Latitudinal gradient of energetic particles in the outer hemisphere during 1985-1986

Physics

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Current Sheets, Energetic Particles, Galactic Cosmic Rays, Heliosphere, Interplanetary Magnetic Fields, Solar Rotation, Imp, Interplanetary Medium, Solar Flares, Solar System, Solar Wind Velocity, Voyager Project

Scientific paper

The authors report a measurement of a sustained latitudinal gradient of 70-MeV galactic cosmic ray protons using data from the interplanetary probes Voyager 1 and 2 and the earth-orbiting satellite IMP 8 during a 1-year period from mid-1985 to mid-1986. They determine an average latitudinal gradient during this period of (-0.53±0.10)% deg-1 or (-0.38±0.11)% deg-1 (i.e., intensity decreasing northward of the solar equatorial plane), assuming either a constant radial gradient or one that decreased at an average rate of -0.025% AU-1, as was the case during 1984, respectively. In addition, the authors present Voyager data at very low (⪆30 keV) ion energies which are associated with acceleration at corotating shocks. These ions also exhibit a latitudinal gradient (≡ -3% deg-1), with lower intensities at higher latitudes, and serve to highlight changes that occurred in the interplanetary medium in early 1985.

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