NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Change in interplanetary shock acceleration preceding STIP Interval 17The intensity and frequency of shock acceleration events in the interplanetary medium decreased dramatically in early 1985. Low energy ions were observed by IMP 8 at 1 AU and Voyagers 1 and 2 at 22 and 16 AU, respectively. Voyager 1 was at 25 deg heliographic latitude while IMP 8 and Voyager 2 were near the solar equatorial plane. The decrease in low energy shock events led to a drop in the average ion flux by a factor of 20 to 50. It started about day 10 of 1985 in the approximately .5 MeV channel on IMP8 and took approximately 75 days to reach the new, lower, background level. The decrease at the Voyagers started approximately 50 days later. The time delay between the start of the decrease at IMP and at Voyager 2 implies that decrease was convected outward with a velocity of approximately 535 km/sec. The intensity and frequency of interplanetary shock events remained at the lower level for at least 1.5 years.
Document ID
19880001337
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Gold, R. E.
(Johns Hopkins Univ. Laurel, MD., United States)
Decker, R. B.
(Johns Hopkins Univ. Laurel, MD., United States)
Lanzerotti, L. J.
(Bell Telephone Labs., Inc. Murray Hill, NJ., United States)
Mclennan, C. G.
(Bell Telephone Labs., Inc. Murray Hill, N. J., United States)
Date Acquired
September 5, 2013
Publication Date
September 14, 1987
Publication Information
Publication: Alabama Univ., Huntsville. STIP Symposium on Physical Interpretation of Solar(Interplanetary and Cometary Intervals
Subject Category
Solar Physics
Accession Number
88N10719
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available