SDO HMI 2014-01-16 02:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.00 | 372.00 | 38.51 | 201.73 | -16.22 | 12.24 | 21.40 | 239.51 | 0.4081 | 904.0 | 401.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.88 | 216.47 | 19.59 | 118.24 | -16.56 | 13.11 | 22.27 | 239.71 | 0.4224 | 1185.9 | 411.0 | |
| 1.62 | -1.00 | 0.88 | -1.00 | -16.67 | 12.56 | 21.71 | 238.92 | 0.4156 | 1204.9 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -15.87 | 12.07 | 21.23 | 240.16 | 0.4032 | 708.0 | 465.0 | |
| 0.00 | 2.72 | 0.00 | 1.47 | -16.41 | 11.83 | 20.99 | 238.69 | 0.4039 | 674.0 | 487.9 | |
| 0.00 | 1.70 | 0.00 | 0.91 | -14.83 | 11.60 | 20.76 | 242.06 | 0.3895 | -345.0 | -256.9 | |
| 0.00 | 1.28 | 0.00 | 0.69 | -17.02 | 11.61 | 20.76 | 237.10 | 0.4055 | 615.0 | 489.8 | |
| 33.50 | 137.23 | 18.04 | 73.82 | -15.82 | 11.41 | 20.57 | 239.55 | 0.3938 | 1255.5 | 483.9 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -14.69 | 11.13 | 20.29 | 241.89 | 0.3819 | 766.0 | 693.1 | |
| 0.00 | 3.32 | 0.00 | 1.74 | -15.23 | 7.25 | 16.41 | 235.58 | 0.3319 | -746.0 | -697.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -16.99 | 6.57 | 15.73 | 230.12 | 0.3393 | -812.0 | -659.8 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -17.80 | 5.23 | 14.38 | 225.81 | 0.3314 | -703.0 | -532.8 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -12.04 | 3.64 | 12.79 | 238.91 | 0.2541 | -792.0 | -699.7 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -12.26 | 3.37 | 12.53 | 237.66 | 0.2520 | -898.0 | -675.2 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -12.05 | 3.20 | 12.36 | 238.05 | 0.2479 | -653.0 | -565.9 | |
| 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. | |