SDO HMI 2014-08-06 20:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.34 | 115.17 | 57.61 | 138.24 | 11.33 | 127.22 | -66.19 | 80.31 | 0.9113 | 15.7 | -3.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.90 | 63.15 | 2.09 | 71.25 | 12.33 | 129.46 | -63.95 | 79.27 | 0.8951 | -672.3 | -167.9 | |
| 7.59 | -1.00 | 8.43 | -1.00 | 12.50 | 129.24 | -64.17 | 79.08 | 0.8968 | -719.0 | 999999 | |
| 1.36 | -1.00 | 1.51 | -1.00 | 11.96 | 129.12 | -64.29 | 79.68 | 0.8977 | -467.1 | 999999 | |
| 7.86 | -1.00 | 8.91 | -1.00 | 12.54 | 128.64 | -64.77 | 79.03 | 0.9012 | -495.3 | 999999 | |
| 4.70 | -1.00 | 5.35 | -1.00 | 12.15 | 128.52 | -64.88 | 79.46 | 0.9022 | -230.1 | 999999 | |
| 0.00 | 1.26 | 0.00 | 1.44 | 10.18 | 128.62 | -64.79 | 81.65 | 0.9019 | 483.0 | 477.7 | |
| 0.00 | 0.72 | 0.00 | 0.83 | 11.13 | 128.16 | -65.25 | 80.59 | 0.9050 | -242.0 | -184.4 | |
| 0.00 | 1.17 | 0.00 | 1.41 | 11.88 | 126.97 | -66.43 | 79.72 | 0.9133 | 290.0 | 246.5 | |
| 1.26 | 2.89 | 1.49 | 3.40 | 9.66 | 127.69 | -65.71 | 82.19 | 0.9087 | 532.2 | 446.4 | |
| 0.00 | 0.99 | 0.00 | 1.18 | 9.72 | 127.37 | -66.04 | 82.11 | 0.9111 | 369.0 | 289.0 | |
| 0.36 | 1.54 | 0.45 | 1.92 | 11.52 | 126.11 | -67.29 | 80.09 | 0.9193 | -143.8 | -127.2 | |
| 0.00 | 1.81 | 0.00 | 2.23 | 10.59 | 126.46 | -66.95 | 81.12 | 0.9171 | 418.0 | 409.5 | |
| 0.00 | 1.17 | 0.00 | 1.44 | 9.80 | 126.63 | -66.77 | 81.98 | 0.9162 | 575.0 | 553.5 | |
| 0.54 | 5.06 | 0.68 | 6.33 | 9.68 | 126.04 | -67.37 | 82.08 | 0.9202 | 494.7 | 428.0 | |
| 1.81 | 35.41 | 2.31 | 46.81 | 9.91 | 125.53 | -67.87 | 81.81 | 0.9235 | 427.5 | 68.7 | |
| 1.08 | -15.00 | 1.40 | -15.00 | 10.13 | 125.27 | -68.14 | 81.56 | 0.9252 | 511.1 | 999999 | |
| 18.88 | -15.00 | 24.99 | -15.00 | 10.20 | 124.73 | -68.68 | 81.46 | 0.9287 | 412.6 | 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. | |