SDO HMI 2014-11-13 11:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.34 | 193.06 | 61.09 | 514.74 | -12.49 | 253.52 | -78.05 | 103.42 | 0.9791 | 293.8 | -12.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.65 | -16.89 | 281.00 | -50.57 | 113.57 | 0.8086 | 114.0 | 216.0 | |
| 0.00 | 0.52 | 0.00 | 0.42 | -5.76 | 279.44 | -52.13 | 99.58 | 0.7988 | 406.0 | 369.5 | |
| 0.60 | 1.46 | 0.55 | 1.33 | -6.63 | 275.24 | -56.33 | 99.92 | 0.8413 | 256.4 | 296.9 | |
| 0.00 | 0.52 | 0.00 | 0.56 | -13.14 | 270.47 | -61.10 | 106.46 | 0.8909 | 284.0 | 347.0 | |
| 0.00 | 0.95 | 0.00 | 0.99 | -9.48 | 270.86 | -60.70 | 102.47 | 0.8829 | 372.0 | 335.0 | |
| 0.00 | 0.95 | 0.00 | 1.30 | -16.65 | 264.62 | -66.94 | 109.14 | 0.9347 | 132.0 | 211.3 | |
| 0.00 | 0.77 | 0.00 | 0.97 | -11.69 | 266.13 | -65.44 | 104.11 | 0.9201 | 377.0 | 338.1 | |
| 0.00 | 0.60 | 0.00 | 0.70 | -6.38 | 267.53 | -64.04 | 98.54 | 0.9053 | 227.0 | 240.0 | |
| 8.26 | 58.18 | 12.88 | 91.65 | -14.04 | 261.54 | -70.03 | 105.91 | 0.9495 | 443.4 | 45.1 | |
| 1.64 | -9.00 | 2.61 | -9.00 | -13.78 | 261.08 | -70.49 | 105.57 | 0.9517 | 139.5 | 999999 | |
| 15.84 | 124.20 | 45.05 | 361.69 | -12.17 | 252.55 | -79.02 | 102.94 | 0.9854 | 289.5 | -7.0 | |
| 0.00 | 0.52 | 0.00 | 1.23 | -9.16 | 254.28 | -77.29 | 100.04 | 0.9790 | 22.0 | -34.8 | |
| 0.00 | 0.95 | 0.00 | 16.89 | -14.46 | 243.77 | -87.80 | 104.56 | 0.9998 | -133.0 | -175.6 | |
| 0.00 | 2.67 | 0.00 | 36.36 | -11.30 | 244.35 | -87.22 | 101.44 | 0.9995 | -174.0 | -155.2 | |
| 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. | |