SDO HMI 2014-03-22 19:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.65 | 272.25 | 44.32 | 268.35 | 11.91 | 262.48 | 57.09 | 288.19 | 0.8660 | -539.9 | -241.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.52 | 0.00 | 0.63 | 12.83 | 268.32 | 62.92 | 287.53 | 0.9122 | -240.0 | -232.5 | |
| 0.00 | 1.13 | 0.00 | 1.34 | 13.00 | 267.92 | 62.53 | 287.82 | 0.9098 | -206.0 | -225.4 | |
| 0.00 | 0.61 | 0.00 | 0.67 | 13.18 | 265.55 | 60.16 | 288.66 | 0.8933 | 357.0 | 289.9 | |
| 0.00 | 0.61 | 0.00 | 0.67 | 13.55 | 265.45 | 60.06 | 289.08 | 0.8933 | 432.0 | 378.0 | |
| 44.65 | 260.40 | 44.32 | 258.15 | 11.85 | 262.73 | 57.34 | 288.01 | 0.8684 | -808.0 | -264.9 | |
| 0.00 | 1.40 | 0.00 | 1.41 | 15.75 | 262.30 | 56.91 | 292.45 | 0.8744 | -230.0 | -190.3 | |
| 0.00 | 0.78 | 0.00 | 0.58 | 12.74 | 249.49 | 44.10 | 294.11 | 0.7460 | 371.0 | 341.6 | |
| 0.00 | 0.52 | 0.00 | 0.38 | 11.53 | 248.94 | 43.55 | 292.85 | 0.7349 | 580.0 | 514.2 | |
| 0.00 | 1.40 | 0.00 | 1.03 | 12.96 | 249.07 | 43.68 | 294.59 | 0.7425 | 610.0 | 547.3 | |
| 0.00 | 0.87 | 0.00 | 0.64 | 13.06 | 248.80 | 43.41 | 294.86 | 0.7401 | 592.0 | 506.5 | |
| 0.00 | 0.96 | 0.00 | 0.69 | 11.77 | 248.49 | 43.09 | 293.38 | 0.7310 | 689.0 | 542.9 | |
| 0.00 | 0.96 | 0.00 | 0.70 | 13.08 | 248.30 | 42.91 | 295.14 | 0.7348 | 580.0 | 476.1 | |
| 0.00 | 1.13 | 0.00 | 0.82 | 12.94 | 247.81 | 42.42 | 295.22 | 0.7290 | 762.0 | 691.0 | |
| 0.00 | 0.96 | 0.00 | 0.64 | 15.76 | 241.53 | 36.14 | 302.66 | 0.6765 | 568.0 | 478.6 | |
| 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. | |