Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995jgr...10017069c&link_type=abstract
Journal of Geophysical Research, Volume 100, Issue A9, p. 17069-17080
Astronomy and Astrophysics
Astrophysics
20
Interplanetary Physics: Solar Wind Plasma, Interplanetary Physics: Plasma Waves And Turbulence, Interplanetary Physics: Solar Cycle Variations, Solar Physics, Astrophysics, And Astronomy: Corona
Scientific paper
Observations of the coherence bandwidth of interplanetary scintillations (IPS) made at the Nançay Radio Observatory between 1982 and 1992 have been used to estimate the variance of electron density δN2e at solar distances of 5 to 15 Rs. These IPS observations are sensitive to scales of the order of 10 km; i.e., they measure the ``microscale variance,'' which is a small fraction of the total density variance. Measurements in the equatorial region are invariant over the solar activity cycle and show the same behavior with distance as the mean density, i.e., δN2e~N2e. They do not show a statistically significant change in the ``transonic region'' as reported by other observers (Lotova et al., 1985). Measurements over the polar region show a clear variation with the solar cycle. At solar maximum, δN2e is invariant with latitude, as is Ne (Withbroe, 1988). However, the apparent δN2e measured by IPS is about 10 times lower in the polar streams which form during the declining and minimum phases of solar activity. Compensation for the line of sight integration inherent in the IPS observations indicates that the local value of δN2e is actually about 15 times lower in the polar streams. We cannot estimate the latitude variation of the ``development'' of the compressive turbulence δNe/Ne between 5 and 15 Rs because measurements of Ne in the polar hole are lacking.
Bourgois Gabriel
Coles William A.
Grall Russell Robert
Klinglesmith M. T.
No associations
LandOfFree
Solar cycle changes in the level of compressive microturbulence near the Sun does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Solar cycle changes in the level of compressive microturbulence near the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar cycle changes in the level of compressive microturbulence near the Sun will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-828633