SDO HMI 2011-10-12 22:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 140.12 | 636.46 | 102.98 | 468.74 | -12.34 | 48.49 | -44.35 | 112.80 | 0.7421 | 65.7 | -25.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.84 | -11.18 | 48.04 | -44.79 | 111.08 | 0.7430 | 690.0 | 553.9 | |
| 2.89 | 329.20 | 2.14 | 253.14 | -11.43 | 47.73 | -45.10 | 111.26 | 0.7473 | 597.0 | -291.7 | |
| 1.05 | 1.49 | 0.77 | 1.10 | -11.40 | 48.09 | -44.75 | 111.37 | 0.7434 | 373.8 | 418.4 | |
| 5.86 | -2.00 | 4.55 | -2.00 | -11.91 | 45.59 | -47.24 | 110.97 | 0.7717 | -611.5 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.86 | -11.81 | 46.78 | -46.06 | 111.34 | 0.7590 | -684.0 | -544.2 | |
| 0.00 | 1.05 | 0.00 | 0.77 | -11.79 | 48.69 | -44.14 | 112.14 | 0.7383 | 291.0 | 267.7 | |
| 1.40 | -2.00 | 1.07 | -2.00 | -12.08 | 46.14 | -46.70 | 111.41 | 0.7667 | -1085.0 | 999999 | |
| 1.14 | 2.62 | 0.82 | 1.88 | -11.97 | 49.97 | -42.87 | 112.97 | 0.7251 | 406.9 | 386.9 | |
| 49.42 | 244.80 | 34.37 | 169.99 | -11.93 | 51.83 | -41.00 | 113.84 | 0.7041 | 1018.4 | 358.9 | |
| 1.22 | -2.00 | 0.96 | -2.00 | -12.51 | 45.49 | -47.34 | 111.67 | 0.7748 | -420.9 | 999999 | |
| 12.86 | 15.13 | 9.18 | 10.80 | -12.20 | 50.30 | -42.54 | 113.42 | 0.7224 | 603.8 | 339.6 | |
| 37.52 | -2.00 | 29.03 | -2.00 | -12.57 | 45.93 | -46.90 | 111.92 | 0.7705 | -876.1 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -12.23 | 50.75 | -42.08 | 113.68 | 0.7176 | 517.0 | 425.7 | |
| 2.62 | 4.20 | 1.90 | 3.04 | -12.69 | 49.61 | -43.22 | 113.72 | 0.7321 | 517.4 | 374.1 | |
| 11.19 | -2.00 | 8.56 | -2.00 | -12.95 | 46.69 | -46.14 | 112.71 | 0.7641 | -1052.5 | 999999 | |
| 3.94 | 7.96 | 2.96 | 5.97 | -12.91 | 47.63 | -45.21 | 113.07 | 0.7542 | -854.3 | -689.0 | |
| 1.05 | -2.00 | 0.82 | -2.00 | -13.06 | 45.63 | -47.21 | 112.40 | 0.7754 | -342.5 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.34 | -12.83 | 49.07 | -43.76 | 113.64 | 0.7385 | -494.0 | -433.5 | |
| 0.00 | 1.31 | 0.00 | 0.95 | -12.81 | 49.71 | -43.12 | 113.92 | 0.7315 | 579.0 | 359.5 | |
| 0.79 | -2.00 | 0.61 | -2.00 | -13.26 | 46.30 | -46.53 | 112.93 | 0.7693 | -521.4 | 999999 | |
| 7.17 | 14.96 | 5.24 | 10.95 | -13.28 | 49.35 | -43.48 | 114.34 | 0.7374 | 671.3 | 70.6 | |
| 0.00 | 0.96 | 0.00 | 0.71 | -13.39 | 48.69 | -44.15 | 114.17 | 0.7450 | 270.0 | 158.5 | |
| 0.00 | 1.40 | 0.00 | 1.05 | -13.72 | 48.13 | -44.70 | 114.31 | 0.7522 | 462.0 | 420.6 | |
| 0.00 | 1.40 | 0.00 | 1.09 | -13.96 | 45.85 | -46.98 | 113.59 | 0.7766 | -544.0 | -441.8 | |
| 0.00 | 2.45 | 0.00 | 1.79 | -14.28 | 49.84 | -42.99 | 115.85 | 0.7367 | 749.0 | 585.5 | |
| 0.00 | 2.45 | 0.00 | 1.79 | -14.30 | 49.58 | -43.25 | 115.75 | 0.7395 | 625.0 | 407.9 | |
| 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. | |