SDO HMI 2014-04-24 16:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.43 | 346.10 | 34.54 | 227.41 | 17.93 | 166.23 | 34.71 | 304.49 | 0.6596 | -740.2 | -297.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.43 | 325.40 | 34.54 | 214.27 | 17.94 | 166.41 | 34.89 | 304.37 | 0.6616 | -1227.7 | -351.9 | |
| 0.00 | 2.40 | 0.00 | 1.54 | 17.23 | 164.61 | 33.09 | 304.78 | 0.6372 | 240.0 | 101.4 | |
| 0.00 | 1.78 | 0.00 | 1.13 | 16.99 | 164.34 | 32.82 | 304.67 | 0.6325 | 650.0 | 548.7 | |
| 0.00 | 1.42 | 0.00 | 0.92 | 18.72 | 164.44 | 32.92 | 306.90 | 0.6459 | 357.0 | 211.6 | |
| 0.00 | 2.13 | 0.00 | 1.35 | 17.72 | 163.28 | 31.77 | 306.50 | 0.6261 | 576.0 | 522.6 | |
| 0.00 | 3.38 | 0.00 | 2.14 | 18.01 | 163.19 | 31.68 | 306.97 | 0.6273 | 663.0 | 586.6 | |
| 0.00 | 1.33 | 0.00 | 0.85 | 18.28 | 163.25 | 31.73 | 307.27 | 0.6299 | 515.0 | 430.0 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 18.30 | 163.03 | 31.51 | 307.49 | 0.6277 | 556.0 | 452.4 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 17.77 | 162.88 | 31.37 | 306.90 | 0.6221 | 566.0 | 492.5 | |
| 0.00 | 2.04 | 0.00 | 1.29 | 18.06 | 162.83 | 31.31 | 307.34 | 0.6237 | 700.0 | 585.7 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 18.25 | 162.76 | 31.24 | 307.66 | 0.6244 | 609.0 | 518.1 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 18.55 | 162.74 | 31.23 | 308.06 | 0.6265 | 694.0 | 585.5 | |
| 0.00 | 0.71 | 0.00 | 0.45 | 18.15 | 162.55 | 31.03 | 307.69 | 0.6214 | 773.0 | 648.9 | |
| 0.00 | 1.07 | 0.00 | 0.65 | 13.80 | 161.73 | 30.21 | 302.21 | 0.5798 | 317.0 | 242.1 | |
| 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. | |