SDO HMI 2011-10-14 09:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.86 | 77.38 | 12.23 | 43.39 | 19.92 | 98.50 | 24.89 | 302.42 | 0.4707 | -267.7 | -370.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.40 | 6.12 | 0.79 | 3.46 | 20.22 | 99.56 | 25.95 | 301.99 | 0.4861 | -717.6 | -609.6 | |
| 0.00 | 0.52 | 0.00 | 0.30 | 19.08 | 99.33 | 25.72 | 300.04 | 0.4756 | -178.0 | -151.8 | |
| 11.02 | 47.65 | 6.20 | 26.82 | 19.58 | 99.23 | 25.62 | 301.07 | 0.4777 | -974.8 | -483.4 | |
| 0.00 | 3.32 | 0.00 | 1.87 | 20.08 | 99.18 | 25.57 | 302.06 | 0.4803 | -685.0 | -650.0 | |
| 3.06 | -3.00 | 1.72 | -3.00 | 19.57 | 98.88 | 25.27 | 301.34 | 0.4729 | -1043.3 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.03 | 20.00 | 98.92 | 25.31 | 302.13 | 0.4763 | -863.0 | -680.7 | |
| 0.00 | 1.66 | 0.00 | 0.93 | 19.80 | 98.36 | 24.75 | 302.26 | 0.4677 | -927.0 | -862.7 | |
| 0.00 | 1.84 | 0.00 | 1.02 | 19.67 | 97.08 | 23.47 | 303.21 | 0.4501 | -872.0 | -741.4 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 23.10 | 96.97 | 23.36 | 309.72 | 0.4760 | 680.0 | 577.5 | |
| 4.98 | 5.86 | 2.76 | 3.24 | 21.04 | 96.09 | 22.48 | 306.90 | 0.4481 | 917.5 | 644.6 | |
| 0.00 | 1.75 | 0.00 | 0.96 | 20.40 | 95.92 | 22.31 | 305.84 | 0.4407 | 819.0 | 566.7 | |
| 0.00 | 2.45 | 0.00 | 1.35 | 20.90 | 95.75 | 22.14 | 307.00 | 0.4427 | 812.0 | 733.2 | |
| 0.00 | 1.22 | 0.00 | 0.67 | 20.36 | 95.36 | 21.75 | 306.38 | 0.4333 | 646.0 | 457.1 | |
| 1.40 | 2.01 | 0.76 | 1.10 | 20.48 | 94.55 | 20.94 | 307.56 | 0.4242 | 996.8 | 652.1 | |
| 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. | |