The Cassini Magnetic Field Investigation

By M. K. Dougherty, S. Kellock, D. Southwood, A. Balogh, Edward J. Smith, B. Tsurutani, B. Gerlach, Karl-Heinz Glassmeier, F. Gleim, Christopher T. Russell and 3 more. 2004

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The THEMIS Fluxgate Magnetometer (2008, methodology): “Experience from magnetometer experiments on more recent missions such as Freja (Zanetti et al. 1994), Equator-S (Fornacon et al. 1999), Cluster (Balogh et al. 2001), Cassini (Dougherty et al. 2004), Double Star (Carr et al. 2005), VenusExpress (Zhang et al. 2006), or Rosetta (Auster et al. 2007; Gla”
Saturnian magnetospheric dynamics: Elucidation of a camshaft model (2007, methodology): “[4] The magnetometer data [Dougherty et al., 2004] acquired during the first 2 1/2 years of Cassini’s tour of Saturn are almost always modulated at a frequency comparable with the expected rotation rate of the planet over a large range of local times in the magnetosphere.”
The Solar Orbiter magnetometer (2020, methodology): “The MAG sensor core design used on Solar Orbiter is essentially identical to those on Double Star (Carr et al. 2005) and Cassini (Dougherty et al. 2004), with two soft magnetic cores procured from Ultra Electronics mounted in a rigid Macor ceramic block to maintain their relative orthogonal orientat”