Analysis of the heliospheric current sheet at Earth's orbit and model comparisons

Details Analysis of the heliospheric current sheet at Earth's orbit and model comparisons Analysis of the heliospheric current sheet at Earth's orbit and model comparisons

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...95l&link_type=abstract

NASA Goddard Space Flight Center, International Solar Wind 8 Conference, p. 95

Physics

Current Sheets, Solar Magnetic Field, Atmospheric Models, Sun, Earth (Planet), Structural Analysis, Solar Physics, Heliosphere, Satellite Observation, Time Series Analysis, Solar Orbits, Earth Orbits, Explorer 50 Satellite, Solar Planetary Interactions

Scientific paper

IMP 8 magnetic field data for the first half of the year 1994, i.e., for about 6 solar rotations, are analyzed around regions of sector boundary crossings with the purpose of obtaining both gross- and fine-scale characteristics of the related heliospheric current sheets separating the observed sectors. For purposes of estimating the attitudes of the normals to the sector boundaries. analysis intervals (sometimes 30 min or more in length) allowing the field to fully complete an excursion of about 180 deg were used in the study, which consisted of variance analyses of the field within those intervals. The resulting boundary normals were analyzed and compared to known (generic) models of projected heliospheric current sheets and to a coronal field model for the same time period. One of the most outstanding features of the resulting ensemble of estimated boundary normals for this period is that they strongly prefer low inclinations, indicating that the observations do not support a 1 AU model that predicts a current sheet whose surface is approximately parallel with the sun's equator, such as the 'sombrero' model. They instead support a model that predicts a relatively high inclination current sheet at 1 AU. Also the normals assume a surprisingly large range of longitudes, somewhat favoring those consistent with a Parker model (45 deg and 225 deg) and/or radial alignment (0 deg and 180 deg). These boundary structures, as defined, are shown typically to be as broad as several hundred proton gyroradii, but having embedded within them very thin structures associated with stronger currents. Such thin structures have normals usually differing markedly from the gross boundary. For some crossings there are indications of a wave-like structure in the current sheet as it passed the spacecraft.

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