SDO HMI 2014-09-08 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.95 | 167.15 | 34.45 | 164.83 | -16.42 | 64.55 | -55.56 | 113.84 | 0.8658 | 203.8 | 23.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.65 | 112.42 | 21.18 | 105.24 | -16.34 | 66.50 | -53.61 | 114.43 | 0.8505 | 686.9 | 168.0 | |
| 1.69 | -1.00 | 1.61 | -1.00 | -16.80 | 66.15 | -53.96 | 114.80 | 0.8548 | -366.7 | 999999 | |
| 0.00 | 0.98 | 0.00 | 0.95 | -16.47 | 65.31 | -54.80 | 114.12 | 0.8606 | 314.0 | 226.5 | |
| 0.00 | 1.52 | 0.00 | 1.43 | -14.94 | 65.70 | -54.40 | 112.57 | 0.8529 | -346.0 | -335.2 | |
| 0.00 | 0.80 | 0.00 | 0.79 | -16.67 | 64.67 | -55.44 | 114.11 | 0.8663 | 326.0 | 319.3 | |
| 1.07 | 3.03 | 1.05 | 2.96 | -16.20 | 64.76 | -55.35 | 113.63 | 0.8642 | 291.2 | 242.6 | |
| 0.00 | 1.96 | 0.00 | 1.96 | -16.63 | 64.12 | -55.98 | 113.87 | 0.8705 | 390.0 | 155.7 | |
| 0.00 | 4.10 | 0.00 | 4.42 | -16.49 | 61.48 | -58.62 | 112.83 | 0.8901 | -655.0 | -479.3 | |
| 4.19 | 40.74 | 4.65 | 45.25 | -16.62 | 60.61 | -59.49 | 112.69 | 0.8966 | -562.2 | -256.4 | |
| 2.67 | -9.00 | 2.95 | -9.00 | -16.29 | 60.65 | -59.45 | 112.35 | 0.8956 | -636.9 | 999999 | |
| 0.00 | 1.60 | 0.00 | 1.83 | -17.34 | 60.04 | -60.06 | 113.27 | 0.9022 | -324.0 | -328.3 | |
| 2.41 | -9.00 | 2.71 | -9.00 | -16.67 | 60.21 | -59.89 | 112.61 | 0.8995 | -207.3 | 999999 | |
| 0.27 | -9.00 | 0.30 | -9.00 | -16.43 | 60.34 | -59.77 | 112.39 | 0.8981 | -357.3 | 999999 | |
| 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. | |