way useful to determine the impact of these phenomena on satellite navigation systems. At-
tention has also been given to the comparison between experimental data and models predictions. It
can be stressed that the models fail to describe the patchy structure of irregularities, a typical feature
of ionospheric irregularities.
4.3. DEVELOPMENT OF ALGORITHMS AND SOFTWARE TO TREAT DISTURBANCES
IN EARTH-SPACE AND SATELLITE-TO-SATELLITE COMMUNICATIONS
Unpredictable variability of the ionospheric parameters due to disturbances related to the iono-
sphere-magnetosphere system limits the efficiency of communications affected by the ionosphere by
causing serious technological problems including range errors, scintillations of satellite signals and
others propagation problems. It is known that in such cases mathematical modeling of the variabili-
ty based on first physical principles is extremely difficult. Therefore data driven models such as Neur-
al Networks based models can be used to forecast ionospheric parameters like TEC. The only re-
quirement for the success of data driven models is the availability of reliable data, which can repre-
sent the characteristics of the process to be modeled. 
The Middle East Technical University Neural Networks (METU-NN) technique to forecast 10
min values of the vertical Total Electron Content (TEC) values up to 24 h ahead during high solar
activity in the current solar cycle has been applied to TEC data evaluated from GPS measurements
from 2000 to 2001 at Chilbolton (51.8 N, 1.26 W). An additional validation has been performed us-
ing an independent data set. The construction work of the Neural Network based model is carried
out in the development mode. It is composed of «training phase or learning phase» and «test phase»
(Tulunay et al., 2004a,b). The good results of this investigation indicate the potential of the Neural
Networks techniques to forecast local vertical TEC values. The possible extension of the same tech-
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Space plasma effects on Earth-space and satellite-to-satellite communications: Working Group 4 overview
nique to forecast two dimensional TEC maps could provide a very useful tool to forecast the effects
of the ionosphere on satellite navigation. 
Since 1995, DLR/IKN has been operating a new system for regularly processing data and pro-
ducing TEC maps over the European region based on GPS measurements by the International GPS
Service (IGS). The existing large database, containing data from all solar/geomagnetic conditions, is
a very useful tool for the validation of all types of ionospheric effects calculations particularly for
highly disturbed ionospheric conditions where the use of other measurement techniques (e.g.,
ionosondes) is limited. Furthermore, DLR/IKN has developed the software modules for deriving
ionospheric grid errors in the EGNOS System Testbed (ESTB) in real-time. 
Auto- and cross-correlation procedures have recently been developed for predicting both the crit-
ical frequency of the F2-region and the TEC, strongly relating the short-term forecast to present and
future geomagnetic activity. Preliminary results of these methods/procedures have already been test-
ed and reported for the one-dimensional case when forecasting is performed at a given location based
on GPS-TEC measurements, solar and geomagnetic activity indices. Extending such a prediction to
several locations in a given region, instantaneous maps of the forecast can be constructed covering
the region of interest. 
Other investigations on TEC and critical frequency of F2 variability have been carried out to-
gether with the application of clustering techniques to characterize F2 critical frequency behavior.
4.4. APPLICATION OF THEORETICAL CONSIDERATIONS TO THE STUDY OF SPACE
PLASMA EFFECTS
A series of investigations have been carried out to study different aspects of the plasma charac-
teristics in the magnetosphere-ionosphere-thermosphere system. Electromagnetic emissions at an
ample range of frequencies measured on-board of low orbiting satellites have shown that during
strong geomagnetic storms a series of phenomena are observed in same regions of the satellite orbital
environment (B ⁄lecki et al., 2003). A study was done on the impact of magnetospheric disturbances
on the daily critical frequency of F2 and considerations on the use of both topside and ground verti-
cal soundings to this purpose have been made (Rothkaehl et al., 2003). Also HF electromagnetic
noise in the ionosphere has been investigated using data from the Coronas-I satellite. The results
show that the electromagnetic noise introduced by broadcast stations can disturb the ionospheric en-
vironment particularly at night (Rothkaehl and Klos, 2002). 
The possible connection between earthquakes and disturbances in electromagnetic emissions has
been studied. 
Also the interaction between the body of the satellite and the surrounding ionospheric plasma has
been investigated. It has been shown that the enhancement of radiation between the local plasma fre-
quency an the F2 critical frequency can be correlated to interaction between the oscillation of elec-
trostatically trapped particles in the wake of a spacecraft and superthermal electrons.
4.5. EFFECTS OF THE VERTICAL AND HORIZONTAL GRADIENTS OF ELECTRON
DENSITY ON EARTH-SPACE AND SATELLITE-TO-SATELLITE COMMUNICATION
The ionosphere introduces a group delay in satellite signal and is at present the main source
of error for satellite navigation systems that operate at single frequency. The possible dependence
of these errors on different parameters has been described in the research done by Nava (2000)
with a systematic approach. NeQuick model has been used to assess this dependence and tests
with experimental data have been performed. The results obtained suggest a way to «build-up» a
correcting error function that applied to vertical TEC could «bind» the error on slant TEC after
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Sandro M. Radicella and Ersin Tulunay
«back conversion». Appropriate model simulations could indicate the influence of thin shell cur-
vature, latitudinal and longitudinal gradients on conversion error as a function of location and
satellite elevation and azimuth. 
Some ionospheric features observed during geomagnetic disturbed periods, were investigated us-
ing particular sets of GPS derived slant total electron content measurements: «Supertruth» data.
These data are high quality slant total electron content measurements obtained at 5 s sampling rate,
using 25 ground stations located in the U.S.A., during specific time periods. The coinciding pierce
point technique used has shown that a strong correlation between Dst index variation and mapping
function errors magnitude exists. Since mapping function errors reflect the presence of strong elec-
tron density and TEC gradients, the coinciding pierce point technique indicated that in some cases it
is possible to detect some ionospheric storm effects in near-real-time (Nava and Radicella, 2003). 
Information about the topside electron concentration distribution is not obtainable from ground-
based measurements. In past decades only few satellites were equipped with ionosondes to sound the
ionosphere above the F2 maximum (topside sounders). Ionospheric electron density models have
their topside formulation based on old databases or different kinds of measurements. NeQuick and
IRI models have been used for comparisons with topside sounder profiles (Coïsson, 2002). From the
study it appears that the NeQuick model performance is strongly affected by its topside thickness pa-
rameter, indicating the need for an improvement of its formulation. The study also shows that the top-
side formulation of IRI leads to an overestimation of the electron density in the upper part of the pro-
files, and consequently an overestimation of TEC. 
With the increasing use of radio systems for practical applications, particularly satellite-based nav-
igation and positioning, interest is now turning to propagation effects on satellite-to-satellite paths.
One specific aspect driving such investigations is concern over future requirements for the station-
keeping of satellites in the commercially very important, but potentially congested, geostationary or-
bit. Geostationary satellites are currently tracked using a network of ground stations. A future possible
development could involve positioning making the use of a satellite navigation system, like GPS. How-
ever, since the GPS system was designed primarily for terrestrial users the satellites have nadir-direct-
ed antennas. In consequence, reception in geostationary orbit would involve the use of signals trans-
mitted by GPS satellites on the far side of the Earth. The model simulation study for GPS-to-geosta-
tionary satellite ray paths has shown that very large TEC values may be encountered (Bailey and Ker-
sley, 2003, in Radicella et al., 2004). It must be noted that for some extreme situations where the tra-
jectory traverses the equatorial ionosphere at grazing incidence the TEC estimates could give rise to
positioning errors in excess of 0.5 km. It is clear from the study that in any use of GPS signals for the
station-keeping of geostationary satellites it would be necessary to exclude any dependence on signals
where the ray-path geometry is close to eclipse, particularly close to the equatorial plane.
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Space plasma effects on Earth-space and satellite-to-satellite communications: Working Group 4 overview
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Space plasma effects on Earth-spaceand satellite-to-satellite communications:Working Group 4 overview

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Space plasma effects on Earth-spaceand satellite-to-satellite communications:Working Group 4 overview

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