SDO HMI 2014-10-13 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.24 | 492.85 | 39.56 | 273.82 | -20.85 | 17.40 | 1.43 | 182.96 | 0.4540 | 1054.2 | 367.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.52 | 1.66 | 0.29 | 0.90 | -18.08 | 20.79 | 4.82 | 191.10 | 0.4170 | 998.7 | 838.8 | |
| 0.00 | 1.57 | 0.00 | 0.88 | -21.67 | 20.09 | 4.12 | 188.20 | 0.4706 | -850.0 | -683.9 | |
| 0.00 | 2.19 | 0.00 | 1.23 | -21.83 | 19.90 | 3.93 | 187.77 | 0.4727 | -771.0 | -603.4 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -21.80 | 19.74 | 3.77 | 187.47 | 0.4718 | -844.0 | -591.0 | |
| 0.00 | 1.40 | 0.00 | 0.76 | -18.16 | 18.96 | 3.00 | 186.92 | 0.4137 | 1056.0 | 879.2 | |
| 21.85 | 470.82 | 12.15 | 261.61 | -20.94 | 17.86 | 1.89 | 183.89 | 0.4558 | 1366.1 | 401.5 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.08 | 17.84 | 1.87 | 184.17 | 0.4265 | 677.0 | 517.7 | |
| 46.42 | -6.00 | 25.77 | -6.00 | -20.84 | 17.25 | 1.28 | 182.65 | 0.4536 | 1473.4 | 999999 | |
| 1.14 | 6.73 | 0.62 | 3.65 | -18.12 | 15.91 | -0.06 | 179.86 | 0.4101 | -896.7 | -742.7 | |
| 0.00 | 0.87 | 0.00 | 0.48 | -19.87 | 13.97 | -2.00 | 175.69 | 0.4391 | -719.0 | -605.4 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -20.91 | 13.82 | -2.14 | 175.58 | 0.4555 | 419.0 | 416.9 | |
| 1.31 | 2.45 | 0.73 | 1.36 | -20.98 | 13.02 | -2.95 | 173.96 | 0.4577 | -863.7 | -708.2 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -25.91 | 10.97 | -5.00 | 171.56 | 0.5358 | -693.0 | -493.8 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -25.81 | 9.91 | -6.06 | 169.76 | 0.5370 | -699.0 | -490.7 | |
| 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. | |