SDO HMI 2014-05-16 17:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.05 | 31.09 | 10.33 | 28.29 | -18.31 | 144.22 | -55.93 | 110.32 | 0.8396 | 304.7 | 100.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.66 | -17.01 | 154.24 | -45.90 | 110.98 | 0.7377 | -581.0 | -437.4 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -17.95 | 153.80 | -46.35 | 112.08 | 0.7451 | -669.0 | -549.5 | |
| 0.00 | 0.72 | 0.00 | 0.53 | -17.66 | 153.75 | -46.39 | 111.69 | 0.7448 | -489.0 | -410.2 | |
| 0.00 | 0.45 | 0.00 | 0.39 | -20.74 | 146.48 | -53.66 | 113.63 | 0.8244 | 501.0 | 482.4 | |
| 0.00 | 0.90 | 0.00 | 0.78 | -18.64 | 146.04 | -54.11 | 111.03 | 0.8245 | 564.0 | 527.5 | |
| 0.00 | 0.54 | 0.00 | 0.47 | -18.35 | 145.79 | -54.35 | 110.63 | 0.8263 | 427.0 | 430.0 | |
| 0.00 | 0.54 | 0.00 | 0.47 | -18.50 | 145.55 | -54.59 | 110.76 | 0.8287 | 479.0 | 468.2 | |
| 0.00 | 1.08 | 0.00 | 0.96 | -19.16 | 145.23 | -54.91 | 111.48 | 0.8327 | 538.0 | 478.8 | |
| 0.00 | 0.72 | 0.00 | 0.65 | -19.08 | 144.82 | -55.32 | 111.30 | 0.8363 | 316.0 | 308.9 | |
| 0.00 | 0.63 | 0.00 | 0.58 | -20.17 | 144.18 | -55.96 | 112.46 | 0.8438 | 263.0 | 254.1 | |
| 0.00 | 1.53 | 0.00 | 1.38 | -18.56 | 144.57 | -55.57 | 110.64 | 0.8377 | 228.0 | 239.8 | |
| 11.05 | 17.15 | 10.33 | 16.07 | -18.22 | 143.06 | -57.09 | 109.97 | 0.8505 | 565.3 | 173.1 | |
| 0.00 | 4.04 | 0.00 | 3.81 | -17.99 | 142.76 | -57.38 | 109.65 | 0.8527 | -51.0 | -56.2 | |
| 0.00 | 0.72 | 0.00 | 0.68 | -18.39 | 142.43 | -57.71 | 110.06 | 0.8561 | -257.0 | -217.8 | |
| 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. | |