SDO HMI 2014-03-02 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.89 | 88.74 | 13.53 | 57.17 | -7.51 | 152.28 | 40.00 | 266.92 | 0.6404 | 642.9 | 326.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.16 | 73.29 | 12.42 | 47.56 | -7.46 | 152.80 | 40.52 | 266.96 | 0.6475 | 964.0 | 350.3 | |
| 0.00 | 1.47 | 0.00 | 0.95 | -7.95 | 152.69 | 40.42 | 266.22 | 0.6459 | 589.0 | 500.0 | |
| 0.69 | -1.00 | 0.45 | -1.00 | -7.79 | 152.48 | 40.20 | 266.48 | 0.6431 | 873.5 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.89 | -7.94 | 152.46 | 40.18 | 266.25 | 0.6427 | 674.0 | 495.3 | |
| 0.00 | 1.29 | 0.00 | 0.82 | -7.45 | 151.46 | 39.19 | 267.07 | 0.6297 | 480.0 | 534.7 | |
| 0.69 | 1.47 | 0.44 | 0.93 | -7.55 | 151.36 | 39.08 | 266.92 | 0.6282 | 698.6 | 662.9 | |
| 0.00 | 1.81 | 0.00 | 1.15 | -7.39 | 151.15 | 38.87 | 267.19 | 0.6254 | 366.0 | 319.2 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -8.45 | 151.27 | 38.99 | 265.48 | 0.6266 | 765.0 | 603.7 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -7.12 | 149.97 | 37.70 | 267.71 | 0.6096 | -484.0 | -363.6 | |
| 0.35 | 1.21 | 0.22 | 0.75 | -7.87 | 149.93 | 37.66 | 266.48 | 0.6086 | -758.5 | -682.3 | |
| 0.00 | 0.78 | 0.00 | 0.48 | -7.29 | 149.23 | 36.96 | 267.47 | 0.5992 | 744.0 | 616.1 | |
| 0.00 | 1.29 | 0.00 | 0.78 | -8.91 | 147.43 | 35.15 | 264.76 | 0.5734 | 746.0 | 625.8 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -9.09 | 147.41 | 35.14 | 264.44 | 0.5732 | 655.0 | 556.3 | |
| 0.00 | 1.99 | 0.00 | 1.16 | -5.77 | 144.53 | 32.25 | 270.64 | 0.5331 | -799.0 | -663.5 | |
| 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. | |