| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.44 | 344.36 | 97.09 | 320.98 | -15.60 | 266.50 | -55.67 | 110.17 | 0.8487 | 63.6 | 43.7 | |
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back to the solar disc SDO HMI 2011-11-19 03:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.26 | 109.29 | 2.78 | 94.26 | -16.81 | 270.47 | -51.71 | 112.67 | 0.8165 | 872.4 | 337.4 | |
| 21.12 | -1.00 | 18.27 | -1.00 | -16.67 | 269.81 | -52.37 | 112.30 | 0.8222 | 764.8 | 999999 | |
| 3.09 | -1.00 | 2.70 | -1.00 | -17.15 | 269.57 | -52.61 | 112.79 | 0.8257 | 413.7 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.70 | -17.66 | 268.31 | -53.87 | 113.01 | 0.8383 | 584.0 | 413.6 | |
| 0.00 | 2.32 | 0.00 | 2.11 | -17.42 | 267.98 | -54.19 | 112.63 | 0.8405 | 585.0 | 415.8 | |
| 0.00 | 1.97 | 0.00 | 1.80 | -17.21 | 267.81 | -54.37 | 112.34 | 0.8415 | 513.0 | 360.0 | |
| 0.00 | 2.83 | 0.00 | 2.52 | -12.97 | 267.72 | -54.45 | 107.37 | 0.8330 | 689.0 | 608.2 | |
| 17.77 | 67.39 | 16.82 | 64.52 | -16.55 | 266.13 | -56.04 | 111.12 | 0.8544 | -760.4 | -267.0 | |
| 8.76 | 62.84 | 7.95 | 56.94 | -13.55 | 267.05 | -55.13 | 107.88 | 0.8402 | 693.3 | 244.8 | |
| 6.27 | -9.00 | 5.67 | -9.00 | -13.21 | 267.11 | -55.06 | 107.50 | 0.8390 | 726.9 | 999999 | |
| 0.00 | 2.58 | 0.00 | 2.39 | -14.52 | 266.48 | -55.70 | 108.88 | 0.8473 | 425.0 | 323.2 | |
| 0.00 | 0.69 | 0.00 | 0.65 | -15.63 | 265.69 | -56.48 | 109.96 | 0.8563 | -526.0 | -449.9 | |
| 0.00 | 1.37 | 0.00 | 1.28 | -14.31 | 266.23 | -55.95 | 108.58 | 0.8491 | 531.0 | 369.6 | |
| 9.53 | -8.00 | 9.39 | -8.00 | -16.82 | 264.76 | -57.42 | 111.07 | 0.8664 | 598.9 | 999999 | |
| 1.03 | 15.88 | 1.00 | 15.37 | -16.19 | 265.05 | -57.12 | 110.43 | 0.8627 | -372.7 | -508.2 | |
| 2.15 | -15.00 | 2.08 | -15.00 | -15.94 | 265.11 | -57.07 | 110.16 | 0.8618 | -383.8 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.89 | -13.54 | 265.58 | -56.60 | 107.53 | 0.8533 | 416.0 | 299.9 | |
| 5.41 | 7.55 | 5.08 | 7.10 | -13.07 | 265.63 | -56.55 | 107.01 | 0.8520 | 387.5 | 81.1 | |
| 0.00 | 0.86 | 0.00 | 0.81 | -13.36 | 265.47 | -56.70 | 107.30 | 0.8538 | 248.0 | 179.4 | |
| 0.00 | 1.55 | 0.00 | 1.50 | -14.55 | 264.73 | -57.45 | 108.50 | 0.8624 | 528.0 | 352.6 | |
| 0.00 | 0.86 | 0.00 | 0.86 | -16.23 | 263.99 | -58.19 | 110.21 | 0.8715 | -517.0 | -462.3 | |
| 0.00 | 1.12 | 0.00 | 1.13 | -16.58 | 263.70 | -58.48 | 110.54 | 0.8745 | -569.0 | -455.1 | |
| 1.12 | 4.46 | 1.13 | 4.53 | -16.06 | 263.54 | -58.64 | 109.92 | 0.8748 | -506.1 | -443.5 | |
| 1.12 | 1.46 | 1.17 | 1.53 | -17.62 | 262.74 | -59.44 | 111.47 | 0.8838 | 202.8 | 149.2 | |
| 0.00 | 0.52 | 0.00 | 0.49 | -12.55 | 264.92 | -57.26 | 106.25 | 0.8572 | 486.0 | 436.3 | |
| 0.00 | 0.94 | 0.00 | 0.97 | -16.04 | 263.18 | -58.99 | 109.82 | 0.8776 | -526.0 | -453.3 | |
| 4.89 | 5.67 | 5.24 | 6.06 | -17.49 | 262.07 | -60.11 | 111.16 | 0.8887 | -568.1 | -548.3 | |
| 0.00 | 0.86 | 0.00 | 0.85 | -13.76 | 263.83 | -58.34 | 107.39 | 0.8684 | -674.0 | -575.7 | |
| 0.00 | 0.77 | 0.00 | 0.81 | -16.69 | 262.49 | -59.68 | 110.38 | 0.8841 | -459.0 | -422.6 | |
| 0.00 | 1.12 | 0.00 | 1.12 | -14.20 | 263.60 | -58.58 | 107.84 | 0.8711 | -548.0 | -521.8 | |
| 8.33 | 28.76 | 8.48 | 29.37 | -14.00 | 262.96 | -59.22 | 107.49 | 0.8760 | -715.3 | -300.1 | |
| 0.00 | 1.55 | 0.00 | 1.72 | -17.72 | 260.91 | -61.27 | 111.16 | 0.8975 | -402.0 | -333.2 | |
| 0.00 | 1.72 | 0.00 | 1.84 | -15.41 | 261.64 | -60.54 | 108.78 | 0.8885 | -657.0 | -527.4 | |
| 0.00 | 0.69 | 0.00 | 0.76 | -16.72 | 260.89 | -61.28 | 110.06 | 0.8961 | -403.0 | -327.1 | |
| 8.59 | 13.91 | 9.33 | 15.10 | -15.21 | 261.17 | -61.01 | 108.46 | 0.8918 | -393.9 | -247.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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 | |
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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. | |