The Venus Express mission is scheduled for launch in 2005. Among many other instruments, it carries a magnetometer to investigate the Venus plasma environment. Although Venus has no intrinsic magnetic moment, magnetic field measurements are essential in studying the solar wind interaction with Venus. Our current understanding of the solar wind interaction with Venus is mainly from the long lasting Pioneer Venus Orbiter (PVO) observations. In this paper, we briefly describe the magnetic field experiment of the Venus Express mission. We compare Venus Express with PVO with respect of the solar wind interaction with Venus. Then we discuss what we will achieve with the upcoming Venus Express mission
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...
The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and...
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...
In situ measurements of the magnetic field are vital to the study of many fundamental problems in p...
Venus has negligible intrinsic magnetic fields to the first order, such that its ionosphere (the cha...
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed ...
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed ...
The MAG (Magnetometer) instrument aboard the Venus Express spacecraft is designed to investigate the...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
The solar wind interaction with the non-magnetic Venerean ionospheric obstacle is unique. Ionospheri...
Today, the earth's instrinsic magnetic field prevents the streaming solar wind plasma from directly ...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
Strong ultraviolet radiation from the Sun ionizes the upper atmosphere of Venus, creating a dense i...
We present a statistical study on the interaction between interplanetary coronal mass ejections (ICM...
We present a statistical study on the interaction between interplanetary coronal mass ejections (ICM...
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...
The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and...
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...
In situ measurements of the magnetic field are vital to the study of many fundamental problems in p...
Venus has negligible intrinsic magnetic fields to the first order, such that its ionosphere (the cha...
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed ...
Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed ...
The MAG (Magnetometer) instrument aboard the Venus Express spacecraft is designed to investigate the...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
The solar wind interaction with the non-magnetic Venerean ionospheric obstacle is unique. Ionospheri...
Today, the earth's instrinsic magnetic field prevents the streaming solar wind plasma from directly ...
International audienceIn order for the Parker Solar Probe (PSP) mission to study the solar corona, i...
Strong ultraviolet radiation from the Sun ionizes the upper atmosphere of Venus, creating a dense i...
We present a statistical study on the interaction between interplanetary coronal mass ejections (ICM...
We present a statistical study on the interaction between interplanetary coronal mass ejections (ICM...
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...
The current state of knowledge of the chemistry, dynamics and energetics of the upper atmosphere and...
Out of the two Venus flybys that BepiColombo uses as a gravity assist manoeuvre to finally arrive at...