SDO HMI 2013-03-30 13:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.02 | 244.69 | 25.42 | 135.18 | 15.02 | 255.21 | 14.99 | 325.57 | 0.4441 | -928.6 | -341.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.37 | 0.00 | 1.28 | 12.03 | 255.52 | 15.31 | 320.71 | 0.4095 | -858.0 | -643.9 | |
| 24.89 | 219.44 | 13.77 | 121.30 | 14.94 | 255.69 | 15.47 | 324.63 | 0.4472 | -1167.1 | -323.2 | |
| 0.00 | 2.54 | 0.00 | 1.39 | 13.14 | 255.44 | 15.22 | 322.56 | 0.4223 | -656.0 | -496.4 | |
| 0.00 | 3.33 | 0.00 | 1.81 | 12.59 | 255.11 | 14.90 | 322.33 | 0.4123 | -568.0 | -782.9 | |
| 1.58 | -2.00 | 0.87 | -2.00 | 14.89 | 255.17 | 14.96 | 325.48 | 0.4419 | -1160.1 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.48 | 14.40 | 255.14 | 14.92 | 324.89 | 0.4355 | -737.0 | -656.9 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 12.84 | 255.00 | 14.79 | 322.91 | 0.4144 | -841.0 | -729.6 | |
| 0.88 | 3.33 | 0.48 | 1.81 | 12.67 | 254.83 | 14.62 | 322.98 | 0.4107 | -1086.7 | -913.6 | |
| 18.67 | -2.00 | 10.30 | -2.00 | 15.20 | 254.78 | 14.56 | 326.59 | 0.4425 | -1197.7 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.00 | 13.65 | 254.64 | 14.42 | 324.77 | 0.4214 | -998.0 | -875.5 | |
| 0.00 | 5.87 | 0.00 | 3.35 | 19.36 | 254.96 | 14.74 | 331.06 | 0.4982 | -397.0 | -535.2 | |
| 0.00 | 0.79 | 0.00 | 0.44 | 16.84 | 251.88 | 11.67 | 333.93 | 0.4422 | 780.0 | 646.0 | |
| 0.00 | 1.67 | 0.00 | 0.90 | 14.76 | 251.57 | 11.35 | 332.27 | 0.4108 | 718.0 | 632.6 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 14.47 | 250.23 | 10.02 | 334.81 | 0.3973 | 762.0 | 558.8 | |
| 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. | |