group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
48.24 | 299.00 | 26.30 | 162.94 | -6.99 | 139.25 | 20.33 | 235.86 | 0.4186 | 862.0 | 369.0 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
44.46 | 273.83 | 24.25 | 149.34 | -6.88 | 139.50 | 20.58 | 236.42 | 0.4207 | 1395.0 | 434.3 | |
1.89 | -1.00 | 1.03 | -1.00 | -6.95 | 138.98 | 20.07 | 235.59 | 0.4145 | 1283.4 | 999999 | |
0.00 | 1.71 | 0.00 | 0.94 | -9.20 | 138.77 | 19.85 | 231.01 | 0.4331 | 855.0 | 667.9 | |
0.00 | 2.51 | 0.00 | 1.44 | -15.83 | 138.33 | 19.42 | 220.02 | 0.4994 | -799.0 | -695.6 | |
0.00 | 1.17 | 0.00 | 0.63 | -6.70 | 137.39 | 18.47 | 233.83 | 0.3914 | 982.0 | 842.9 | |
0.54 | 2.34 | 0.29 | 1.26 | -7.56 | 137.16 | 18.25 | 231.73 | 0.3970 | 963.5 | 759.5 | |
0.72 | 1.80 | 0.39 | 0.97 | -7.78 | 137.04 | 18.13 | 231.12 | 0.3977 | 960.0 | 778.1 | |
0.00 | 1.62 | 0.00 | 0.86 | -5.96 | 136.91 | 17.99 | 234.66 | 0.3783 | -860.0 | -638.9 | |
0.63 | 7.72 | 0.34 | 4.15 | -7.50 | 136.49 | 17.57 | 230.78 | 0.3880 | -741.1 | -579.2 | |
0.00 | 1.17 | 0.00 | 0.62 | -5.56 | 135.34 | 16.42 | 233.00 | 0.3538 | -712.0 | -571.4 | |
0.00 | 1.35 | 0.00 | 0.72 | -6.27 | 135.32 | 16.41 | 231.40 | 0.3608 | -789.0 | -531.7 | |
0.00 | 0.99 | 0.00 | 0.52 | -4.96 | 135.13 | 16.21 | 234.02 | 0.3452 | -832.0 | -705.3 | |
0.00 | 1.53 | 0.00 | 0.83 | -10.29 | 135.30 | 16.39 | 223.56 | 0.4045 | -770.0 | -682.9 | |
0.00 | 1.26 | 0.00 | 0.66 | -5.14 | 134.91 | 16.00 | 233.23 | 0.3441 | -795.0 | -581.9 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |