SDO HMI 2014-10-01 06:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.32 | 219.98 | 49.87 | 511.29 | 15.40 | 260.18 | 78.74 | 284.36 | 0.9759 | 57.6 | -105.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.08 | 0.00 | 13.72 | 12.59 | 266.31 | 84.88 | 281.98 | 0.9942 | 65.0 | 72.5 | |
| 0.00 | 0.88 | 0.00 | 3.46 | 13.08 | 265.52 | 84.09 | 282.40 | 0.9926 | -215.0 | -195.1 | |
| 0.00 | 3.35 | 0.00 | 13.08 | 13.54 | 265.35 | 83.92 | 282.85 | 0.9922 | -64.0 | 68.5 | |
| 0.00 | 3.00 | 0.00 | 11.67 | 13.94 | 265.40 | 83.97 | 283.25 | 0.9922 | 83.0 | 126.0 | |
| 0.00 | 2.64 | 0.00 | 8.64 | 13.77 | 263.93 | 82.50 | 282.95 | 0.9888 | -196.0 | -68.3 | |
| 0.00 | 2.20 | 0.00 | 7.52 | 14.17 | 264.49 | 83.06 | 283.41 | 0.9901 | 206.0 | 158.4 | |
| 5.46 | 108.76 | 14.09 | 276.14 | 15.03 | 261.65 | 80.22 | 284.06 | 0.9820 | -366.7 | -233.7 | |
| 2.91 | -7.00 | 6.59 | -7.00 | 15.17 | 260.12 | 78.68 | 284.10 | 0.9768 | -464.5 | 999999 | |
| 0.00 | 3.08 | 0.00 | 5.82 | 14.60 | 257.40 | 75.97 | 283.36 | 0.9661 | 474.0 | 336.3 | |
| 0.00 | 3.61 | 0.00 | 6.93 | 15.67 | 257.66 | 76.23 | 284.47 | 0.9670 | 395.0 | 231.4 | |
| 1.41 | 68.93 | 2.66 | 127.07 | 15.97 | 257.49 | 76.05 | 284.78 | 0.9662 | 172.0 | 60.4 | |
| 13.04 | -11.00 | 23.83 | -11.00 | 16.50 | 256.94 | 75.51 | 285.30 | 0.9636 | 384.0 | 999999 | |
| 0.97 | 17.63 | 1.74 | 32.35 | 17.18 | 256.73 | 75.30 | 286.00 | 0.9626 | 303.8 | -139.5 | |
| 0.53 | -13.00 | 0.96 | -13.00 | 17.33 | 256.79 | 75.36 | 286.16 | 0.9628 | 211.2 | 999999 | |
| 0.00 | 2.82 | 0.00 | 4.89 | 17.45 | 256.06 | 74.63 | 286.25 | 0.9594 | 532.0 | 434.1 | |
| 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. | |