group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
14.05 | 72.87 | 8.80 | 44.46 | -10.22 | 358.12 | 35.74 | 262.12 | 0.5826 | 198.0 | 291.5 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 0.78 | 0.00 | 0.50 | -7.83 | 1.77 | 39.39 | 266.43 | 0.6322 | 220.0 | 270.1 | |
2.34 | 5.81 | 1.49 | 3.69 | -7.86 | 1.35 | 38.97 | 266.40 | 0.6265 | 740.5 | 584.9 | |
0.00 | 1.30 | 0.00 | 0.82 | -7.22 | 1.16 | 38.79 | 267.44 | 0.6243 | 473.0 | 462.3 | |
0.00 | 1.30 | 0.00 | 0.82 | -7.43 | 1.11 | 38.73 | 267.10 | 0.6235 | 594.0 | 523.8 | |
0.00 | 0.52 | 0.00 | 0.33 | -7.95 | 0.97 | 38.59 | 266.27 | 0.6214 | 539.0 | 538.2 | |
0.00 | 1.91 | 0.00 | 1.20 | -6.80 | 0.74 | 38.36 | 268.15 | 0.6188 | 462.0 | 489.8 | |
0.00 | 0.87 | 0.00 | 0.55 | -5.71 | 0.53 | 38.15 | 269.94 | 0.6170 | 394.0 | 348.7 | |
0.00 | 0.69 | 0.00 | 0.44 | -7.54 | 0.50 | 38.13 | 266.97 | 0.6152 | 582.0 | 585.0 | |
0.00 | 1.22 | 0.00 | 0.76 | -7.97 | 0.40 | 38.02 | 266.28 | 0.6135 | 582.0 | 470.6 | |
0.00 | 1.56 | 0.00 | 0.97 | -7.09 | 0.15 | 37.78 | 267.73 | 0.6106 | 632.0 | 628.9 | |
0.00 | 2.52 | 0.00 | 1.57 | -6.82 | 0.13 | 37.75 | 268.17 | 0.6105 | 646.0 | 477.7 | |
0.00 | 1.04 | 0.00 | 0.66 | -12.90 | 0.95 | 38.58 | 258.28 | 0.6230 | 269.0 | 430.4 | |
9.11 | 17.18 | 5.69 | 10.71 | -9.78 | 0.15 | 37.78 | 263.30 | 0.6101 | 863.8 | 488.7 | |
2.60 | 6.68 | 1.62 | 4.15 | -9.17 | 359.85 | 37.47 | 264.30 | 0.6058 | 792.0 | 608.9 | |
0.00 | 2.69 | 0.00 | 1.65 | -8.76 | 359.00 | 36.62 | 265.00 | 0.5941 | 736.0 | 672.5 | |
0.00 | 2.86 | 0.00 | 1.77 | -13.09 | 359.24 | 36.86 | 257.73 | 0.6002 | 833.0 | 661.5 | |
0.00 | 3.21 | 0.00 | 1.94 | -10.99 | 357.49 | 35.11 | 261.09 | 0.5737 | 693.0 | 610.3 | |
0.00 | 0.95 | 0.00 | 0.57 | -10.55 | 357.32 | 34.94 | 261.84 | 0.5710 | 643.0 | 574.2 | |
0.00 | 1.04 | 0.00 | 0.63 | -11.06 | 357.01 | 34.63 | 260.93 | 0.5670 | 675.0 | 662.5 | |
0.00 | 0.95 | 0.00 | 0.58 | -15.25 | 357.39 | 35.01 | 253.70 | 0.5789 | 641.0 | 534.1 | |
0.00 | 1.39 | 0.00 | 0.83 | -11.83 | 356.71 | 34.33 | 259.53 | 0.5636 | 601.0 | 547.9 | |
0.00 | 0.52 | 0.00 | 0.31 | -16.58 | 356.00 | 33.62 | 250.96 | 0.5635 | -484.0 | -454.3 | |
0.00 | 1.04 | 0.00 | 0.62 | -16.23 | 355.89 | 33.51 | 251.55 | 0.5610 | -538.0 | -419.6 | |
0.00 | 1.22 | 0.00 | 0.72 | -14.67 | 355.20 | 32.82 | 254.11 | 0.5474 | 728.0 | 715.0 | |
0.00 | 1.22 | 0.00 | 0.71 | -16.58 | 354.15 | 31.77 | 250.26 | 0.5382 | -645.0 | -549.3 | |
0.00 | 0.35 | 0.00 | 0.20 | -8.69 | 352.87 | 30.49 | 265.08 | 0.5055 | -550.0 | -580.5 | |
0.00 | 1.13 | 0.00 | 0.66 | -16.47 | 353.58 | 31.20 | 250.24 | 0.5299 | -741.0 | -561.5 | |
0.00 | 1.04 | 0.00 | 0.60 | -12.25 | 352.55 | 30.17 | 257.98 | 0.5041 | -670.0 | -434.5 | |
0.00 | 1.56 | 0.00 | 0.89 | -14.07 | 352.29 | 29.92 | 254.33 | 0.5045 | -701.0 | -575.4 | |
0.00 | 0.78 | 0.00 | 0.44 | -10.65 | 351.66 | 29.28 | 261.03 | 0.4887 | -573.0 | -545.8 | |
0.00 | 0.95 | 0.00 | 0.54 | -13.19 | 351.82 | 29.44 | 255.91 | 0.4954 | -679.0 | -499.1 | |
0.00 | 0.87 | 0.00 | 0.49 | -14.01 | 351.16 | 28.78 | 254.04 | 0.4878 | -662.0 | -557.1 | |
0.00 | 0.95 | 0.00 | 0.54 | -11.04 | 350.63 | 28.25 | 260.04 | 0.4736 | -706.0 | -479.8 | |
0.00 | 1.30 | 0.00 | 0.71 | -7.75 | 347.38 | 25.00 | 267.10 | 0.4212 | -666.0 | -498.1 | |
0.00 | 1.82 | 0.00 | 0.99 | -13.01 | 346.89 | 24.51 | 254.48 | 0.4212 | -737.0 | -583.9 | |
0.00 | 0.87 | 0.00 | 0.47 | -14.22 | 346.78 | 24.40 | 251.63 | 0.4238 | -610.0 | -491.4 | |
0.00 | 0.78 | 0.00 | 0.43 | -16.54 | 346.25 | 23.87 | 246.03 | 0.4264 | -809.0 | -621.4 |
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. |