SDO HMI 2014-05-28 06:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.82 | 34.28 | 8.27 | 21.38 | -10.49 | 83.64 | 36.20 | 253.78 | 0.6059 | 272.2 | 89.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.82 | 16.52 | 8.27 | 10.65 | -9.76 | 86.52 | 39.08 | 256.05 | 0.6424 | 853.1 | 512.6 | |
| 0.00 | 0.81 | 0.00 | 0.51 | -9.93 | 84.89 | 37.45 | 255.32 | 0.6214 | 679.0 | 557.7 | |
| 0.00 | 1.44 | 0.00 | 0.91 | -10.98 | 84.49 | 37.05 | 253.52 | 0.6191 | 663.0 | 505.8 | |
| 0.00 | 1.08 | 0.00 | 0.68 | -10.12 | 84.33 | 36.89 | 254.84 | 0.6145 | 678.0 | 624.3 | |
| 0.00 | 2.80 | 0.00 | 1.74 | -11.98 | 83.36 | 35.93 | 251.51 | 0.6074 | 687.0 | 458.5 | |
| 0.00 | 2.08 | 0.00 | 1.27 | -12.24 | 81.95 | 34.52 | 250.50 | 0.5897 | 633.0 | 544.3 | |
| 0.00 | 2.17 | 0.00 | 1.30 | -10.25 | 80.60 | 33.17 | 253.29 | 0.5642 | -458.0 | -422.2 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -10.07 | 80.51 | 33.07 | 253.57 | 0.5623 | -598.0 | -468.9 | |
| 0.00 | 1.26 | 0.00 | 0.76 | -10.41 | 80.40 | 32.96 | 252.94 | 0.5620 | -619.0 | -561.0 | |
| 0.00 | 1.26 | 0.00 | 0.76 | -11.89 | 80.04 | 32.60 | 250.21 | 0.5624 | -464.0 | -448.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -9.83 | 79.78 | 32.35 | 253.70 | 0.5514 | -506.0 | -478.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -11.06 | 76.18 | 28.74 | 249.68 | 0.5053 | -679.0 | -512.0 | |
| 0.00 | 1.44 | 0.00 | 0.82 | -14.12 | 74.00 | 26.56 | 242.40 | 0.4913 | -773.0 | -637.4 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -9.45 | 72.70 | 25.26 | 250.80 | 0.4476 | -508.0 | -302.2 | |
| 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. | |