SDO HMI 2011-06-30 20:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.02 | 130.21 | 29.41 | 83.21 | 16.23 | 350.90 | -37.39 | 67.41 | 0.6333 | -119.9 | 25.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.36 | 0.00 | 0.21 | 17.62 | 359.06 | -29.22 | 60.64 | 0.5360 | -595.0 | -488.8 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 19.11 | 357.70 | -30.59 | 59.14 | 0.5622 | -770.0 | -576.2 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 17.41 | 355.75 | -32.54 | 63.16 | 0.5774 | -672.0 | -516.9 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 15.72 | 355.84 | -32.45 | 65.91 | 0.5679 | -562.0 | -498.1 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 20.61 | 352.69 | -35.59 | 60.00 | 0.6313 | -653.0 | -552.5 | |
| 0.00 | 0.82 | 0.00 | 0.52 | 20.42 | 352.63 | -35.66 | 60.32 | 0.6311 | -420.0 | -372.4 | |
| 0.00 | 0.45 | 0.00 | 0.28 | 16.65 | 353.29 | -35.00 | 65.71 | 0.6051 | -699.0 | -621.4 | |
| 0.00 | 1.36 | 0.00 | 0.85 | 18.10 | 352.93 | -35.36 | 63.65 | 0.6161 | -730.0 | -622.4 | |
| 0.00 | 1.00 | 0.00 | 0.62 | 15.74 | 353.17 | -35.12 | 67.22 | 0.6028 | -824.0 | -668.6 | |
| 1.45 | 52.57 | 0.90 | 32.91 | 16.24 | 352.91 | -35.38 | 66.56 | 0.6081 | -940.7 | -522.3 | |
| 7.08 | -10.00 | 4.41 | -10.00 | 15.95 | 352.85 | -35.44 | 67.03 | 0.6077 | -920.7 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.62 | 16.48 | 352.58 | -35.70 | 66.33 | 0.6133 | -531.0 | -374.5 | |
| 0.00 | 2.00 | 0.00 | 1.24 | 15.42 | 352.80 | -35.49 | 67.90 | 0.6062 | -599.0 | -441.4 | |
| 10.35 | -10.00 | 6.48 | -10.00 | 16.10 | 352.51 | -35.78 | 66.96 | 0.6127 | -787.8 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.26 | 17.32 | 352.08 | -36.21 | 65.27 | 0.6231 | -781.0 | -652.3 | |
| 7.54 | -10.00 | 4.75 | -10.00 | 16.30 | 351.95 | -36.34 | 66.89 | 0.6205 | -671.2 | 999999 | |
| 1.54 | 3.36 | 0.97 | 2.11 | 15.27 | 351.93 | -36.36 | 68.51 | 0.6168 | -567.4 | -549.5 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 16.54 | 351.50 | -36.78 | 66.72 | 0.6271 | -347.0 | -259.9 | |
| 0.00 | 1.27 | 0.00 | 0.81 | 17.57 | 351.10 | -37.18 | 65.34 | 0.6362 | -375.0 | -345.9 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 13.98 | 351.55 | -36.73 | 70.70 | 0.6172 | -616.0 | -485.6 | |
| 0.00 | 1.18 | 0.00 | 0.75 | 15.22 | 351.19 | -37.10 | 68.90 | 0.6261 | -369.0 | -226.5 | |
| 0.00 | 1.73 | 0.00 | 1.11 | 15.35 | 350.33 | -37.96 | 69.04 | 0.6375 | 34.0 | 19.2 | |
| 3.27 | 17.98 | 2.12 | 11.67 | 15.74 | 349.71 | -38.57 | 68.68 | 0.6465 | 922.1 | 691.8 | |
| 0.00 | 1.82 | 0.00 | 1.18 | 15.32 | 349.52 | -38.77 | 69.38 | 0.6475 | 757.0 | 681.9 | |
| 5.90 | -23.00 | 3.85 | -23.00 | 15.91 | 349.31 | -38.98 | 68.57 | 0.6521 | 866.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.95 | 15.60 | 349.34 | -38.95 | 69.03 | 0.6507 | 835.0 | 676.6 | |
| 0.00 | 9.35 | 0.00 | 6.15 | 16.21 | 348.78 | -39.50 | 68.33 | 0.6596 | 561.0 | 682.1 | |
| 0.00 | 1.73 | 0.00 | 1.13 | 15.74 | 348.65 | -39.64 | 69.08 | 0.6596 | 632.0 | 596.6 | |
| 0.00 | 1.36 | 0.00 | 0.89 | 14.64 | 348.81 | -39.47 | 70.64 | 0.6542 | 782.0 | 633.3 | |
| 0.00 | 2.27 | 0.00 | 1.49 | 14.67 | 348.56 | -39.72 | 70.69 | 0.6574 | 748.0 | 568.2 | |
| 3.81 | 13.62 | 2.54 | 9.08 | 16.91 | 347.94 | -40.34 | 67.63 | 0.6721 | 864.8 | 766.6 | |
| 3.72 | -31.00 | 2.48 | -31.00 | 16.57 | 347.99 | -40.30 | 68.11 | 0.6704 | 904.2 | 999999 | |
| 1.36 | -31.00 | 0.91 | -31.00 | 17.10 | 347.85 | -40.43 | 67.39 | 0.6738 | 749.2 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.41 | 18.07 | 347.42 | -40.87 | 66.18 | 0.6823 | 795.0 | 713.5 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 16.09 | 347.86 | -40.43 | 68.84 | 0.6704 | 649.0 | 496.8 | |
| 0.00 | 1.63 | 0.00 | 1.09 | 16.87 | 347.66 | -40.63 | 67.79 | 0.6753 | 445.0 | 415.9 | |
| 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. | |