Abstract
Solar wind plasma and magnetic field measurements from Pioneers 9 and 10 during August 2–17, 1972, reveal complex and large-amplitude variations on a one-hour time scale and numerous discontinuities. During this time period an approximate radial alignment of the two spacecraft as seen from the Sun occurred with heliocentric distances of 0.8 AU for Pioneer 9 and 2.2 AU for Pioneer 10, both at 45° east of the Earth’s solar longitude. The peak hourly average solar wind proton bulk velocity measured at Pioneer 9 was 990 km s−1 during hour 0 UT of August 5. The peak hourly average proton number density was 62 cm−3 during hour 11 UT of August 3. The peak solar wind speeds are generally much reduced at Pioneer 10 compared with those observed at Pioneer 9. The peak 30-min average magnetic field magnitude was 85 γ during 1245–1315 UT of August 3. The Pioneer 9 data indicate passage of four fast forward interplanetary shocks, and one slow forward interplanetary shock.
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© 1974 D. Reidel Publishing Company, Dordrecht-Holland
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Mihalov, J.D., Colburn, D.S., Collard, H.R., Smith, B.F., Sonett, C.P., Wolfe, J.H. (1974). Pioneer Solar Plasma and Magnetic Field Measurements in Interplanetary Space during August 2–17, 1972. In: Page, D.E. (eds) Correlated Interplanetary and Magnetospheric Observations. Astrophysics and Space Science Library, vol 42. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2172-2_35
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DOI: https://doi.org/10.1007/978-94-010-2172-2_35
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