SDO HMI 2014-01-12 12:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.77 | 492.45 | 42.62 | 273.86 | -16.46 | 13.48 | -24.58 | 118.63 | 0.4561 | 973.7 | 367.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.94 | 3.23 | 0.50 | 1.74 | -14.69 | 16.88 | -21.17 | 117.97 | 0.3973 | 909.7 | 631.6 | |
| 0.00 | 1.70 | 0.00 | 0.93 | -16.11 | 16.17 | -21.89 | 120.41 | 0.4171 | -659.0 | -480.6 | |
| 43.69 | 477.64 | 24.17 | 265.37 | -16.50 | 14.15 | -23.91 | 119.28 | 0.4474 | 1348.8 | 391.7 | |
| 1.70 | -3.00 | 0.95 | -3.00 | -16.48 | 13.44 | -24.61 | 118.62 | 0.4569 | 989.2 | 999999 | |
| 7.48 | -3.00 | 4.17 | -3.00 | -16.59 | 13.12 | -24.93 | 118.56 | 0.4620 | 1115.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -15.48 | 13.07 | -24.99 | 116.27 | 0.4559 | 561.0 | 339.6 | |
| 1.45 | -3.00 | 0.81 | -3.00 | -16.71 | 12.83 | -25.22 | 118.54 | 0.4666 | 787.2 | 999999 | |
| 21.51 | -3.00 | 12.02 | -3.00 | -16.28 | 12.69 | -25.37 | 117.58 | 0.4659 | 1207.1 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.64 | -16.82 | 8.15 | -29.90 | 115.40 | 0.5304 | -742.0 | -502.8 | |
| 0.00 | 0.77 | 0.00 | 0.46 | -19.18 | 6.90 | -31.15 | 118.68 | 0.5591 | -700.0 | -607.6 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -16.22 | 6.72 | -31.33 | 113.52 | 0.5468 | -739.0 | -614.9 | |
| 0.00 | 1.28 | 0.00 | 0.76 | -17.17 | 6.33 | -31.73 | 114.95 | 0.5564 | -782.0 | -683.7 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -16.12 | 6.52 | -31.53 | 113.24 | 0.5490 | -660.0 | -497.4 | |
| 0.00 | 2.81 | 0.00 | 1.70 | -18.89 | 5.09 | -32.97 | 117.11 | 0.5807 | -781.0 | -677.7 | |
| 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. | |