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Observations and Discussion

Both of the above properties are systematically observed in our data (see Figures 2a and 2b (top)). This allows us to locate the largest tex2html_wrap_inline615 resonance in each observed harmonic band: a check of self-consistency can be made by comparing the different tex2html_wrap_inline611 resonances, using the theoretical Doppler-shifted dispersion curves, which are plotted, in the same frequency range, under each spectrum of Figures 2a and 2b. The abrupt drop of the spectral density is actually observed in about 80% of the spectra acquired by Ulysses between 1800 and 2300 UT. Because (1) contains tex2html_wrap_inline675 , this detection of a high noise level band (where multiple resonances occur), abruptly followed by the forbidden band where tex2html_wrap_inline853 is low, will allow us to determine the plasma density in a number of spectra. The problems to be solved are first to clearly identify the detected tex2html_wrap_inline611 and then to derive from that detection the plasma frequency or more exactly the cold plasma frequency as discussed below.

  figure134
Figure 2a: Two power spectra at 1912 and 1931 UT showing abrupt drops together with the corresponding dispersion curves and the derived tex2html_wrap_inline617 . (top) The solid line is the average of individual measurements (dots) over a frequency step (i.e., 4 measurements acquired in 2 s). The abrupt drop of the signal level at tex2html_wrap_inline619 is indicated by an arrow. The variation of tex2html_wrap_inline861 is plotted at the top with its minima indicated as vertical dotted lines. (bottom) Dispersion curves computed by fitting the values of tex2html_wrap_inline619 to the observed abrupt drop frequencies are shown; they are plotted with fixed tex2html_wrap_inline625 and various tex2html_wrap_inline627 (10, 15, 25, 35, and 50). Note that tex2html_wrap_inline619 which defines the low-frequency side of the forbidden band (grey strip), is only a function of tex2html_wrap_inline631 . The gyrofrequency tex2html_wrap_inline633 is deduced from the magnetometer data at the time of the signal drop.

  figure143
Figure 2b: Two power spectra at 1944 and 2008 UT, showing the abrupt drops (top) and the dispersion curves (bottom) with the forbidden bands (grey strips), plotted as in Figure 2a with the same notations. Since tex2html_wrap_inline633 was lower than for the spectra shown in Figure 2a, we observe an additional intraharmonic band tex2html_wrap_inline637 including the resonance tex2html_wrap_inline639 which defines the low-frequency side of a second forbidden band.




next up previous
Next: Identifying the Q frequency Up: Detection of Bernstein wave Previous: Quasi-Thermal Noise in Bernstein

Michel Moncuquet
Tue Nov 18 19:11:02 MET 1997