SDO HMI 2014-03-04 21:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.70 | 0.00 | 11.89 | 9.11 | 119.47 | 37.95 | 294.42 | 0.6592 | -204.2 | -154.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.67 | 5.30 | 129.97 | 48.45 | 283.21 | 0.7677 | -545.0 | -444.9 | |
| 0.00 | 1.12 | 0.00 | 0.86 | 5.01 | 129.80 | 48.28 | 282.90 | 0.7652 | -456.0 | -402.8 | |
| 0.00 | 1.55 | 0.00 | 1.20 | 7.45 | 129.52 | 48.00 | 286.08 | 0.7692 | -664.0 | -520.6 | |
| 0.00 | 0.95 | 0.00 | 0.73 | 6.27 | 129.32 | 47.80 | 284.66 | 0.7634 | -560.0 | -474.6 | |
| 0.00 | 1.73 | 0.00 | 1.34 | 7.91 | 129.55 | 48.03 | 286.65 | 0.7709 | -573.0 | -461.6 | |
| 0.00 | 0.69 | 0.00 | 0.53 | 6.49 | 129.03 | 47.51 | 285.03 | 0.7610 | -744.0 | -674.9 | |
| 0.00 | 0.78 | 0.00 | 0.53 | 12.53 | 120.47 | 38.95 | 296.88 | 0.6904 | -711.0 | -552.8 | |
| 0.00 | 0.69 | 0.00 | 0.47 | 13.09 | 119.64 | 38.12 | 298.13 | 0.6841 | -702.0 | -600.6 | |
| 0.00 | 1.30 | 0.00 | 0.87 | 12.80 | 119.51 | 37.99 | 297.83 | 0.6810 | -727.0 | -551.1 | |
| 0.00 | 0.86 | 0.00 | 0.55 | 12.52 | 114.58 | 33.06 | 300.87 | 0.6228 | -634.0 | -474.7 | |
| 0.00 | 1.38 | 0.00 | 0.83 | 12.54 | 110.04 | 28.52 | 304.77 | 0.5696 | 660.0 | 460.5 | |
| 0.00 | 1.21 | 0.00 | 0.73 | 14.34 | 109.47 | 27.95 | 307.91 | 0.5779 | 619.0 | 478.6 | |
| 0.00 | 2.16 | 0.00 | 1.24 | 8.03 | 107.53 | 26.01 | 300.02 | 0.5036 | 682.0 | 552.2 | |
| 0.00 | 1.04 | 0.00 | 0.58 | 6.53 | 105.85 | 24.33 | 299.02 | 0.4700 | 618.0 | 516.3 | |
| 0.00 | 1.38 | 0.00 | 0.76 | 9.76 | 101.24 | 19.72 | 310.62 | 0.4400 | 674.0 | 455.4 | |
| 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. | |