The high-frequency electric sensors onboard Solar Orbiter are part of the radio and plasma wave experiment (RPW). The sensors consist of cylindrical antennas (ANT) mounted on three booms extruded from the central body of the spacecraft. Due to the parasitic effects of the conducting spacecraft body and solar panels the true antenna properties (effective axes and length, capacitances) do not coincide with their physical representations. The numerical analysis of the reception properties of these antennas is presented. In order to analyze the antenna system we applied a numerical method. The current distribution on the spacecraft body and the effective length vector was calculated, by solving the underlying field equations using electromagnet...
Solar Orbiter is an M-class mission in the ESA Science Programme Cosmic Vision 2015 – 2025 having an...
International audienceWe will review the instrumental capabilities of the Radio and Plasma Waves (RP...
International audienceWe present numerical simulations of the Solar Orbiter spacecraft (SC)/plasma i...
Currents on the conducting surfaces of the spacecraft hull, induced by electric fields of radio wave...
De resultaten worden beschreven voor de antennes op schaal voor de Solar Orbiter satelliet voor een ...
This master thesis report describes the expected noise that the electric antennas of theSolar Orbite...
International audienceThe main characteristics of the long-boom electric antennas installed on board...
For investigation of receiving antenna behaviors in space plasma, inhomogeneous plasma environment r...
Context. In order to allow for a comparison with the measurements from other antenna systems, the vo...
International audienceThe reception properties of the Radio Wave Instrument (RWI) onboard JUICE (Jup...
A document discusses concepts for the design of an antenna to be deployed from a spacecraft for meas...
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is described in this pa...
Electric field antennas are capable of detecting dust impacts in different space environment. We ana...
Solar Orbiter is an M-class mission in the ESA Science Programme Cosmic Vision 2015 – 2025 having an...
International audienceWe will review the instrumental capabilities of the Radio and Plasma Waves (RP...
International audienceWe present numerical simulations of the Solar Orbiter spacecraft (SC)/plasma i...
Currents on the conducting surfaces of the spacecraft hull, induced by electric fields of radio wave...
De resultaten worden beschreven voor de antennes op schaal voor de Solar Orbiter satelliet voor een ...
This master thesis report describes the expected noise that the electric antennas of theSolar Orbite...
International audienceThe main characteristics of the long-boom electric antennas installed on board...
For investigation of receiving antenna behaviors in space plasma, inhomogeneous plasma environment r...
Context. In order to allow for a comparison with the measurements from other antenna systems, the vo...
International audienceThe reception properties of the Radio Wave Instrument (RWI) onboard JUICE (Jup...
A document discusses concepts for the design of an antenna to be deployed from a spacecraft for meas...
The Radio and Plasma Waves (RPW) instrument on the ESA Solar Orbiter mission is described in this pa...
Electric field antennas are capable of detecting dust impacts in different space environment. We ana...
Solar Orbiter is an M-class mission in the ESA Science Programme Cosmic Vision 2015 – 2025 having an...
International audienceWe will review the instrumental capabilities of the Radio and Plasma Waves (RP...
International audienceWe present numerical simulations of the Solar Orbiter spacecraft (SC)/plasma i...