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Magnetic Lasso: A New Kinematic Solar Wind Propagation Method. Magnetic Lasso Propagation
DOI: 10.1007/s11207-018-1340-3 Bibcode: 2018SoPh..293..127D

Dósa, M.; Opitz, A.; Dálya, Z. +1 more

Solar wind propagation from the point of measurement to an arbitrary target in the heliosphere is an important input for heliospheric, planetary and cometary studies. In this paper a new kinematic propagation method, the magnetic lasso method is presented. Compared to the simple ballistic approach our method is based on reconstructing the ideal Pa…

2018 Solar Physics
MEx 4
Coronal Radio Occultation Experiments with the Helios Solar Probes: Correlation/Spectral Analysis of Faraday Rotation Fluctuations
DOI: 10.1007/s11207-015-0687-y Bibcode: 2015SoPh..290.2397E

Pätzold, M.; Bird, M. K.; Efimov, A. I. +4 more

The coronal Faraday rotation (FR) experiments using the linearly polarized signals of the Helios-1 and Helios-2 interplanetary probes remain a unique investigation of the magnetic field of the solar corona and its aperiodic and quasi-periodic variations. The unexpectedly long lifetime of these spacecraft (1974 - 1986) enabled studies from very dee…

2015 Solar Physics
MEx 9
Two-Way Frequency Fluctuations Observed During Coronal Radio Sounding Experiments
DOI: 10.1007/s11207-013-0417-2 Bibcode: 2014SoPh..289.1715E

Pätzold, M.; Bird, M. K.; Efimov, A. I. +5 more

Coronal radio-sounding experiments were carried out using two-way coherent dual-frequency carrier signals of the ESA spacecraft Rosetta (ROS) in 2006. Frequency measurements recorded at both NASA and ESA tracking stations (sample rate: 1 Hz) are analyzed in this work. Spectral analysis of the S-band, X-band, and differential frequency records has …

2014 Solar Physics
MEx Rosetta Ulysses 5
Coronal Density Structures and CMEs: Superior Solar Conjunctions of Mars Express, Venus Express, and Rosetta: 2004, 2006, and 2008
DOI: 10.1007/s11207-012-9991-y Bibcode: 2012SoPh..279..127P

Tellmann, Silvia; Tyler, G. Leonard; Tsurutani, Bruce T. +5 more

Coronal radio-sounding experiments were carried out using the S-band (2.3 GHz) and X-band (8.4 GHz) signals of the ESA Mars Express, Venus Express, and Rosetta spacecraft during five superior conjunctions occurring in 2004, 2006 (3×), and 2008/2009. Differential frequency and propagation delay (ranging) observations were recorded during these oppo…

2012 Solar Physics
MEx Rosetta SOHO Ulysses VenusExpress 21
Solar-Wind Bulk Velocity Throughout the Inner Heliosphere from Multi-Spacecraft Measurements
DOI: 10.1007/s11207-010-9583-7 Bibcode: 2010SoPh..264..377O

Fedorov, A.; Barabash, S.; Sauvaud, J. -A. +6 more

We extrapolate solar-wind bulk velocity measurements for different in-ecliptic heliospheric positions by calculating the theoretical time lag between the locations. The solar-wind bulk velocity dataset is obtained from in-situ plasma measurements by STEREO A and B, SOHO, Venus Express, and Mars Express. During their simultaneous measurements betwe…

2010 Solar Physics
MEx SOHO VenusExpress 16