SDO HMI 2014-08-04 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.62 | 0.00 | 10.86 | 13.60 | 256.98 | 35.46 | 285.80 | 0.5889 | 473.9 | 418.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.53 | 16.51 | 269.08 | 47.57 | 286.89 | 0.7418 | -349.0 | -426.2 | |
| 0.00 | 1.18 | 0.00 | 0.82 | 16.16 | 266.22 | 44.70 | 286.90 | 0.7084 | -700.0 | -533.5 | |
| 0.00 | 0.72 | 0.00 | 0.46 | 9.21 | 260.19 | 38.67 | 277.24 | 0.6240 | 577.0 | 491.0 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 9.34 | 259.97 | 38.45 | 277.47 | 0.6211 | 626.0 | 597.1 | |
| 0.00 | 1.45 | 0.00 | 0.90 | 4.09 | 259.09 | 37.57 | 268.88 | 0.6105 | 514.0 | 396.4 | |
| 0.00 | 1.18 | 0.00 | 0.74 | 8.89 | 259.40 | 37.89 | 276.77 | 0.6132 | 668.0 | 573.0 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 7.05 | 259.08 | 37.57 | 273.74 | 0.6086 | 692.0 | 598.6 | |
| 0.00 | 1.45 | 0.00 | 0.92 | 16.65 | 259.52 | 38.00 | 289.23 | 0.6270 | 569.0 | 455.6 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 13.29 | 257.26 | 35.74 | 284.39 | 0.5891 | 686.0 | 547.8 | |
| 0.00 | 1.90 | 0.00 | 1.18 | 17.16 | 257.84 | 36.32 | 290.60 | 0.6069 | 607.0 | 529.4 | |
| 0.00 | 2.08 | 0.00 | 1.25 | 14.64 | 255.81 | 34.29 | 287.09 | 0.5725 | 635.0 | 533.0 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 16.35 | 248.16 | 26.65 | 293.82 | 0.4724 | 648.0 | 518.5 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 10.58 | 244.95 | 23.43 | 282.70 | 0.4024 | 579.0 | 465.8 | |
| 0.00 | 2.35 | 0.00 | 1.30 | 20.19 | 244.55 | 23.04 | 304.53 | 0.4476 | 882.0 | 733.3 | |
| 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. | |