SDO HMI 2011-08-26 12:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.48 | 169.55 | 29.20 | 180.76 | 17.39 | 61.82 | 63.00 | 286.05 | 0.8851 | -127.0 | -93.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.78 | 64.89 | 11.59 | 77.20 | 16.79 | 65.06 | 66.25 | 285.28 | 0.9101 | -711.4 | -112.3 | |
| 0.00 | 1.17 | 0.00 | 1.26 | 15.69 | 62.27 | 63.45 | 284.05 | 0.8897 | -270.0 | -250.4 | |
| 0.00 | 0.63 | 0.00 | 0.68 | 16.31 | 62.56 | 63.75 | 284.75 | 0.8919 | -418.0 | -309.1 | |
| 0.00 | 0.99 | 0.00 | 1.07 | 16.72 | 62.59 | 63.78 | 285.21 | 0.8922 | -334.0 | -323.0 | |
| 3.05 | 9.06 | 3.31 | 9.88 | 17.42 | 62.52 | 63.71 | 285.99 | 0.8917 | -494.7 | -137.9 | |
| 1.62 | -5.00 | 1.76 | -5.00 | 17.67 | 62.54 | 63.73 | 286.27 | 0.8919 | -471.9 | 999999 | |
| 0.00 | 1.17 | 0.00 | 1.27 | 17.85 | 62.65 | 63.84 | 286.47 | 0.8928 | -271.0 | -267.7 | |
| 0.00 | 1.17 | 0.00 | 1.29 | 18.88 | 63.07 | 64.26 | 287.62 | 0.8961 | 203.0 | 166.8 | |
| 0.00 | 1.97 | 0.00 | 2.15 | 18.32 | 62.61 | 63.80 | 287.01 | 0.8926 | -563.0 | -403.6 | |
| 0.00 | 1.26 | 0.00 | 1.30 | 16.62 | 60.91 | 62.10 | 285.11 | 0.8791 | -534.0 | -442.0 | |
| 1.53 | 19.56 | 1.57 | 20.01 | 16.97 | 60.84 | 62.03 | 285.52 | 0.8786 | -704.9 | -557.3 | |
| 1.08 | 2.69 | 1.12 | 2.80 | 17.35 | 61.07 | 62.26 | 285.95 | 0.8805 | -520.0 | -381.3 | |
| 0.81 | 2.69 | 0.81 | 2.69 | 16.70 | 59.82 | 61.01 | 285.24 | 0.8703 | 137.4 | -178.6 | |
| 0.00 | 0.90 | 0.00 | 0.89 | 16.51 | 59.52 | 60.71 | 285.03 | 0.8678 | 135.0 | 118.4 | |
| 0.45 | 2.06 | 0.45 | 2.09 | 18.16 | 60.26 | 61.45 | 286.90 | 0.8743 | -467.4 | -447.5 | |
| 0.00 | 5.03 | 0.00 | 5.05 | 17.84 | 60.01 | 61.19 | 286.54 | 0.8721 | -110.0 | -172.3 | |
| 0.00 | 1.53 | 0.00 | 1.56 | 18.96 | 60.56 | 61.74 | 287.80 | 0.8769 | -394.0 | -366.8 | |
| 0.00 | 0.99 | 0.00 | 0.95 | 15.89 | 58.63 | 59.81 | 284.32 | 0.8601 | -420.0 | -289.3 | |
| 0.00 | 1.35 | 0.00 | 1.31 | 17.73 | 59.02 | 60.21 | 286.45 | 0.8639 | 143.0 | 66.3 | |
| 0.00 | 1.08 | 0.00 | 1.05 | 17.41 | 58.78 | 59.97 | 286.09 | 0.8618 | 153.0 | 110.5 | |
| 0.72 | 13.10 | 0.70 | 12.92 | 18.32 | 59.10 | 60.29 | 287.13 | 0.8648 | 360.5 | 127.9 | |
| 0.00 | 0.45 | 0.00 | 0.42 | 15.34 | 57.56 | 58.75 | 283.71 | 0.8507 | 426.0 | 373.2 | |
| 5.74 | 9.42 | 5.49 | 9.00 | 17.08 | 58.29 | 59.47 | 285.73 | 0.8575 | 523.5 | 513.2 | |
| 0.00 | 0.99 | 0.00 | 0.98 | 19.40 | 59.63 | 60.82 | 288.35 | 0.8696 | 529.0 | 503.5 | |
| 0.00 | 0.90 | 0.00 | 0.85 | 16.71 | 57.97 | 59.16 | 285.30 | 0.8546 | 385.0 | 362.7 | |
| 0.00 | 1.17 | 0.00 | 1.16 | 19.63 | 59.58 | 60.76 | 288.62 | 0.8693 | 329.0 | 231.4 | |
| 1.53 | 6.37 | 1.45 | 6.11 | 17.50 | 58.13 | 59.32 | 286.23 | 0.8563 | 457.2 | 263.3 | |
| 0.00 | 1.35 | 0.00 | 1.33 | 19.69 | 59.29 | 60.47 | 288.71 | 0.8669 | 394.0 | 284.4 | |
| 0.00 | 0.81 | 0.00 | 0.80 | 20.36 | 59.26 | 60.45 | 289.49 | 0.8671 | 174.0 | 130.1 | |
| 0.00 | 0.99 | 0.00 | 0.96 | 19.72 | 58.72 | 59.90 | 288.78 | 0.8622 | 368.0 | 342.7 | |
| 0.00 | 2.33 | 0.00 | 2.24 | 20.30 | 58.31 | 59.50 | 289.48 | 0.8592 | 621.0 | 329.5 | |
| 0.00 | 1.17 | 0.00 | 1.07 | 19.89 | 56.44 | 57.63 | 289.15 | 0.8428 | 464.0 | 354.5 | |
| 0.00 | 3.32 | 0.00 | 2.82 | 13.93 | 53.65 | 54.84 | 282.12 | 0.8138 | 139.0 | 220.1 | |
| 0.00 | 1.17 | 0.00 | 0.94 | 17.91 | 51.24 | 52.43 | 287.23 | 0.7919 | 610.0 | 567.2 | |
| 1.17 | 1.97 | 0.95 | 1.61 | 24.31 | 50.93 | 52.12 | 295.29 | 0.7977 | -562.5 | -450.0 | |
| 0.00 | 1.97 | 0.00 | 1.57 | 22.82 | 49.94 | 51.13 | 293.62 | 0.7855 | 313.0 | 258.4 | |
| 0.00 | 1.88 | 0.00 | 1.48 | 24.95 | 48.84 | 50.03 | 296.55 | 0.7790 | 507.0 | 430.3 | |
| 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. | |