SDO HMI 2014-06-10 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.19 | 0.00 | 11.26 | 6.53 | 257.50 | 30.94 | 282.40 | 0.5225 | 417.0 | 359.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.95 | 6.56 | 270.93 | 44.36 | 278.85 | 0.7053 | -484.0 | -392.8 | |
| 0.00 | 1.18 | 0.00 | 0.81 | 5.25 | 270.28 | 43.72 | 277.06 | 0.6958 | -656.0 | -573.8 | |
| 0.00 | 0.36 | 0.00 | 0.25 | 5.28 | 270.07 | 43.51 | 277.13 | 0.6932 | -702.0 | -706.5 | |
| 0.00 | 1.81 | 0.00 | 1.08 | 4.18 | 260.23 | 33.67 | 276.78 | 0.5589 | 657.0 | 532.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -0.50 | 258.14 | 31.57 | 268.24 | 0.5258 | 775.0 | 621.2 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 1.39 | 257.33 | 30.76 | 271.89 | 0.5136 | 581.0 | 386.7 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 4.68 | 257.12 | 30.55 | 278.34 | 0.5140 | 620.0 | 550.0 | |
| 0.00 | 3.89 | 0.00 | 2.24 | 9.94 | 255.77 | 29.21 | 288.96 | 0.5103 | 647.0 | 424.4 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 9.70 | 254.31 | 27.74 | 289.32 | 0.4882 | 716.0 | 611.8 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 9.45 | 254.11 | 27.55 | 288.95 | 0.4843 | 623.0 | 558.6 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 9.24 | 253.71 | 27.15 | 288.76 | 0.4775 | 777.0 | 664.2 | |
| 0.00 | 2.63 | 0.00 | 1.47 | 6.35 | 253.47 | 26.90 | 282.90 | 0.4633 | 752.0 | 598.8 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 4.48 | 248.78 | 22.21 | 280.54 | 0.3850 | 667.0 | 477.0 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 6.75 | 245.89 | 19.32 | 288.43 | 0.3478 | 865.0 | 717.2 | |
| 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. | |