SDO HMI 2014-05-30 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.27 | 36.08 | 7.95 | 21.21 | -20.05 | 50.61 | 26.33 | 231.01 | 0.5361 | 231.0 | 83.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.93 | 13.00 | 5.99 | 7.84 | -19.55 | 54.22 | 29.95 | 235.68 | 0.5718 | 827.0 | 634.8 | |
| 0.00 | 1.44 | 0.00 | 0.87 | -19.39 | 53.86 | 29.58 | 235.63 | 0.5664 | 865.0 | 730.4 | |
| 1.81 | 5.60 | 1.08 | 3.34 | -19.01 | 53.56 | 29.29 | 235.98 | 0.5601 | 925.5 | 701.6 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -19.40 | 52.46 | 28.19 | 234.44 | 0.5498 | 603.0 | 456.0 | |
| 0.00 | 0.90 | 0.00 | 0.53 | -19.18 | 52.24 | 27.96 | 234.59 | 0.5454 | 688.0 | 620.1 | |
| 0.00 | 0.99 | 0.00 | 0.58 | -19.93 | 50.59 | 26.32 | 231.89 | 0.5318 | -637.0 | -455.9 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -20.67 | 50.44 | 26.17 | 230.58 | 0.5362 | 715.0 | 632.8 | |
| 1.53 | 3.07 | 0.88 | 1.76 | -19.58 | 48.67 | 24.40 | 230.48 | 0.5066 | -875.0 | -736.9 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -19.87 | 48.40 | 24.13 | 229.72 | 0.5060 | -641.0 | -543.8 | |
| 0.00 | 1.26 | 0.00 | 0.75 | -23.88 | 48.66 | 24.38 | 223.99 | 0.5457 | 563.0 | 589.2 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -19.79 | 46.00 | 21.73 | 227.06 | 0.4778 | -727.0 | -658.8 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -22.00 | 42.57 | 18.29 | 218.94 | 0.4649 | -730.0 | -609.2 | |
| 0.00 | 3.52 | 0.00 | 1.95 | -22.40 | 40.76 | 16.49 | 215.60 | 0.4526 | -690.0 | -531.1 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -21.56 | 38.36 | 14.08 | 212.69 | 0.4207 | -815.0 | -618.4 | |
| 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. | |