SDO HMI 2014-10-11 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.98 | 115.40 | 38.78 | 230.79 | -15.12 | 123.24 | 73.21 | 252.60 | 0.9689 | 133.4 | 62.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.96 | 80.27 | 2.17 | 173.76 | -14.40 | 125.21 | 75.17 | 253.70 | 0.9765 | -1.1 | 95.0 | |
| 5.87 | -1.00 | 13.00 | -1.00 | -15.12 | 124.83 | 74.79 | 252.91 | 0.9756 | 93.6 | 999999 | |
| 0.26 | -1.00 | 0.58 | -1.00 | -15.49 | 124.72 | 74.68 | 252.52 | 0.9755 | 270.0 | 999999 | |
| 3.07 | -1.00 | 6.41 | -1.00 | -14.87 | 124.00 | 73.96 | 253.01 | 0.9724 | 510.7 | 999999 | |
| 1.93 | -1.00 | 3.84 | -1.00 | -14.41 | 123.47 | 73.43 | 253.39 | 0.9699 | 620.9 | 999999 | |
| 0.00 | 2.80 | 0.00 | 5.48 | -15.11 | 123.00 | 72.97 | 252.58 | 0.9685 | 515.0 | 377.9 | |
| 1.23 | 2.54 | 2.32 | 4.81 | -15.12 | 122.48 | 72.44 | 252.48 | 0.9663 | 512.6 | 445.8 | |
| 0.00 | 0.26 | 0.00 | 0.48 | -15.19 | 121.92 | 71.88 | 252.30 | 0.9640 | 495.0 | 415.7 | |
| 0.44 | 1.40 | 0.72 | 2.31 | -14.61 | 120.02 | 69.99 | 252.52 | 0.9546 | -117.4 | -46.2 | |
| 0.00 | 0.96 | 0.00 | 1.54 | -14.80 | 119.44 | 69.40 | 252.20 | 0.9518 | -79.0 | -112.0 | |
| 3.77 | 14.55 | 6.03 | 23.37 | -15.37 | 119.40 | 69.36 | 251.61 | 0.9523 | -204.6 | 16.1 | |
| 0.00 | 1.58 | 0.00 | 2.47 | -15.48 | 118.95 | 68.91 | 251.40 | 0.9501 | -450.0 | -420.1 | |
| 0.79 | 1.93 | 1.21 | 2.96 | -17.03 | 118.21 | 68.17 | 249.65 | 0.9481 | -297.6 | -119.1 | |
| 1.66 | 9.11 | 2.50 | 13.61 | -17.10 | 117.67 | 67.64 | 249.45 | 0.9454 | -525.4 | -385.4 | |
| 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. | |