A Proxy for the Upstream IMF Clock Angle Using MAVEN Magnetic Field Data. Issue 11 (28th November 2018)

• Record Type: Journal Article
• Authors: Hurley, Dana M.; Dong, Yaxue; Fang, Xiaohua; Brain, David A.
• Is Part Of: Journal of geophysical research. Volume 123:Issue 11(2018)
• Page Start: 9612
• Page End: 9618
• Publication Date: 2018-11-28
• Subjects: interplanetary magnetic field -- MAVEN magnetometer; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2018JA025578
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: Without an upstream monitor at Mars to provide a contemporaneous measurement of solar wind conditions, it is useful to have techniques of inferring the upstream solar wind conditions using downstream data. We develop a method to estimate the upstream interplanetary magnetic field (IMF) clock angle, defined as the orientation of the IMF vector in the plane perpendicular to the solar wind velocity, at Mars using magnetometer data from the Mars Atmosphere and Volatile Evolution (MAVEN) mission. The technique fits MAVEN magnetometer data from within the Martian magnetosheath to a model of the draped magnetic field direction in a coordinate system aligned with the motional electric field. The results provide a proxy for the clock angle that agrees with upstream measurements and reproduces the observed distribution of clock angles. Even if upstream observations are available for a given orbit, the proxy provides an estimate of the clock angle at the time when the spacecraft is in the magnetosheath, which may correct for inherent temporal variability, because the solar wind varies on timescales shorter than the 4.5‐hr MAVEN orbit. The clock angle proxy can be applied for any orientation of the MAVEN orbit, even when MAVEN does not traverse into the upstream solar wind. Key Points: A proxy for the upstream IMF clock angle is derived from Martian magnetosheath magnetic fields The distribution of inferred clock angles reproduces the measured distribution The uncertainty of the proxy reflects IMF fluctuations with time