SDO HMI 2014-09-16 19:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.01 | 28.83 | 6.36 | 26.06 | -15.96 | 64.61 | 52.35 | 245.54 | 0.8384 | 301.6 | 110.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.95 | 0.00 | 1.75 | -13.96 | 65.09 | 52.83 | 247.99 | 0.8363 | 91.0 | 147.5 | |
| 0.00 | 0.98 | 0.00 | 0.90 | -15.64 | 65.48 | 53.21 | 246.24 | 0.8448 | 395.0 | 343.5 | |
| 0.00 | 0.62 | 0.00 | 0.55 | -14.08 | 64.77 | 52.51 | 247.72 | 0.8338 | 527.0 | 448.3 | |
| 3.55 | 6.30 | 3.26 | 5.79 | -15.88 | 65.36 | 53.10 | 245.92 | 0.8445 | 545.0 | 423.7 | |
| 0.00 | 1.15 | 0.00 | 1.05 | -15.51 | 65.22 | 52.96 | 246.28 | 0.8422 | 417.0 | 318.4 | |
| 0.00 | 1.15 | 0.00 | 1.04 | -14.95 | 64.76 | 52.50 | 246.74 | 0.8364 | 659.0 | 513.7 | |
| 0.53 | 1.51 | 0.48 | 1.36 | -15.31 | 64.84 | 52.57 | 246.36 | 0.8382 | 717.8 | 597.9 | |
| 0.00 | 0.44 | 0.00 | 0.41 | -16.02 | 65.10 | 52.83 | 245.67 | 0.8427 | 406.0 | 423.6 | |
| 0.00 | 0.44 | 0.00 | 0.40 | -14.57 | 64.53 | 52.26 | 247.08 | 0.8332 | 724.0 | 748.6 | |
| 0.00 | 0.89 | 0.00 | 0.79 | -14.73 | 64.48 | 52.21 | 246.88 | 0.8332 | 729.0 | 581.3 | |
| 0.00 | 2.66 | 0.00 | 2.41 | -15.85 | 64.77 | 52.51 | 245.73 | 0.8394 | 295.0 | 297.4 | |
| 2.31 | 7.28 | 2.06 | 6.51 | -16.89 | 63.83 | 51.57 | 244.18 | 0.8348 | -591.8 | -442.2 | |
| 0.62 | 2.75 | 0.56 | 2.48 | -17.33 | 64.00 | 51.74 | 243.76 | 0.8378 | -518.6 | -305.7 | |
| 0.00 | 0.71 | 0.00 | 0.62 | -15.97 | 63.04 | 50.77 | 244.90 | 0.8246 | -336.0 | -327.0 | |
| 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. | |