SDO HMI 2014-03-15 09:01:14 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.52 | 277.68 | 103.86 | 385.35 | 5.09 | 11.49 | 68.33 | 278.23 | 0.9366 | 97.3 | 7.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.61 | 4.17 | 1.16 | 7.94 | 4.63 | 17.38 | 74.21 | 276.77 | 0.9670 | -185.9 | -243.5 | |
| 0.00 | 2.09 | 0.00 | 4.03 | 5.06 | 17.40 | 74.24 | 277.21 | 0.9674 | -271.0 | -154.0 | |
| 5.39 | 18.26 | 8.53 | 28.82 | 6.24 | 13.84 | 70.68 | 279.02 | 0.9512 | -298.5 | -154.3 | |
| 2.87 | 251.68 | 4.16 | 342.56 | 3.09 | 12.57 | 69.41 | 275.94 | 0.9413 | 420.2 | 28.7 | |
| 14.87 | -4.00 | 21.20 | -4.00 | 3.58 | 12.14 | 68.98 | 276.53 | 0.9392 | -597.6 | 999999 | |
| 1.83 | -4.00 | 2.58 | -4.00 | 3.00 | 12.05 | 68.88 | 275.93 | 0.9381 | -348.7 | 999999 | |
| 11.56 | -4.00 | 16.21 | -4.00 | 4.99 | 11.50 | 68.34 | 278.12 | 0.9368 | -232.5 | 999999 | |
| 15.82 | -4.00 | 21.60 | -4.00 | 6.03 | 10.79 | 67.63 | 279.35 | 0.9336 | 465.9 | 999999 | |
| 1.13 | -4.00 | 1.51 | -4.00 | 5.14 | 10.41 | 67.25 | 278.48 | 0.9302 | 344.5 | 999999 | |
| 0.00 | 0.70 | 0.00 | 0.91 | 5.09 | 10.01 | 66.85 | 278.50 | 0.9277 | 462.0 | 426.5 | |
| 5.48 | -4.00 | 7.11 | -4.00 | 4.68 | 9.85 | 66.69 | 278.09 | 0.9262 | 445.4 | 999999 | |
| 12.00 | -4.00 | 15.98 | -4.00 | 6.36 | 10.17 | 67.00 | 279.81 | 0.9301 | 757.5 | 999999 | |
| 2.96 | -4.00 | 3.82 | -4.00 | 4.98 | 9.61 | 66.45 | 278.46 | 0.9249 | 712.2 | 999999 | |
| 0.00 | 0.78 | 0.00 | 1.09 | 10.88 | 10.26 | 67.10 | 284.56 | 0.9362 | -18.0 | -45.0 | |
| 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. | |