SDO HMI 2011-05-31 22:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.74 | 186.14 | 19.59 | 136.52 | -20.17 | 19.95 | -44.31 | 117.15 | 0.7390 | 342.3 | 304.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.99 | -18.92 | 23.43 | -40.84 | 116.99 | 0.6965 | -820.0 | -664.4 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -18.99 | 23.32 | -40.94 | 117.03 | 0.6979 | -597.0 | -617.0 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -17.74 | 23.47 | -40.79 | 115.39 | 0.6911 | -804.0 | -680.3 | |
| 0.00 | 0.63 | 0.00 | 0.43 | -17.49 | 23.54 | -40.72 | 115.07 | 0.6893 | -659.0 | -591.7 | |
| 0.00 | 0.81 | 0.00 | 0.57 | -19.53 | 22.81 | -41.45 | 117.53 | 0.7059 | -532.0 | -419.4 | |
| 0.00 | 2.08 | 0.00 | 1.43 | -17.90 | 23.25 | -41.01 | 115.52 | 0.6942 | -699.0 | -578.7 | |
| 0.00 | 2.98 | 0.00 | 2.08 | -18.82 | 22.43 | -41.84 | 116.41 | 0.7072 | -735.0 | -629.2 | |
| 0.00 | 1.08 | 0.00 | 0.76 | -19.33 | 22.22 | -42.04 | 117.00 | 0.7115 | -482.0 | -495.7 | |
| 4.61 | 12.46 | 3.26 | 8.83 | -18.59 | 21.58 | -42.68 | 115.74 | 0.7156 | -720.4 | -175.3 | |
| 0.00 | 1.54 | 0.00 | 1.10 | -19.00 | 20.83 | -43.43 | 115.98 | 0.7253 | 718.0 | 505.7 | |
| 18.34 | 160.50 | 13.50 | 118.48 | -20.34 | 19.74 | -44.52 | 117.28 | 0.7420 | 1061.8 | 394.2 | |
| 0.00 | 0.81 | 0.00 | 0.61 | -21.74 | 19.16 | -45.11 | 118.81 | 0.7533 | 483.0 | 366.1 | |
| 3.79 | -11.00 | 2.83 | -11.00 | -20.66 | 19.16 | -45.10 | 117.45 | 0.7492 | 802.4 | 999999 | |
| 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. | |