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

Journal Article · · J. Geophys. Res.; (United States)
We 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. Starting in early 1985 the intensity of cosmic rays at Voyager 2 began increasing faster than that at Voyager 1. By mid- 1985 the intensity at Voyager 2 (helioradius 17 AU, heliolatitude --0/sup 0/) exceeded and remained higher than that at Voyager 1 (helioradius 24 AU, heliolatitude --26/sup 0/) for at least 14 solar rotations. Using the Voyager 2-IMP 8 data to correct for the radial gradient, we determine an average latitudinal gradient during this period of (-0.53 +- 0.10)% deg/sup -1/ or (-0.38 +- 0.11)% deg/sup -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/sup -1/ AU/sup -1/, as was the case during 1984, respectively. In addition, we present Voyager data at very low (approx. >30 keV) ion energies which are associated with acceleration at corotating shocks. These ions also exhibit a latitudinal gradient (---3% deg/sup -1/), with lower intensities at higher latitudes, and serve to highlight changes that occurred in the interplanetary medium in early 1985. Copyright American Geophysical Union 1987.
Research Organization:
Applied Physics Laboratory, John Hopkins University, Laurel, Maryland
OSTI ID:
6569728
Journal Information:
J. Geophys. Res.; (United States), Journal Name: J. Geophys. Res.; (United States) Vol. 92:A4; ISSN JGREA
Country of Publication:
United States
Language:
English