SDO HMI 2014-03-15 18:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.30 | 191.01 | 65.67 | 341.76 | 5.51 | 11.28 | 73.06 | 277.86 | 0.9622 | 116.0 | 62.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 2.04 | 4.64 | 17.77 | 79.55 | 275.99 | 0.9863 | -8.0 | 6.5 | |
| 0.00 | 1.22 | 0.00 | 2.34 | 2.83 | 12.85 | 74.63 | 274.86 | 0.9677 | 274.0 | 241.6 | |
| 3.30 | 16.24 | 7.07 | 34.94 | 6.31 | 13.83 | 75.60 | 278.26 | 0.9739 | -239.3 | -38.3 | |
| 0.00 | 5.56 | 0.00 | 10.76 | 3.12 | 12.80 | 74.57 | 275.17 | 0.9676 | 260.0 | 195.0 | |
| 6.69 | 15.98 | 12.75 | 30.22 | 3.67 | 12.58 | 74.36 | 275.77 | 0.9670 | -410.5 | -395.2 | |
| 0.00 | 1.04 | 0.00 | 1.97 | 3.17 | 12.47 | 74.24 | 275.27 | 0.9662 | -204.0 | -200.9 | |
| 0.00 | 9.12 | 0.00 | 16.49 | 3.12 | 11.80 | 73.58 | 275.32 | 0.9631 | -605.0 | -465.9 | |
| 0.00 | 5.65 | 0.00 | 10.63 | 4.82 | 12.12 | 73.89 | 277.02 | 0.9657 | -263.0 | -343.7 | |
| 0.00 | 0.87 | 0.00 | 1.57 | 3.53 | 11.67 | 73.45 | 275.76 | 0.9628 | -549.0 | -531.5 | |
| 5.21 | 9.47 | 9.51 | 17.17 | 5.15 | 11.57 | 73.34 | 277.44 | 0.9635 | -39.9 | -267.0 | |
| 0.00 | 0.78 | 0.00 | 1.50 | 6.84 | 12.19 | 73.97 | 279.07 | 0.9675 | -66.0 | -124.0 | |
| 9.90 | 103.80 | 17.36 | 177.68 | 6.00 | 10.81 | 72.58 | 278.44 | 0.9606 | 356.2 | 286.7 | |
| 9.29 | -12.00 | 15.89 | -12.00 | 6.39 | 10.24 | 72.02 | 278.94 | 0.9582 | 616.3 | 999999 | |
| 1.91 | 17.81 | 3.09 | 29.52 | 4.55 | 9.60 | 71.37 | 277.14 | 0.9534 | 512.9 | -90.0 | |
| 0.00 | 2.78 | 0.00 | 4.93 | 10.89 | 10.12 | 71.90 | 283.58 | 0.9615 | -430.0 | -333.0 | |
| 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. | |