SDO HMI 2014-09-16 08:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.39 | 202.55 | 47.73 | 281.15 | 15.45 | 88.54 | 70.23 | 283.84 | 0.9357 | 447.7 | 155.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.33 | 150.91 | 35.36 | 210.39 | 14.86 | 88.62 | 70.31 | 283.21 | 0.9363 | 626.7 | 194.6 | |
| 1.33 | 17.15 | 1.93 | 24.58 | 16.60 | 89.48 | 71.16 | 285.11 | 0.9409 | -482.1 | -118.3 | |
| 2.31 | -2.00 | 3.31 | -2.00 | 16.82 | 89.27 | 70.96 | 285.33 | 0.9397 | 105.0 | 999999 | |
| 0.00 | 2.04 | 0.00 | 2.88 | 17.23 | 88.96 | 70.65 | 285.76 | 0.9379 | 538.0 | 386.0 | |
| 0.00 | 1.24 | 0.00 | 1.78 | 17.76 | 89.26 | 70.94 | 286.34 | 0.9395 | -191.0 | -160.8 | |
| 0.00 | 2.04 | 0.00 | 2.79 | 17.32 | 88.19 | 69.87 | 285.84 | 0.9333 | 158.0 | 105.3 | |
| 0.00 | 0.89 | 0.00 | 1.27 | 18.82 | 89.19 | 70.88 | 287.46 | 0.9390 | -209.0 | -176.7 | |
| 0.00 | 0.27 | 0.00 | 0.37 | 18.20 | 88.50 | 70.19 | 286.79 | 0.9351 | -172.0 | -146.0 | |
| 4.53 | 6.58 | 6.03 | 8.74 | 17.24 | 87.56 | 69.25 | 285.74 | 0.9295 | 489.8 | 410.0 | |
| 0.00 | 4.18 | 0.00 | 5.43 | 16.55 | 87.01 | 68.70 | 284.98 | 0.9261 | 511.0 | 406.0 | |
| 0.00 | 9.60 | 0.00 | 12.94 | 17.64 | 87.91 | 69.59 | 286.17 | 0.9315 | 140.0 | 109.3 | |
| 0.00 | 3.56 | 0.00 | 4.91 | 18.80 | 88.50 | 70.18 | 287.43 | 0.9350 | -604.0 | -453.6 | |
| 0.89 | 2.49 | 1.10 | 3.08 | 15.79 | 85.69 | 67.38 | 284.13 | 0.9177 | 411.8 | 284.5 | |
| 0.00 | 1.07 | 0.00 | 1.34 | 17.36 | 86.18 | 67.86 | 285.86 | 0.9207 | 336.0 | 258.8 | |
| 0.00 | 0.53 | 0.00 | 0.65 | 17.70 | 85.44 | 67.12 | 286.22 | 0.9158 | 352.0 | 274.3 | |
| 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. | |