SDO HMI 2011-07-19 08:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.33 | 100.94 | 31.13 | 118.25 | 24.50 | 78.81 | -64.66 | 65.11 | 0.9079 | -124.4 | -177.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.27 | 1.82 | 1.47 | 2.10 | 25.44 | 79.34 | -64.13 | 64.03 | 0.9056 | -289.1 | -192.3 | |
| 12.44 | 66.45 | 14.02 | 74.76 | 24.49 | 80.02 | -63.45 | 64.99 | 0.9001 | -716.2 | -387.9 | |
| 1.72 | -2.00 | 1.96 | -2.00 | 24.80 | 79.73 | -63.74 | 64.69 | 0.9024 | -509.4 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.93 | 25.70 | 78.84 | -64.63 | 63.80 | 0.9091 | -170.0 | -106.7 | |
| 2.36 | 4.45 | 2.75 | 5.19 | 24.61 | 78.97 | -64.50 | 64.98 | 0.9073 | -163.5 | -106.0 | |
| 0.00 | 1.45 | 0.00 | 1.74 | 24.36 | 78.19 | -65.28 | 65.35 | 0.9122 | 407.0 | 357.2 | |
| 0.00 | 1.63 | 0.00 | 1.98 | 23.70 | 77.78 | -65.69 | 66.11 | 0.9144 | 577.0 | 479.1 | |
| 0.00 | 1.82 | 0.00 | 2.17 | 23.26 | 78.12 | -65.35 | 66.55 | 0.9119 | 505.0 | 429.0 | |
| 5.45 | 6.08 | 6.79 | 7.57 | 23.84 | 77.06 | -66.42 | 66.02 | 0.9191 | 510.0 | 590.6 | |
| 0.00 | 1.45 | 0.00 | 1.84 | 24.24 | 76.56 | -66.91 | 65.64 | 0.9224 | 412.0 | 372.9 | |
| 0.00 | 1.82 | 0.00 | 2.31 | 24.04 | 76.51 | -66.96 | 65.86 | 0.9226 | 355.0 | 278.4 | |
| 0.91 | 8.53 | 1.23 | 11.59 | 25.05 | 74.92 | -68.55 | 64.91 | 0.9326 | 566.2 | 304.5 | |
| 1.36 | 3.81 | 1.80 | 5.07 | 24.23 | 75.60 | -67.87 | 65.73 | 0.9282 | 409.9 | 248.6 | |
| 0.82 | -12.00 | 1.11 | -12.00 | 24.84 | 74.80 | -68.67 | 65.14 | 0.9332 | 280.7 | 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. | |