SDO HMI 2013-03-28 18:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.18 | 243.83 | 22.75 | 131.62 | 15.00 | 255.32 | -8.52 | 21.21 | 0.3972 | -995.8 | -372.2 | |
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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 | 0.59 | 10.33 | 258.96 | -4.89 | 15.98 | 0.3057 | -858.0 | -670.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 13.38 | 255.78 | -8.06 | 21.74 | 0.3701 | -962.0 | -855.8 | |
| 23.19 | 229.80 | 12.50 | 124.05 | 15.08 | 255.69 | -8.16 | 20.32 | 0.3962 | -1342.0 | -381.6 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 13.10 | 255.38 | -8.46 | 23.00 | 0.3683 | -967.0 | -815.0 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 16.64 | 255.18 | -8.66 | 20.06 | 0.4223 | -492.0 | -423.0 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 12.91 | 255.23 | -8.61 | 23.57 | 0.3665 | -1061.0 | -800.8 | |
| 14.88 | -3.00 | 8.03 | -3.00 | 15.02 | 255.09 | -8.75 | 21.71 | 0.3988 | -1249.3 | 999999 | |
| 3.41 | -3.00 | 1.84 | -3.00 | 14.80 | 254.88 | -8.96 | 22.40 | 0.3968 | -1032.4 | 999999 | |
| 0.70 | -3.00 | 0.38 | -3.00 | 14.58 | 254.86 | -8.98 | 22.67 | 0.3936 | -1008.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 18.86 | 254.21 | -9.63 | 20.21 | 0.4602 | -702.0 | -529.9 | |
| 0.00 | 2.80 | 0.00 | 1.54 | 16.99 | 254.03 | -9.82 | 22.16 | 0.4341 | 809.0 | 507.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 11.79 | 252.91 | -10.93 | 30.49 | 0.3673 | -925.0 | -842.4 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 11.76 | 252.76 | -11.08 | 30.88 | 0.3682 | -784.0 | -568.3 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 15.65 | 251.59 | -12.25 | 28.40 | 0.4314 | 841.0 | 656.6 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 16.40 | 250.62 | -13.22 | 29.40 | 0.4489 | 594.0 | 539.7 | |
| 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. | |