group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
23.35 | 85.20 | 13.40 | 48.03 | -10.72 | 357.84 | 28.32 | 260.23 | 0.4759 | 419.3 | 318.5 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 2.34 | 0.00 | 1.36 | -7.91 | 1.37 | 31.84 | 266.59 | 0.5256 | 799.0 | 672.0 | |
0.00 | 1.04 | 0.00 | 0.61 | -14.55 | 2.19 | 32.67 | 254.27 | 0.5449 | 569.0 | 489.8 | |
1.56 | 5.30 | 0.90 | 3.06 | -8.03 | 0.88 | 31.36 | 266.37 | 0.5184 | 828.4 | 738.6 | |
0.43 | 3.13 | 0.25 | 1.80 | -7.71 | 0.68 | 31.16 | 266.99 | 0.5155 | 888.8 | 723.8 | |
0.00 | 0.78 | 0.00 | 0.45 | -13.29 | 1.12 | 31.60 | 256.31 | 0.5270 | 594.0 | 516.0 | |
0.00 | 3.47 | 0.00 | 2.00 | -7.82 | 0.44 | 30.92 | 266.79 | 0.5119 | 934.0 | 804.4 | |
0.00 | 1.22 | 0.00 | 0.70 | -6.73 | 0.22 | 30.70 | 268.95 | 0.5091 | 626.0 | 553.2 | |
0.00 | 1.48 | 0.00 | 0.85 | -7.50 | 0.24 | 30.72 | 267.42 | 0.5090 | 923.0 | 823.4 | |
0.00 | 0.78 | 0.00 | 0.45 | -7.09 | 0.17 | 30.65 | 268.24 | 0.5082 | 775.0 | 695.1 | |
0.00 | 1.30 | 0.00 | 0.75 | -7.64 | 359.97 | 30.45 | 267.17 | 0.5049 | 911.0 | 748.7 | |
14.85 | 20.15 | 8.53 | 11.57 | -9.87 | 0.14 | 30.61 | 262.74 | 0.5078 | 1030.9 | 684.4 | |
6.51 | 8.42 | 3.72 | 4.82 | -9.24 | 359.72 | 30.20 | 263.97 | 0.5013 | 1008.0 | 728.5 | |
0.00 | 2.17 | 0.00 | 1.22 | -10.95 | 357.53 | 28.01 | 260.16 | 0.4699 | 691.0 | 591.0 | |
0.00 | 0.87 | 0.00 | 0.49 | -10.87 | 357.42 | 27.90 | 260.32 | 0.4681 | 702.0 | 620.4 | |
0.00 | 1.04 | 0.00 | 0.58 | -11.05 | 357.37 | 27.85 | 259.92 | 0.4676 | 672.0 | 531.2 | |
0.00 | 0.87 | 0.00 | 0.49 | -15.09 | 357.24 | 27.71 | 251.39 | 0.4758 | 648.0 | 515.0 | |
0.00 | 1.56 | 0.00 | 0.87 | -11.74 | 356.82 | 27.30 | 258.31 | 0.4605 | 833.0 | 622.7 | |
0.00 | 1.22 | 0.00 | 0.68 | -14.46 | 357.05 | 27.52 | 252.59 | 0.4709 | 832.0 | 701.7 | |
0.00 | 1.22 | 0.00 | 0.68 | -11.51 | 356.59 | 27.07 | 258.74 | 0.4566 | 841.0 | 651.6 | |
0.00 | 1.82 | 0.00 | 1.02 | -12.95 | 356.72 | 27.20 | 255.67 | 0.4616 | 670.0 | 516.5 | |
0.00 | 1.56 | 0.00 | 0.88 | -15.34 | 356.96 | 27.44 | 250.73 | 0.4727 | 788.0 | 678.2 | |
0.00 | 1.82 | 0.00 | 1.02 | -14.69 | 356.76 | 27.24 | 252.00 | 0.4675 | 804.0 | 639.0 | |
0.00 | 2.69 | 0.00 | 1.49 | -11.53 | 356.32 | 26.80 | 258.64 | 0.4525 | 798.0 | 718.7 | |
0.00 | 0.87 | 0.00 | 0.48 | -11.32 | 356.23 | 26.71 | 259.07 | 0.4508 | 834.0 | 665.9 | |
0.00 | 2.78 | 0.00 | 1.56 | -16.72 | 356.67 | 27.15 | 247.75 | 0.4741 | -720.0 | -613.5 | |
0.00 | 0.35 | 0.00 | 0.19 | -14.32 | 355.30 | 25.78 | 252.11 | 0.4447 | 602.0 | 654.8 | |
0.00 | 0.69 | 0.00 | 0.38 | -16.17 | 355.00 | 25.47 | 247.89 | 0.4477 | -570.0 | -489.9 | |
0.00 | 1.22 | 0.00 | 0.67 | -17.16 | 354.76 | 25.23 | 245.64 | 0.4490 | -754.0 | -580.9 | |
0.00 | 0.87 | 0.00 | 0.47 | -14.69 | 352.51 | 22.98 | 249.64 | 0.4046 | -657.0 | -459.2 | |
0.00 | 1.04 | 0.00 | 0.56 | -14.62 | 352.06 | 22.54 | 249.51 | 0.3977 | -714.0 | -553.2 | |
0.00 | 0.96 | 0.00 | 0.51 | -10.54 | 351.53 | 22.01 | 259.64 | 0.3762 | -716.0 | -520.6 | |
0.00 | 0.87 | 0.00 | 0.47 | -14.49 | 351.62 | 22.10 | 249.52 | 0.3904 | -830.0 | -676.3 | |
0.00 | 1.22 | 0.00 | 0.65 | -13.32 | 351.01 | 21.48 | 252.09 | 0.3762 | -836.0 | -760.6 | |
0.00 | 2.34 | 0.00 | 1.24 | -9.27 | 349.89 | 20.37 | 262.72 | 0.3478 | -900.0 | -712.0 | |
0.00 | 1.48 | 0.00 | 0.78 | -15.36 | 349.62 | 20.10 | 245.72 | 0.3651 | -685.0 | -550.2 | |
0.00 | 1.65 | 0.00 | 0.87 | -9.33 | 349.06 | 19.53 | 262.33 | 0.3344 | -747.0 | -459.7 | |
0.00 | 0.96 | 0.00 | 0.50 | -13.33 | 346.79 | 17.26 | 248.72 | 0.3113 | -788.0 | -633.2 | |
0.00 | 1.65 | 0.00 | 0.86 | -13.07 | 346.54 | 17.02 | 249.29 | 0.3062 | -1036.0 | -877.8 |
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. |