SDO HMI 2014-05-26 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.05 | 195.11 | 100.69 | 404.41 | -18.66 | 150.08 | 75.63 | 251.05 | 0.9689 | 123.8 | -50.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.71 | 0.00 | 6.46 | -17.35 | 152.33 | 77.89 | 252.55 | 0.9792 | 393.0 | 316.3 | |
| 16.42 | 78.75 | 44.35 | 219.03 | -18.44 | 153.78 | 79.33 | 251.50 | 0.9839 | 191.0 | -32.6 | |
| 0.00 | 6.04 | 0.00 | 11.61 | -17.33 | 149.15 | 74.70 | 252.42 | 0.9670 | -46.0 | 25.3 | |
| 0.00 | 0.99 | 0.00 | 1.98 | -19.36 | 149.68 | 75.24 | 250.35 | 0.9698 | 225.0 | 290.0 | |
| 0.00 | 0.72 | 0.00 | 1.20 | -17.51 | 146.72 | 72.27 | 252.08 | 0.9560 | 130.0 | 157.0 | |
| 2.89 | 34.46 | 4.58 | 54.15 | -17.53 | 145.80 | 71.36 | 251.99 | 0.9514 | -289.2 | -227.6 | |
| 3.61 | -6.00 | 5.66 | -6.00 | -17.75 | 145.52 | 71.07 | 251.73 | 0.9501 | -353.9 | 999999 | |
| 4.06 | -6.00 | 6.28 | -6.00 | -18.08 | 145.23 | 70.78 | 251.36 | 0.9487 | -374.6 | 999999 | |
| 0.63 | 5.41 | 1.03 | 8.74 | -19.86 | 146.14 | 71.69 | 249.58 | 0.9541 | -70.9 | -243.1 | |
| 19.12 | 48.89 | 28.99 | 74.51 | -19.11 | 144.76 | 70.31 | 250.23 | 0.9467 | 477.8 | -138.7 | |
| 0.00 | 1.35 | 0.00 | 2.14 | -20.26 | 145.45 | 71.00 | 249.09 | 0.9509 | -382.0 | -352.4 | |
| 3.25 | -10.00 | 5.01 | -10.00 | -20.08 | 144.95 | 70.51 | 249.24 | 0.9483 | -558.8 | 999999 | |
| 3.07 | 15.79 | 4.79 | 24.59 | -21.05 | 145.10 | 70.66 | 248.23 | 0.9496 | -209.4 | 210.0 | |
| 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. | |