MGS proxies data at AMDA

• MGS proxies data are taken from the SSL/Space Physics Research Group site.
• IMF Draping Direction: draping direction of the IMF, detected at 400 km altitudes on the Martian dayside by MGS MAG/ER. More information
• Subsolar Magnetic Field Strength at 400 km altitudes at Mars: subsolar magnetic field magnitude at 400 km altitudes above Mars, inferred from measurements on the Martian dayside by MGS MAG/ER. More information
• Mars EUV proxy proxy for the EUV flux at Mars, determined by extrapolating measurements of the F10.7 flux from Earth to Mars. More information