SDO HMI 2014-10-13 15:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.93 | 484.13 | 40.43 | 268.75 | -20.75 | 17.32 | -0.85 | 178.25 | 0.4522 | 914.2 | 354.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.40 | 2.89 | 0.76 | 1.57 | -18.07 | 20.70 | 2.52 | 185.86 | 0.4113 | 1028.7 | 811.2 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -18.00 | 19.91 | 1.74 | 184.05 | 0.4091 | 687.0 | 578.1 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -21.66 | 19.88 | 1.71 | 183.42 | 0.4666 | -898.0 | -682.5 | |
| 0.00 | 1.22 | 0.00 | 0.66 | -17.73 | 19.78 | 1.61 | 183.80 | 0.4048 | 816.0 | 679.8 | |
| 0.35 | 2.36 | 0.19 | 1.28 | -18.19 | 18.68 | 0.51 | 181.18 | 0.4113 | 1024.8 | 830.6 | |
| 19.24 | 455.02 | 10.68 | 252.70 | -20.91 | 17.89 | -0.29 | 179.41 | 0.4542 | 1335.9 | 390.8 | |
| 0.00 | 1.31 | 0.00 | 0.72 | -19.01 | 17.86 | -0.31 | 179.30 | 0.4243 | 942.0 | 727.1 | |
| 49.40 | -6.00 | 27.42 | -6.00 | -20.81 | 17.28 | -0.89 | 178.15 | 0.4528 | 1374.3 | 999999 | |
| 2.54 | 8.13 | 1.38 | 4.42 | -18.16 | 15.98 | -2.20 | 174.91 | 0.4123 | -954.0 | -644.9 | |
| 0.00 | 0.52 | 0.00 | 0.28 | -12.92 | 14.72 | -3.46 | 169.71 | 0.3305 | -588.0 | -567.5 | |
| 0.00 | 1.49 | 0.00 | 0.82 | -19.82 | 14.36 | -3.81 | 171.81 | 0.4413 | -820.0 | -599.3 | |
| 0.00 | 1.92 | 0.00 | 1.07 | -20.92 | 13.50 | -4.68 | 170.44 | 0.4605 | -683.0 | -484.7 | |
| 0.00 | 2.10 | 0.00 | 1.15 | -18.36 | 11.23 | -6.94 | 164.42 | 0.4289 | -796.0 | -549.2 | |
| 0.00 | 1.31 | 0.00 | 0.77 | -25.81 | 9.80 | -8.37 | 166.00 | 0.5441 | -475.0 | -428.7 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -25.60 | 9.72 | -8.46 | 165.76 | 0.5414 | -724.0 | -533.2 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -24.87 | 9.43 | -8.74 | 164.92 | 0.5321 | -589.0 | -406.6 | |
| 0.00 | 1.66 | 0.00 | 0.92 | -18.13 | 7.26 | -10.92 | 156.13 | 0.4466 | -661.0 | -524.6 | |
| 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. | |