SDO HMI 2011-11-07 13:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.88 | 262.98 | 51.20 | 255.72 | 9.55 | 55.53 | -59.39 | 81.10 | 0.8598 | -400.4 | -217.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.27 | 219.68 | 23.48 | 206.23 | 9.27 | 56.98 | -57.94 | 81.39 | 0.8480 | -811.2 | -206.6 | |
| 0.00 | 0.86 | 0.00 | 0.81 | 10.69 | 56.57 | -58.34 | 79.73 | 0.8521 | -298.0 | -326.3 | |
| 4.74 | 6.12 | 4.56 | 5.88 | 12.04 | 55.89 | -59.03 | 78.19 | 0.8588 | 418.7 | 108.9 | |
| 0.00 | 2.67 | 0.00 | 2.59 | 11.75 | 55.63 | -59.28 | 78.53 | 0.8609 | -360.0 | -252.1 | |
| 4.57 | -1.00 | 4.33 | -1.00 | 9.35 | 56.26 | -58.65 | 81.32 | 0.8545 | -325.9 | 999999 | |
| 3.28 | -1.00 | 3.12 | -1.00 | 9.67 | 56.11 | -58.80 | 80.95 | 0.8559 | -343.1 | 999999 | |
| 1.64 | -1.00 | 1.56 | -1.00 | 8.59 | 56.17 | -58.74 | 82.21 | 0.8552 | -272.1 | 999999 | |
| 1.98 | 2.67 | 1.94 | 2.61 | 11.13 | 55.24 | -59.67 | 79.28 | 0.8640 | -606.3 | -554.4 | |
| 0.00 | 1.04 | 0.00 | 0.99 | 8.27 | 55.72 | -59.19 | 82.59 | 0.8592 | -194.0 | -135.7 | |
| 5.00 | 21.74 | 5.75 | 24.95 | 9.48 | 50.19 | -64.72 | 81.27 | 0.9041 | -582.0 | -397.7 | |
| 0.00 | 0.60 | 0.00 | 0.70 | 10.04 | 49.92 | -65.00 | 80.65 | 0.9062 | -141.0 | -194.9 | |
| 0.00 | 0.78 | 0.00 | 1.02 | 11.28 | 46.76 | -68.15 | 79.34 | 0.9279 | -150.0 | -163.4 | |
| 0.00 | 1.04 | 0.00 | 1.44 | 12.41 | 45.37 | -69.54 | 78.14 | 0.9366 | 374.0 | 261.9 | |
| 4.40 | 5.78 | 6.46 | 8.50 | 12.73 | 44.26 | -70.65 | 77.80 | 0.9431 | 376.6 | 121.4 | |
| 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. | |