SDO HMI 2014-04-11 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.12 | 302.33 | 70.11 | 290.07 | 4.58 | 242.99 | -58.00 | 81.00 | 0.8570 | -222.9 | -132.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.71 | 0.00 | 0.62 | 8.35 | 246.96 | -54.02 | 75.71 | 0.8284 | 239.0 | 287.0 | |
| 39.17 | 230.69 | 35.94 | 212.45 | 4.72 | 244.57 | -56.42 | 80.54 | 0.8438 | -951.4 | -253.1 | |
| 2.65 | -2.00 | 2.44 | -2.00 | 3.83 | 244.28 | -56.70 | 81.64 | 0.8450 | -526.6 | 999999 | |
| 2.21 | -2.00 | 2.11 | -2.00 | 5.63 | 243.27 | -57.72 | 79.76 | 0.8570 | -393.3 | 999999 | |
| 0.00 | 1.15 | 0.00 | 1.10 | 5.99 | 243.04 | -57.95 | 79.40 | 0.8596 | -334.0 | -263.1 | |
| 0.00 | 1.24 | 0.00 | 1.20 | 3.47 | 242.16 | -58.83 | 82.45 | 0.8635 | 196.0 | 157.6 | |
| 0.00 | 0.97 | 0.00 | 0.96 | 4.52 | 241.74 | -59.24 | 81.34 | 0.8686 | 532.0 | 513.6 | |
| 0.00 | 0.26 | 0.00 | 0.26 | 4.24 | 241.78 | -59.21 | 81.65 | 0.8679 | 372.0 | 309.7 | |
| 3.88 | 9.53 | 3.86 | 9.47 | 3.29 | 241.52 | -59.46 | 82.78 | 0.8687 | 681.1 | 517.2 | |
| 0.00 | 2.38 | 0.00 | 2.47 | 5.31 | 240.41 | -60.57 | 80.69 | 0.8808 | 603.0 | 466.7 | |
| 0.00 | 0.71 | 0.00 | 0.76 | 4.73 | 239.11 | -61.87 | 81.58 | 0.8904 | 446.0 | 356.2 | |
| 19.50 | 43.31 | 21.48 | 47.63 | 4.09 | 238.42 | -62.56 | 82.41 | 0.8950 | 578.7 | 260.0 | |
| 0.00 | 0.26 | 0.00 | 0.30 | 5.33 | 237.55 | -63.43 | 81.19 | 0.9030 | 118.0 | 166.7 | |
| 3.71 | 11.12 | 4.28 | 12.85 | 4.72 | 237.18 | -63.81 | 81.92 | 0.9050 | 389.2 | 289.7 | |
| 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. | |