The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
In this view several white squares of different sizes can be seen on the side of the spacecraft;this side has five of the six MWR antennas. The triangular boom on the right is the Magnetometer (MAG) instrument
In this view several white squares of different sizes can be seen on the side of the spacecraft;this side has five of the six MWR antennas. The triang
The white square is the biggest MWR antenna, and takes up another side of the spacecraft. This antenna is for 600 MHz.
The white square is the biggest MWR antenna, and takes up another side of the spacecraft. This antenna is for 600 MHz.
This visualization released by NASA depicts the layers that MWR will observe below the top visible cloud layer
This visualization released by NASA depicts the layers that MWR will observe below the top visible cloud layer
Layers of the Jovian atmosphere and corresponding MWR channels
Layers of the Jovian atmosphere and corresponding MWR channels
Components of Waves
Components of Waves
Waves being installed on Juno spacecraft
Waves being installed on Juno spacecraft
The path of the Ulysses spacecraft through the magnetosphere of Jupiter in 1992, shows the location of the Jovian bow shock.
The path of the Ulysses spacecraft through the magnetosphere of Jupiter in 1992, shows the location of the Jovian bow shock.
This illustration shows how the Jovian magnetosphere is thought to interact with the incoming solar wind (yellow arrows)
This illustration shows how the Jovian magnetosphere is thought to interact with the incoming solar wind (yellow arrows)