Solar type III radio bursts are an important diagnostic tool in the understanding of solar
accelerated electron beams. They are a signature of propagating beams of nonthermal …

For decades, observations of Faraday rotation have provided unique insights into the
plasma density and magnetic field structure of the solar wind. Faraday rotation (FR) is the …

We have produced a computer assisted tomography program that optimizes a three‐
dimensional model to fit observational data. We have used this program with interplanetary …

Abstract Knowledge of the radial evolution of the coronal mass ejection (CME) is important
for the understanding of its arrival at the near-Earth space and of its interaction with the …

We have examined the relationship between solar wind speed and electron density
fluctuations on scale sizes around 100 km in the heliocentric distance range of 0.3 to 0.8 AU …

The Sun frequently accelerates near-relativistic electron beams that travel out through the
solar corona and interplanetary space. Interacting with their plasma environment, these …

Explore the development and state-of-the-art in deep space exploration using radio science
techniques In Radio Science Techniques for Deep Space Exploration, accomplished …

Radial variations of the amplitude and the energy flux of compressive waves in the solar
corona were explored for the first time using a spacecraft radio occultation technique. By …

We present an estimation of the electron density modulation index (δ N e N e δN_eN_e) for
the first time using solar type IIIb radio burst observations. The mean value of δ N e N e …

We have developed a Monte Carlo simulation code to study the effects of refraction due to
spatial variation of the solar wind density and scattering due to random density fluctuations …