Ion cyclotron waves at Mars: Occurrence and wave properties

• Published in: Journal of geophysical research. Space physics 2014-07, Vol.119 (7), p.5244-5258
• Main Authors: Wei, H. Y., Cowee, M. M., Russell, C. T., Leinweber, H. K.
• Format: Article
• Language: English
• Subjects: Astrophysics; Electric fields; exosphere; ion cyclotron wave; Ions; Magnetic fields; Mars; pickup; Wave power
• ISSN: 2169-9380; 2169-9402
• DOI: 10.1002/2014JA020067

Ion cyclotron waves (ICWs) are generated during the interaction between the solar wind and the Martian exosphere in a process called ion pickup. Mars Global Surveyor (MGS) detected waves near the proton gyrofrequency, indicating pickup of the exospheric hydrogen. To analyze these waves, we first improve the zero levels of the MGS magnetic field data taken during the first aerobreaking phase and then perform a statistical study of the ICWs observed from just outside the Martian bow shock to over 14 Mars radii away. These ICW events typically last for 5 to 30 min but can occasionally last for hours. The wave power decreases slowly with distance on both the upstream and downstream sides. From the variation of wave properties with the strength of the background field, we find that there are likely still remaining offsets in at least some the data sets even after applying our calibration technique. Thus, we use the events with a strong background field to examine the wave properties that depend on an accurate determination of the field direction and strength. We find the pickup angle associated with the largest occurrence rate of ICWs to be around 45°, but neither the wave amplitude, nor wave frequency, nor wave duration appear to vary with pickup angle. Finally, we find the waves with background field strength greater than 4 nT occur on both the positive and negative electric field sides of Mars but have a larger occurrence rate on the side of Mars in the positive electric field direction (which is defined as the direction of the cross product of the magnetic field vector and solar wind flow vector). Key Points ICWs are found extensively at Mars in the MGS data with improved zero levels The pickup angle for the largest wave occurrence rate is around 45° Waves with large ambient B field occur asymmetrically in SW E field direction