SDO HMI 2011-08-04 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.73 | 39.06 | 10.77 | 26.75 | 18.25 | 243.35 | -42.95 | 69.73 | 0.6915 | -285.2 | -115.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.71 | 17.81 | 246.19 | -40.11 | 69.62 | 0.6567 | -720.0 | -562.8 | |
| 5.97 | 7.14 | 3.92 | 4.70 | 18.14 | 246.01 | -40.29 | 69.17 | 0.6597 | -830.1 | -613.4 | |
| 0.00 | 1.27 | 0.00 | 0.83 | 17.51 | 245.93 | -40.37 | 70.14 | 0.6590 | -751.0 | -640.9 | |
| 0.00 | 1.99 | 0.00 | 1.31 | 17.87 | 245.79 | -40.51 | 69.63 | 0.6617 | -776.0 | -589.5 | |
| 0.00 | 1.27 | 0.00 | 0.84 | 17.57 | 245.54 | -40.76 | 70.15 | 0.6641 | -702.0 | -572.1 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 17.79 | 245.43 | -40.87 | 69.86 | 0.6659 | -665.0 | -589.4 | |
| 0.00 | 1.08 | 0.00 | 0.72 | 17.80 | 245.18 | -41.12 | 69.92 | 0.6690 | -598.0 | -470.8 | |
| 0.00 | 1.18 | 0.00 | 0.78 | 17.13 | 245.36 | -40.94 | 70.86 | 0.6651 | -518.0 | -443.9 | |
| 0.00 | 1.54 | 0.00 | 1.03 | 17.97 | 244.87 | -41.43 | 69.75 | 0.6731 | -507.0 | -427.6 | |
| 0.00 | 1.08 | 0.00 | 0.73 | 18.04 | 244.55 | -41.75 | 69.74 | 0.6772 | -607.0 | -468.8 | |
| 5.33 | 6.96 | 3.68 | 4.80 | 18.36 | 242.80 | -43.51 | 69.74 | 0.6988 | -639.1 | -443.2 | |
| 0.00 | 0.63 | 0.00 | 0.45 | 19.99 | 240.88 | -45.42 | 67.96 | 0.7245 | 521.0 | 529.3 | |
| 0.00 | 1.72 | 0.00 | 1.22 | 18.67 | 240.94 | -45.37 | 69.75 | 0.7209 | 840.0 | 657.9 | |
| 0.00 | 1.90 | 0.00 | 1.36 | 19.06 | 240.66 | -45.64 | 69.28 | 0.7248 | 639.0 | 555.5 | |
| 3.07 | 3.53 | 2.19 | 2.51 | 18.13 | 240.93 | -45.37 | 70.49 | 0.7198 | 702.3 | 653.0 | |
| 1.36 | 2.35 | 0.98 | 1.70 | 18.83 | 240.14 | -46.16 | 69.71 | 0.7302 | 573.8 | 547.3 | |
| 0.00 | 2.89 | 0.00 | 2.10 | 18.66 | 239.92 | -46.38 | 69.99 | 0.7322 | 571.0 | 443.3 | |
| 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. | |