group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
24.60 | 150.41 | 22.15 | 133.46 | -1.61 | 153.39 | 55.94 | 272.96 | 0.8309 | -503.6 | -181.5 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
23.05 | 119.49 | 20.86 | 108.26 | -1.63 | 154.22 | 56.77 | 272.79 | 0.8393 | -855.5 | -198.3 | |
0.00 | 1.30 | 0.00 | 1.17 | -3.60 | 154.24 | 56.79 | 270.44 | 0.8372 | -271.0 | -243.5 | |
0.00 | 3.19 | 0.00 | 2.84 | -0.25 | 153.38 | 55.93 | 274.57 | 0.8331 | -704.0 | -518.6 | |
0.00 | 0.95 | 0.00 | 0.83 | -2.64 | 152.82 | 55.37 | 271.79 | 0.8246 | 225.0 | 178.1 | |
0.00 | 2.76 | 0.00 | 2.37 | -1.37 | 152.09 | 54.63 | 273.45 | 0.8189 | -561.0 | -462.5 | |
0.00 | 1.38 | 0.00 | 1.17 | -2.42 | 151.77 | 54.32 | 272.22 | 0.8144 | -637.0 | -570.8 | |
0.00 | 2.94 | 0.00 | 2.50 | -1.38 | 151.67 | 54.22 | 273.50 | 0.8148 | -681.0 | -632.1 | |
0.00 | 0.52 | 0.00 | 0.44 | -1.60 | 151.63 | 54.18 | 273.25 | 0.8141 | -636.0 | -584.7 | |
1.55 | 5.27 | 1.29 | 4.35 | -1.59 | 150.52 | 53.07 | 273.44 | 0.8028 | -791.8 | -570.2 | |
0.00 | 0.69 | 0.00 | 0.56 | -3.00 | 150.19 | 52.74 | 271.74 | 0.7975 | -567.0 | -500.4 | |
0.00 | 1.90 | 0.00 | 1.52 | -2.09 | 149.07 | 51.62 | 273.06 | 0.7868 | 645.0 | 470.1 | |
0.00 | 0.78 | 0.00 | 0.61 | 1.08 | 147.48 | 50.03 | 277.40 | 0.7750 | 515.0 | 453.6 | |
0.00 | 2.16 | 0.00 | 1.64 | 3.01 | 145.92 | 48.47 | 280.26 | 0.7620 | 563.0 | 407.7 | |
0.00 | 0.78 | 0.00 | 0.58 | -2.68 | 145.44 | 47.99 | 272.91 | 0.7455 | 360.0 | 294.3 | |
0.00 | 2.33 | 0.00 | 1.72 | -2.85 | 145.27 | 47.82 | 272.72 | 0.7433 | 526.0 | 406.8 | |
0.00 | 1.90 | 0.00 | 1.39 | -2.90 | 145.01 | 47.55 | 272.69 | 0.7401 | 638.0 | 570.4 | |
0.00 | 2.07 | 0.00 | 1.51 | -2.77 | 144.78 | 47.33 | 272.90 | 0.7377 | 744.0 | 688.6 |
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. |