SDO HMI 2014-01-12 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.05 | 93.61 | 36.88 | 134.88 | 8.45 | 102.95 | 68.75 | 280.73 | 0.9369 | 228.3 | 129.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 2.66 | 6.21 | 110.83 | 76.63 | 277.37 | 0.9763 | -112.0 | -90.1 | |
| 0.68 | 13.08 | 1.50 | 29.22 | 6.47 | 110.69 | 76.49 | 277.65 | 0.9758 | -326.2 | 45.7 | |
| 3.65 | -2.00 | 8.08 | -2.00 | 6.88 | 110.64 | 76.44 | 278.07 | 0.9758 | 127.8 | 999999 | |
| 0.00 | 0.51 | 0.00 | 1.00 | 5.56 | 108.97 | 74.77 | 276.90 | 0.9685 | -175.0 | -143.2 | |
| 3.23 | 4.76 | 5.31 | 7.82 | 6.96 | 105.93 | 71.73 | 278.69 | 0.9549 | -285.3 | -225.1 | |
| 0.00 | 1.53 | 0.00 | 2.29 | 6.65 | 104.17 | 69.97 | 278.59 | 0.9453 | -426.0 | -364.5 | |
| 0.93 | 1.61 | 1.37 | 2.37 | 8.44 | 103.52 | 69.32 | 280.56 | 0.9429 | 141.3 | 156.0 | |
| 0.42 | 1.36 | 0.54 | 1.72 | 8.23 | 100.12 | 65.92 | 280.84 | 0.9217 | 494.0 | 457.7 | |
| 1.36 | 5.52 | 1.70 | 6.94 | 7.91 | 99.94 | 65.74 | 280.53 | 0.9202 | 61.6 | 242.1 | |
| 1.27 | 56.66 | 1.64 | 71.99 | 9.51 | 100.43 | 66.23 | 282.17 | 0.9250 | 238.5 | 172.0 | |
| 4.59 | -10.00 | 5.83 | -10.00 | 9.31 | 100.05 | 65.85 | 282.01 | 0.9223 | 462.0 | 999999 | |
| 2.72 | -10.00 | 3.40 | -10.00 | 9.43 | 99.66 | 65.46 | 282.21 | 0.9199 | 711.6 | 999999 | |
| 1.10 | -10.00 | 1.38 | -10.00 | 9.64 | 99.67 | 65.47 | 282.43 | 0.9201 | 609.4 | 999999 | |
| 5.10 | 6.63 | 6.13 | 7.96 | 9.30 | 98.69 | 64.49 | 282.23 | 0.9131 | 571.7 | 455.7 | |
| 0.00 | 0.76 | 0.00 | 0.91 | 9.52 | 98.34 | 64.15 | 282.53 | 0.9109 | 604.0 | 549.3 | |
| 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. | |