Table 1.
Parameters calculated in the analysis of the zebras.
Date | f(s1) | s1 | A | Lchar | B | N | C | |
---|---|---|---|---|---|---|---|---|
DD:MM:YY | (MHz) | (G) | (108 cm−3) | |||||
25/10/94 | 144.8 | 78 | 0.00098 | 2.87 | 0.66 | 2.60 | 0.76 | |
17/08/98 | 260.3 | 78 | 0.0011 | 2.09 | 1.19 | 8.40 | 0.71 | |
14/02/99 | 1526 | 64 | 0.0053 | 4.60 | 8.52 | 289 | 0.76 | |
21/04/02 | 2668 | 52 | 0.0032 | 5.60 | 18.3 | 883 | 0.70 | |
01/08/10 | 1120 | 114 | 0.0044 | 6.48 | 3.51 | 156 | 0.86 | |
24/02/11 | 2977 | 70 | 0.0039 | 4.21 | 15.3 | 1100 | 0.70 | |
21/06/11 | 160.7 | 152 | 0.00064 | 3.50 | 0.38 | 3.20 | 0.47 |
Notes. f(s1) is the zebra-stripe frequency corresponding to the gyroharmonic number s1. A is the amplitude of the cosine approximation of variations dN/N and corresponding wavelength Lchar, B is the magnetic field strength, N is the plasma density, and C is the correlation coefficient between the analyzed variations and the fitted cosine function.
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