SDO HMI 2014-03-10 11:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.86 | 66.33 | 8.10 | 33.88 | 6.40 | 11.12 | 3.15 | 347.09 | 0.2457 | 179.4 | 230.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.60 | 0.00 | 1.34 | 4.22 | 18.34 | 10.37 | 317.58 | 0.2672 | 723.0 | 601.5 | |
| 2.43 | 4.85 | 1.24 | 2.48 | 5.92 | 14.07 | 6.10 | 334.99 | 0.2512 | -1052.6 | -768.1 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 6.19 | 13.71 | 5.74 | 336.72 | 0.2529 | -993.0 | -802.2 | |
| 0.00 | 3.29 | 0.00 | 1.69 | 6.73 | 13.27 | 5.30 | 339.14 | 0.2587 | -1077.0 | -852.1 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 6.00 | 13.11 | 5.14 | 338.67 | 0.2461 | -1018.0 | -741.4 | |
| 6.24 | 11.36 | 3.20 | 5.82 | 7.30 | 11.59 | 3.62 | 345.97 | 0.2594 | -929.4 | -470.6 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 6.78 | 10.83 | 2.87 | 348.40 | 0.2479 | 839.0 | 700.3 | |
| 0.95 | 3.81 | 0.48 | 1.94 | 5.22 | 10.65 | 2.68 | 347.81 | 0.2212 | 1109.0 | 899.8 | |
| 0.35 | 1.39 | 0.18 | 0.71 | 5.58 | 10.38 | 2.41 | 349.31 | 0.2264 | 976.8 | 894.5 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 4.76 | 10.37 | 2.40 | 348.61 | 0.2126 | 895.0 | 704.9 | |
| 0.00 | 1.91 | 0.00 | 0.97 | 5.67 | 10.29 | 2.32 | 349.77 | 0.2277 | 733.0 | 606.8 | |
| 1.82 | 5.90 | 0.93 | 3.02 | 7.51 | 10.12 | 2.15 | 351.68 | 0.2581 | -829.8 | -88.5 | |
| 0.00 | 0.78 | 0.00 | 0.40 | 7.23 | 10.12 | 2.15 | 351.53 | 0.2535 | 409.0 | 291.9 | |
| 0.00 | 0.87 | 0.00 | 0.44 | 5.58 | 9.90 | 1.93 | 351.40 | 0.2250 | 944.0 | 773.1 | |
| 4.07 | 12.92 | 2.07 | 6.57 | 5.88 | 9.84 | 1.87 | 351.85 | 0.2301 | 1064.6 | 595.5 | |
| 0.00 | 6.85 | 0.00 | 3.50 | 6.89 | 9.76 | 1.79 | 352.77 | 0.2469 | 945.0 | 792.5 | |
| 0.00 | 2.17 | 0.00 | 1.10 | 6.22 | 8.70 | 0.73 | 356.86 | 0.2338 | 846.0 | 743.3 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 8.01 | 5.88 | -2.09 | 7.82 | 0.2663 | 773.0 | 540.1 | |
| 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. | |