SDO HMI 2014-03-29 15:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.23 | 29.60 | 0.66 | 16.29 | 3.95 | 138.77 | 23.49 | 293.74 | 0.4361 | -18.0 | 199.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.64 | 3.48 | 142.04 | 26.76 | 290.01 | 0.4803 | -783.0 | -645.5 | |
| 0.00 | 2.01 | 0.00 | 1.14 | 4.81 | 142.03 | 26.74 | 292.60 | 0.4877 | -964.0 | -797.0 | |
| 0.00 | 0.96 | 0.00 | 0.54 | 4.32 | 141.91 | 26.62 | 291.76 | 0.4831 | -673.0 | -465.2 | |
| 0.00 | 1.31 | 0.00 | 0.74 | 5.17 | 141.88 | 26.59 | 293.40 | 0.4878 | -789.0 | -602.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | 2.68 | 141.38 | 26.10 | 288.92 | 0.4665 | -787.0 | -648.9 | |
| 0.00 | 1.93 | 0.00 | 1.08 | 4.70 | 141.05 | 25.77 | 293.20 | 0.4733 | -746.0 | -666.5 | |
| 0.00 | 1.31 | 0.00 | 0.74 | 7.00 | 140.37 | 25.08 | 298.17 | 0.4793 | -676.0 | -515.9 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 6.77 | 140.15 | 24.87 | 297.96 | 0.4748 | -657.0 | -561.0 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 2.90 | 138.39 | 23.10 | 291.83 | 0.4239 | 800.0 | 579.3 | |
| 0.00 | 4.03 | 0.00 | 2.20 | 4.50 | 137.39 | 22.11 | 296.27 | 0.4202 | 475.0 | 576.0 | |
| 1.23 | 4.82 | 0.66 | 2.61 | 2.52 | 137.21 | 21.93 | 292.07 | 0.4043 | 1044.4 | 733.8 | |
| 0.00 | 1.93 | 0.00 | 1.05 | 4.25 | 137.22 | 21.94 | 295.91 | 0.4160 | 974.0 | 837.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 4.07 | 137.22 | 21.93 | 295.52 | 0.4146 | 802.0 | 669.8 | |
| 0.00 | 3.07 | 0.00 | 1.66 | 2.75 | 137.02 | 21.74 | 292.79 | 0.4030 | 1114.0 | 859.0 | |
| 0.00 | 3.15 | 0.00 | 1.71 | 3.69 | 137.01 | 21.73 | 294.91 | 0.4091 | 957.0 | 718.5 | |
| 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. | |