SDO HMI 2011-10-12 12:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.92 | 158.23 | 39.51 | 119.10 | 9.66 | 49.14 | -49.21 | 82.45 | 0.7548 | -35.0 | 44.5 | |
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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 | 0.80 | 9.53 | 52.44 | -45.91 | 82.58 | 0.7166 | -569.0 | -472.7 | |
| 0.00 | 1.49 | 0.00 | 1.06 | 9.49 | 52.19 | -46.16 | 82.66 | 0.7197 | -771.0 | -617.6 | |
| 7.17 | 9.10 | 5.11 | 6.49 | 9.96 | 52.06 | -46.29 | 82.00 | 0.7213 | -802.0 | -664.1 | |
| 2.36 | 6.04 | 1.70 | 4.35 | 9.83 | 51.51 | -46.84 | 82.20 | 0.7278 | -710.4 | -540.8 | |
| 0.00 | 1.92 | 0.00 | 1.39 | 9.42 | 51.36 | -46.99 | 82.76 | 0.7295 | -716.0 | -680.7 | |
| 1.40 | 1.57 | 1.01 | 1.14 | 10.01 | 51.16 | -47.19 | 81.95 | 0.7320 | -420.4 | -487.5 | |
| 0.00 | 1.57 | 0.00 | 1.14 | 9.43 | 51.13 | -47.22 | 82.74 | 0.7322 | -594.0 | -571.0 | |
| 0.00 | 3.67 | 0.00 | 2.68 | 9.78 | 50.89 | -47.46 | 82.28 | 0.7351 | -486.0 | -341.6 | |
| 0.00 | 1.40 | 0.00 | 1.02 | 10.04 | 50.79 | -47.56 | 81.92 | 0.7363 | 209.0 | 150.0 | |
| 6.12 | 11.29 | 4.47 | 8.24 | 9.28 | 50.71 | -47.64 | 82.96 | 0.7372 | -544.8 | -519.0 | |
| 0.00 | 1.57 | 0.00 | 1.16 | 9.71 | 50.45 | -47.90 | 82.37 | 0.7402 | 372.0 | 268.3 | |
| 7.70 | 15.57 | 5.69 | 11.50 | 8.90 | 50.09 | -48.26 | 83.47 | 0.7443 | -507.7 | -181.5 | |
| 0.00 | 1.31 | 0.00 | 0.97 | 10.09 | 49.87 | -48.48 | 81.87 | 0.7470 | 587.0 | 382.0 | |
| 7.79 | 61.77 | 5.82 | 46.31 | 9.73 | 49.48 | -48.87 | 82.36 | 0.7514 | 563.3 | 173.6 | |
| 3.32 | -14.00 | 2.50 | -14.00 | 10.23 | 49.28 | -49.07 | 81.70 | 0.7536 | -639.8 | 999999 | |
| 4.99 | -14.00 | 3.75 | -14.00 | 9.40 | 49.12 | -49.23 | 82.81 | 0.7554 | 711.7 | 999999 | |
| 0.00 | 3.06 | 0.00 | 2.32 | 10.32 | 48.94 | -49.41 | 81.59 | 0.7576 | -635.0 | -501.8 | |
| 1.66 | -14.00 | 1.25 | -14.00 | 9.81 | 49.00 | -49.35 | 82.26 | 0.7568 | -430.4 | 999999 | |
| 2.45 | -14.00 | 1.85 | -14.00 | 9.65 | 48.89 | -49.46 | 82.47 | 0.7580 | -500.4 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.60 | 9.53 | 48.53 | -49.82 | 82.63 | 0.7620 | -13.0 | -100.7 | |
| 0.00 | 1.66 | 0.00 | 1.27 | 8.72 | 48.55 | -49.80 | 83.70 | 0.7619 | -448.0 | -355.2 | |
| 0.00 | 1.66 | 0.00 | 1.28 | 9.13 | 48.00 | -50.35 | 83.16 | 0.7680 | -437.0 | -313.7 | |
| 0.00 | 0.96 | 0.00 | 0.75 | 11.01 | 47.35 | -51.00 | 80.72 | 0.7753 | 720.0 | 584.3 | |
| 0.00 | 1.49 | 0.00 | 1.17 | 11.15 | 47.17 | -51.18 | 80.55 | 0.7773 | 621.0 | 520.6 | |
| 0.00 | 1.57 | 0.00 | 1.24 | 9.65 | 47.02 | -51.33 | 82.48 | 0.7787 | 425.0 | 353.7 | |
| 0.00 | 2.45 | 0.00 | 1.93 | 9.47 | 46.96 | -51.39 | 82.72 | 0.7793 | 643.0 | 497.0 | |
| 6.91 | 15.05 | 5.51 | 11.97 | 9.45 | 46.38 | -51.97 | 82.74 | 0.7856 | 334.2 | 396.9 | |
| 0.00 | 0.61 | 0.00 | 0.49 | 10.33 | 46.13 | -52.22 | 81.61 | 0.7883 | 780.0 | 656.0 | |
| 1.05 | 1.57 | 0.85 | 1.27 | 10.38 | 45.92 | -52.43 | 81.56 | 0.7905 | 622.8 | 517.3 | |
| 0.00 | 0.87 | 0.00 | 0.71 | 10.82 | 45.76 | -52.59 | 81.00 | 0.7922 | 471.0 | 422.1 | |
| 0.00 | 1.40 | 0.00 | 1.13 | 10.19 | 45.86 | -52.49 | 81.79 | 0.7911 | 602.0 | 510.1 | |
| 0.00 | 0.44 | 0.00 | 0.35 | 10.39 | 45.71 | -52.64 | 81.54 | 0.7926 | 479.0 | 471.2 | |
| 0.00 | 1.40 | 0.00 | 1.13 | 10.57 | 45.62 | -52.73 | 81.32 | 0.7936 | 500.0 | 432.1 | |
| 0.00 | 0.87 | 0.00 | 0.71 | 10.16 | 45.51 | -52.84 | 81.83 | 0.7947 | 511.0 | 427.0 | |
| 0.00 | 0.61 | 0.00 | 0.50 | 10.46 | 45.39 | -52.96 | 81.46 | 0.7960 | 325.0 | 237.0 | |
| 0.00 | 1.05 | 0.00 | 0.90 | 10.43 | 43.31 | -55.04 | 81.50 | 0.8171 | 547.0 | 472.3 | |
| 0.00 | 1.31 | 0.00 | 1.13 | 10.57 | 43.17 | -55.18 | 81.33 | 0.8185 | 422.0 | 365.7 | |
| 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. | |