SDO HMI 2013-03-30 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 |
| 43.38 | 218.23 | 24.32 | 122.34 | 15.04 | 255.18 | 17.72 | 321.06 | 0.4697 | -965.3 | -405.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.36 | 18.79 | 257.93 | 20.47 | 321.88 | 0.5385 | -585.0 | -554.9 | |
| 0.00 | 2.10 | 0.00 | 1.21 | 17.21 | 257.14 | 19.68 | 321.02 | 0.5134 | -869.0 | -674.7 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 12.27 | 255.51 | 18.05 | 316.41 | 0.4409 | -875.0 | -725.2 | |
| 21.38 | 199.14 | 12.01 | 111.67 | 14.95 | 255.69 | 18.23 | 320.13 | 0.4735 | -1164.9 | -385.9 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 12.74 | 255.35 | 17.89 | 317.41 | 0.4445 | -811.0 | -691.1 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 12.96 | 255.27 | 17.81 | 317.87 | 0.4461 | -837.0 | -694.8 | |
| 0.00 | 1.93 | 0.00 | 1.07 | 13.18 | 255.19 | 17.73 | 318.34 | 0.4478 | -680.0 | -668.5 | |
| 0.00 | 3.59 | 0.00 | 1.98 | 12.70 | 255.05 | 17.59 | 317.81 | 0.4409 | -982.0 | -840.5 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 12.92 | 255.01 | 17.54 | 318.23 | 0.4429 | -955.0 | -733.2 | |
| 2.02 | -4.00 | 1.13 | -4.00 | 14.90 | 255.13 | 17.67 | 320.93 | 0.4674 | -1058.0 | 999999 | |
| 19.98 | -4.00 | 11.18 | -4.00 | 15.24 | 254.74 | 17.28 | 322.03 | 0.4677 | -1190.7 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.46 | 19.44 | 254.86 | 17.40 | 326.99 | 0.5197 | -762.0 | -641.6 | |
| 0.00 | 1.14 | 0.00 | 0.65 | 17.21 | 254.36 | 16.90 | 325.16 | 0.4882 | 668.0 | 588.8 | |
| 0.00 | 1.84 | 0.00 | 1.00 | 11.82 | 253.55 | 16.09 | 318.97 | 0.4150 | -935.0 | -770.8 | |
| 0.00 | 1.49 | 0.00 | 0.85 | 20.11 | 250.80 | 13.34 | 334.12 | 0.4985 | -726.0 | -676.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 14.53 | 250.26 | 12.80 | 329.06 | 0.4189 | 824.0 | 685.3 | |
| 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. | |