Mapping of steady-state electric fields and convective drifts in geomagnetic fields – Part 2: The IGRF Annales Geophysicae DOI 10.5194/angeo-34-67-2016 19 January 2016 The method of electric field mapping along geomagnetic field lines, derived in an accompanying paper, is applied to the International Geomagnetic Reference Field. Formulae for the geomagnetic field gradient tensor are derived and these are used in a software package developed to map the electric field. A number of examples are presented illustrating the method. The method will be of importance in conjugate studies of ionospheric convection when the external magnetic field can be neglected. IGRF">Read more
Mapping of steady-state electric fields and convective drifts in geomagnetic fields – Part 1: Elementary models Annales Geophysicae DOI 10.5194/angeo-34-55-2016 19 January 2016 This paper introduces a new method for mapping electric fields in the magnetosphere along geomagnetic field lines. This is important for conjugate studies of electric fields measured in the ionosphere by SuperDARN radars, and at spacecraft carrying electric field probes. First elementary methods in a dipole field are reviewed and then the theory of of a new method described for general magnetic field models. The method is tested in a dipole model with a Harris magnetotail field. Read more
Magnetospheric conditions near the equatorial footpoints of proton isotropy boundaries Annales Geophysicae DOI 10.5194/angeo-33-1485-2015 9 December 2015 Adaptive magnetospheric models based on THEMIS magnetic observations made at 6-9Re in the nightside magnetosphere are used to map the magnetically conjugate 30 and 80keV proton isotropy boundaries (IBs) to investigate the value of Kib=Rc/rc (magnetic curvature radius to particle gyroradius) in the neutral sheet at the IB generation place. For the most accurate mapping, the group Kib spread spans from 4 to 32; its median value is ~13, slightly larger than Kib8 expected for current sheet scatter. Read more
Recent highlights from Cluster, the first 3-D magnetospheric mission Annales Geophysicae DOI 10.5194/angeo-33-1221-2015 2 October 2015 This paper presents recent highlights from the Cluster mission on solar wind turbulence, magnetopause asymmetries and magnetosheath density enhancements, dipolarisation currents, reconnection variability, FTE in greatest detail, plasmaspheric wind and re-filling of the plasmasphere, radiation belts, updates of magnetospheric electric and magnetic field models, and magnetosheath and magnetopause properties under low Mach number. Public access to all high-resolution data (CSA) is also presented. Read more
Observation of a new type of low-frequency waves at comet 67P/Churyumov-Gerasimenko Annales Geophysicae DOI 10.5194/angeo-33-1031-2015 19 August 2015 We present a first report on magnetic field measurements made in the coma of comet 67P/C-G in its low activity state. The plasma environment is dominated by quasi-coherent, large-amplitude, compressional magnetic field oscillations around 40 mHz, differing from the observations at strongly active comets where waves at the cometary ion gyro-frequencies are the main feature. We propose a cross-field current instability associated with the newborn cometary ions as a possible source mechanism. Read more
Three-dimensional morphology of equatorial plasma bubbles deduced from measurements onboard CHAMP Annales Geophysicae DOI 10.5194/angeo-33-129-2015 28 January 2015 Total electron content (TEC) between Low-Earth-Orbit (LEO) satellites and the Global Navigation Satellite System (GNSS) satellites can be used to constrain three-dimensional morphology of equatorial plasma bubbles (EPBs). TEC gradient observed along the LEO track is strongest when the corresponding GNSS satellite is located equatorward and westward of the LEO satellite. This anisotropy supports the idea that EPBs have three-dimensional shell structures. CHAMP">Read more
Experimental test of the ρ(1-α) evolution for rotational discontinuities: cluster magnetopause observations Annales Geophysicae DOI 10.5194/angeo-33-79-2015 15 January 2015 Rotational discontinuities (RDs) in plasma allow a magnetic connection between different plasma regimes. One of their defining relations describes a balance between changes in plasma mass density and pressure anisotropy. The paper uses the high time resolution data from the Cluster satellites to directly test that relation at the terrestrial magnetopause, when standard analysis predicts that this boundary behaves like an RD. The experimental evidence shows that the said relation is not fulfilled. Read more
Internally and externally induced deformations of the magnetospheric equatorial current as inferred from spacecraft data Annales Geophysicae DOI 10.5194/angeo-33-1-2015 6 January 2015 A new quantitative model of the global shape of the neutral sheet in the Earth’s magnetosphere is developed, parameterized by the dipole tilt, solar wind pressure, and IMF By and Bz. The model is based on data from the Polar, Cluster, Geotail, and Themis satellites taken in 1995-2013. The paper quantifies and further explains our earlier finding of the bowl-shaped deformation of the neutral sheet due to the Earth’s dipole tilt (Tsyganenko and Andreeva, GRL, v.41(4), 2014). Read more
A possible influence of the Great White Spot on Saturn kilometric radiation periodicity Annales Geophysicae DOI 10.5194/angeo-32-1463-2014 4 December 2014 In this paper we show that the large thunderstorm called Great White Spot, which raged for about 9 months in Saturn’s troposphere in 2010/2011, was accompanied by changes in the periodicity and phasing of auroral radio emissions. We suggest that the thunderstorm was a source of intense gravity waves causing a global change in Saturn’s ionospheric winds via energy and momentum deposition. This supports the theory that Saturn’s magnetospheric periodicities are driven by the upper atmosphere. Read more
A comparison between VEGA 1, 2 and Giotto flybys of comet 1P/Halley: implications for Rosetta Annales Geophysicae DOI 10.5194/angeo-32-1441-2014 28 November 2014 We discuss three flybys (within a time span of 8 days) of comet 1P/Halley by VEGA 1, 2 and Giotto. Looking at two different plasma phenomena: mirror mode waves and field line draping; we study the differences in SW-comet interaction between these three flybys. We find that on this time scale (comparable to Rosetta’s orbits) there is a significant difference, both caused by changing outgassing rate of the comet and changes in the solar wind. We discuss implications for Rosetta RPC observations. VEGA 1, 2 and Giotto flybys of comet 1P/Halley: implications for Rosetta">Read more
