SDO HMI 2014-09-11 11:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.65 | 203.99 | 22.22 | 114.78 | -15.81 | 66.26 | -16.43 | 144.95 | 0.4747 | 435.0 | 277.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.36 | 1.78 | 0.20 | 0.99 | -16.27 | 69.29 | -13.39 | 150.65 | 0.4556 | -795.0 | -661.7 | |
| 0.00 | 1.07 | 0.00 | 0.56 | -8.19 | 69.56 | -13.13 | 139.44 | 0.3472 | 731.0 | 592.2 | |
| 0.00 | 1.96 | 0.00 | 1.08 | -14.57 | 69.15 | -13.54 | 148.39 | 0.4340 | -933.0 | -740.0 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -15.30 | 68.94 | -13.75 | 148.88 | 0.4453 | -751.0 | -596.5 | |
| 0.00 | 1.25 | 0.00 | 0.70 | -15.92 | 67.93 | -14.76 | 147.80 | 0.4617 | 844.0 | 737.0 | |
| 0.00 | 2.32 | 0.00 | 1.29 | -15.82 | 67.87 | -14.82 | 147.59 | 0.4610 | 605.0 | 525.2 | |
| 0.00 | 1.60 | 0.00 | 0.90 | -16.19 | 67.68 | -15.01 | 147.69 | 0.4673 | 579.0 | 391.7 | |
| 6.15 | 165.32 | 3.44 | 92.67 | -15.71 | 67.20 | -15.49 | 146.29 | 0.4652 | 1059.6 | 374.2 | |
| 2.32 | -8.00 | 1.29 | -8.00 | -15.52 | 67.05 | -15.64 | 145.80 | 0.4641 | 1317.9 | 999999 | |
| 2.85 | -8.00 | 1.60 | -8.00 | -15.92 | 66.98 | -15.71 | 146.18 | 0.4696 | 849.5 | 999999 | |
| 4.99 | -8.00 | 2.80 | -8.00 | -15.82 | 66.80 | -15.89 | 145.75 | 0.4701 | 1032.3 | 999999 | |
| 22.18 | -8.00 | 12.43 | -8.00 | -15.67 | 66.61 | -16.08 | 145.25 | 0.4697 | 1128.2 | 999999 | |
| 0.00 | 3.74 | 0.00 | 2.11 | -14.81 | 64.20 | -18.49 | 140.28 | 0.4818 | 666.0 | 574.1 | |
| 0.00 | 5.34 | 0.00 | 3.04 | -15.73 | 64.08 | -18.61 | 141.33 | 0.4936 | 668.0 | 554.7 | |
| 0.00 | 1.43 | 0.00 | 0.81 | -16.06 | 63.98 | -18.71 | 141.61 | 0.4984 | 585.0 | 507.2 | |
| 0.00 | 1.34 | 0.00 | 0.78 | -18.43 | 63.55 | -19.14 | 143.90 | 0.5299 | 755.0 | 585.3 | |
| 0.00 | 0.89 | 0.00 | 0.51 | -15.97 | 63.06 | -19.63 | 140.15 | 0.5061 | -637.0 | -445.0 | |
| 0.00 | 1.78 | 0.00 | 1.02 | -15.59 | 62.76 | -19.93 | 139.22 | 0.5047 | -812.0 | -647.3 | |
| 0.80 | 1.87 | 0.46 | 1.08 | -15.96 | 61.78 | -20.91 | 138.36 | 0.5184 | -850.4 | -737.4 | |
| 0.00 | 2.49 | 0.00 | 1.46 | -17.29 | 61.59 | -21.09 | 139.82 | 0.5347 | -815.0 | -623.3 | |
| 0.00 | 2.41 | 0.00 | 1.42 | -18.05 | 60.99 | -21.70 | 139.97 | 0.5488 | -927.0 | -744.5 | |
| 0.00 | 1.34 | 0.00 | 0.78 | -16.36 | 61.13 | -21.56 | 138.01 | 0.5291 | -747.0 | -537.1 | |
| 0.00 | 1.43 | 0.00 | 0.84 | -17.77 | 60.68 | -22.01 | 139.23 | 0.5486 | -697.0 | -556.2 | |
| 0.00 | 0.71 | 0.00 | 0.44 | -22.16 | 59.56 | -23.13 | 142.92 | 0.6056 | 690.0 | 567.2 | |
| 0.00 | 0.98 | 0.00 | 0.59 | -18.44 | 59.83 | -22.85 | 139.00 | 0.5638 | -758.0 | -554.2 | |
| 0.00 | 0.98 | 0.00 | 0.59 | -19.47 | 59.44 | -23.25 | 139.75 | 0.5782 | -532.0 | -479.0 | |
| 0.00 | 0.89 | 0.00 | 0.53 | -18.49 | 59.52 | -23.17 | 138.67 | 0.5673 | -702.0 | -612.2 | |
| 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. | |