SDO HMI 2011-11-12 20:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.67 | 277.61 | 17.64 | 141.16 | 9.96 | 55.57 | 10.44 | 306.19 | 0.2234 | -541.7 | -316.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.82 | 218.94 | 6.53 | 111.56 | 9.34 | 57.43 | 12.30 | 297.40 | 0.2379 | -1365.6 | -476.6 | |
| 20.22 | -1.00 | 10.29 | -1.00 | 9.50 | 57.03 | 11.91 | 298.73 | 0.2331 | -1507.4 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 11.60 | 56.62 | 11.50 | 307.12 | 0.2460 | -890.0 | -698.5 | |
| 0.00 | 2.15 | 0.00 | 1.09 | 11.00 | 55.86 | 10.73 | 306.93 | 0.2297 | -811.0 | -669.3 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 11.87 | 55.86 | 10.74 | 309.90 | 0.2387 | -828.0 | -505.6 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 9.01 | 55.64 | 10.51 | 299.69 | 0.2084 | -824.0 | -464.0 | |
| 0.00 | 3.70 | 0.00 | 1.88 | 9.96 | 55.58 | 10.45 | 303.73 | 0.2158 | -819.0 | -732.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 11.91 | 55.56 | 10.43 | 310.81 | 0.2351 | -662.0 | -517.7 | |
| 0.00 | 1.38 | 0.00 | 0.70 | 12.63 | 55.12 | 9.99 | 314.32 | 0.2378 | 923.0 | 703.6 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 16.58 | 53.30 | 8.17 | 329.65 | 0.2708 | 829.0 | 676.7 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 10.74 | 51.55 | 6.42 | 320.29 | 0.1727 | -655.0 | -493.1 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 13.15 | 50.10 | 4.98 | 334.06 | 0.1940 | 801.0 | 688.9 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 12.70 | 49.73 | 4.60 | 334.74 | 0.1843 | 1097.0 | 910.3 | |
| 0.00 | 4.56 | 0.00 | 2.37 | 19.86 | 49.71 | 4.58 | 345.35 | 0.2985 | 581.0 | 600.8 | |
| 1.63 | 3.87 | 0.82 | 1.94 | 10.06 | 49.05 | 3.92 | 330.75 | 0.1386 | -1030.2 | -792.6 | |
| 0.00 | 2.32 | 0.00 | 1.16 | 9.35 | 48.83 | 3.71 | 329.42 | 0.1259 | -1019.0 | -737.8 | |
| 0.00 | 2.41 | 0.00 | 1.21 | 10.66 | 48.55 | 3.42 | 335.85 | 0.1439 | -1145.0 | -904.0 | |
| 0.00 | 1.98 | 0.00 | 0.99 | 10.25 | 48.33 | 3.20 | 335.99 | 0.1358 | -647.0 | -492.1 | |
| 0.00 | 1.20 | 0.00 | 0.60 | 11.00 | 47.88 | 2.76 | 340.90 | 0.1450 | -647.0 | -625.0 | |
| 0.00 | 1.55 | 0.00 | 0.77 | 9.32 | 47.81 | 2.68 | 336.73 | 0.1175 | 934.0 | 733.9 | |
| 0.00 | 1.98 | 0.00 | 0.99 | 10.79 | 47.25 | 2.12 | 344.69 | 0.1383 | 1063.0 | 839.5 | |
| 0.00 | 11.01 | 0.00 | 5.51 | 11.15 | 45.95 | 0.82 | 354.21 | 0.1403 | 1174.0 | 901.2 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 11.51 | 45.95 | 0.82 | 354.45 | 0.1465 | 901.0 | 663.7 | |
| 0.00 | 4.73 | 0.00 | 2.36 | 10.55 | 45.92 | 0.79 | 353.97 | 0.1299 | 788.0 | 910.5 | |
| 0.00 | 0.86 | 0.00 | 0.43 | 12.80 | 45.92 | 0.80 | 355.36 | 0.1688 | 856.0 | 670.1 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 17.44 | 45.32 | 0.19 | 359.25 | 0.2478 | 890.0 | 680.5 | |
| 0.00 | 1.20 | 0.00 | 0.61 | 12.92 | 45.13 | 0.01 | 359.96 | 0.1703 | 827.0 | 600.9 | |
| 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. | |