SDO HMI 2014-09-13 20:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 26.03 | 0.33 | 16.46 | -23.92 | 73.74 | 22.42 | 214.07 | 0.6222 | 76.3 | 96.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.69 | 0.00 | 1.10 | -21.58 | 80.04 | 28.73 | 223.71 | 0.6490 | 684.0 | 582.6 | |
| 0.00 | 0.80 | 0.00 | 0.53 | -23.21 | 80.23 | 28.91 | 222.07 | 0.6654 | 588.0 | 444.7 | |
| 0.00 | 0.98 | 0.00 | 0.63 | -22.34 | 79.02 | 27.71 | 221.85 | 0.6468 | 389.0 | 481.3 | |
| 0.00 | 4.71 | 0.00 | 3.10 | -23.60 | 79.16 | 27.84 | 220.61 | 0.6597 | 806.0 | 603.2 | |
| 0.00 | 1.24 | 0.00 | 0.81 | -23.42 | 78.60 | 27.28 | 220.24 | 0.6533 | 754.0 | 553.2 | |
| 0.00 | 1.87 | 0.00 | 1.18 | -23.52 | 75.04 | 23.72 | 216.34 | 0.6249 | 807.0 | 527.0 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -22.33 | 74.79 | 23.47 | 217.30 | 0.6102 | 711.0 | 540.1 | |
| 0.00 | 3.02 | 0.00 | 1.93 | -24.56 | 74.67 | 23.35 | 214.87 | 0.6328 | 626.0 | 424.9 | |
| 0.00 | 1.42 | 0.00 | 0.87 | -24.16 | 69.53 | 18.21 | 208.97 | 0.5909 | -844.0 | -715.6 | |
| 0.00 | 2.04 | 0.00 | 1.26 | -24.99 | 69.02 | 17.71 | 207.58 | 0.5976 | -688.0 | -595.9 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -24.66 | 68.77 | 17.45 | 207.52 | 0.5919 | -607.0 | -641.0 | |
| 0.53 | 3.56 | 0.33 | 2.18 | -24.86 | 68.59 | 17.27 | 207.11 | 0.5933 | -877.5 | -733.8 | |
| 0.00 | 1.33 | 0.00 | 0.80 | -22.94 | 67.03 | 15.71 | 206.59 | 0.5592 | -236.0 | -155.2 | |
| 0.00 | 2.04 | 0.00 | 1.25 | -25.80 | 65.14 | 13.82 | 201.65 | 0.5851 | -729.0 | -519.6 | |
| 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. | |