Open AccessAnalysis of an Interplanetary Coronal Mass Ejection by a Spacecraft Radio Signal: A Case Study
Author(s) -
Molera Calvés G.,
Kallio E.,
Cimo G.,
Quick J.,
Duev D. A.,
Bocanegra Bahamón T.,
Nickola M.,
Kharinov M. A.,
Mikhailov A. G.
Publication year - 2017
Publication title -
space weather
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.254
H-Index - 56
ISSN - 1542-7390
DOI - 10.1002/2017sw001701
Subject(s) - interplanetary scintillation , coronal mass ejection , physics , heliosphere , solar wind , interplanetary spaceflight , spacecraft , scintillation , interplanetary medium , astronomy , solar physics , astrophysics , remote sensing , plasma , optics , geology , quantum mechanics , detector
Tracking radio communication signals from planetary spacecraft with ground‐based telescopes offers the possibility to study the electron density and the interplanetary scintillation of the solar wind. Observations of the telemetry link of planetary spacecraft have been conducted regularly with ground antennae from the European Very Long Baseline Interferometry Network, aiming to study the propagation of radio signals in the solar wind at different solar elongations and distances from the Sun. We have analyzed the Mars Express spacecraft radio signal phase fluctuations while, based on a 3‐D heliosphere plasma simulation, an interplanetary coronal mass ejection (ICME) crossed the radio path during one of our observations on 6 April 2015. Our measurements showed that the phase scintillation indices increased by a factor of 4 during the passage of the ICME. The method presented here confirms that the phase scintillation technique based on spacecraft signals provides information of the properties and propagation of the ICMEs in the heliosphere.