SDO HMI 2014-08-14 11:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.57 | 352.71 | 42.54 | 230.46 | 14.79 | 133.17 | 40.56 | 284.95 | 0.6527 | -498.6 | -226.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.66 | 13.72 | 134.72 | 42.11 | 283.21 | 0.6714 | 546.0 | 350.6 | |
| 50.60 | 309.54 | 33.52 | 204.88 | 15.38 | 134.10 | 41.49 | 285.78 | 0.6660 | -1200.4 | -320.4 | |
| 2.89 | -2.00 | 1.90 | -2.00 | 14.92 | 133.61 | 41.00 | 285.18 | 0.6591 | -1029.9 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 10.96 | 128.29 | 35.68 | 279.64 | 0.5831 | 595.0 | 533.8 | |
| 0.00 | 1.44 | 0.00 | 0.88 | 12.76 | 127.99 | 35.38 | 282.77 | 0.5813 | 758.0 | 603.8 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 9.84 | 126.64 | 34.03 | 277.85 | 0.5587 | 602.0 | 456.7 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 9.83 | 126.38 | 33.77 | 277.85 | 0.5550 | 608.0 | 419.0 | |
| 0.00 | 1.17 | 0.00 | 0.70 | 9.35 | 126.25 | 33.64 | 276.99 | 0.5528 | 705.0 | 572.5 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 9.58 | 126.02 | 33.41 | 277.42 | 0.5496 | 700.0 | 623.3 | |
| 0.81 | 28.05 | 0.48 | 16.52 | 10.58 | 125.65 | 33.04 | 279.29 | 0.5452 | 740.3 | 677.4 | |
| 0.63 | 1.80 | 0.37 | 1.06 | 9.58 | 125.50 | 32.89 | 277.47 | 0.5421 | 848.7 | 749.7 | |
| 0.00 | 1.35 | 0.00 | 0.80 | 10.89 | 125.62 | 33.01 | 279.87 | 0.5451 | 605.0 | 558.9 | |
| 10.64 | -10.00 | 6.27 | -10.00 | 10.01 | 125.48 | 32.87 | 278.27 | 0.5421 | 950.6 | 999999 | |
| 0.00 | 1.98 | 0.00 | 1.16 | 9.17 | 125.24 | 32.63 | 276.73 | 0.5380 | 886.0 | 758.3 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 10.64 | 125.15 | 32.54 | 279.48 | 0.5380 | 777.0 | 661.8 | |
| 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. | |