SDO HMI 2014-07-03 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 31.24 | 0.00 | 16.42 | 5.84 | 266.62 | -17.17 | 80.26 | 0.3006 | 156.7 | 165.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.72 | 3.30 | 279.92 | -3.87 | 87.54 | 0.0678 | -866.0 | -592.3 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 7.11 | 279.84 | -3.95 | 44.62 | 0.0979 | -854.0 | -697.4 | |
| 0.00 | 2.45 | 0.00 | 1.22 | 3.57 | 278.84 | -4.95 | 84.89 | 0.0868 | -1045.0 | -819.5 | |
| 0.00 | 1.91 | 0.00 | 0.95 | 4.04 | 275.95 | -7.84 | 83.18 | 0.1376 | -902.0 | -625.7 | |
| 0.00 | 4.81 | 0.00 | 2.42 | 1.50 | 273.99 | -9.80 | 99.29 | 0.1732 | -843.0 | -646.8 | |
| 0.00 | 3.27 | 0.00 | 1.68 | 9.30 | 269.39 | -14.40 | 66.07 | 0.2697 | 737.0 | 754.3 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 11.89 | 265.92 | -17.87 | 62.73 | 0.3392 | 737.0 | 606.2 | |
| 0.00 | 3.27 | 0.00 | 1.76 | 8.74 | 261.18 | -22.62 | 75.02 | 0.3951 | 901.0 | 715.4 | |
| 0.00 | 2.45 | 0.00 | 1.33 | 8.91 | 260.76 | -23.03 | 74.82 | 0.4021 | 531.0 | 524.4 | |
| 0.00 | 1.73 | 0.00 | 0.93 | 9.06 | 260.55 | -23.24 | 74.57 | 0.4059 | 706.0 | 660.1 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -1.14 | 258.84 | -24.95 | 99.36 | 0.4293 | 755.0 | 596.5 | |
| 0.00 | 2.00 | 0.00 | 1.10 | 7.72 | 258.00 | -25.79 | 78.82 | 0.4414 | 873.0 | 744.8 | |
| 0.00 | 2.36 | 0.00 | 1.33 | 5.13 | 255.66 | -28.13 | 84.99 | 0.4733 | 872.0 | 707.6 | |
| 0.00 | 1.82 | 0.00 | 1.05 | 3.00 | 252.47 | -31.32 | 89.38 | 0.5212 | 592.0 | 565.8 | |
| 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. | |