SDO HMI 2011-09-02 02:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.15 | 164.84 | 16.49 | 87.08 | 13.69 | 291.58 | 19.75 | 290.16 | 0.3514 | -578.4 | -450.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.38 | 14.60 | 293.32 | 21.50 | 291.13 | 0.3818 | -728.0 | -515.6 | |
| 0.00 | 1.43 | 0.00 | 0.77 | 14.39 | 293.27 | 21.44 | 290.64 | 0.3800 | -718.0 | -599.2 | |
| 7.34 | 151.77 | 3.89 | 80.24 | 13.20 | 291.99 | 20.16 | 288.41 | 0.3552 | -1025.1 | -519.2 | |
| 8.23 | -3.00 | 4.36 | -3.00 | 14.02 | 291.89 | 20.07 | 290.72 | 0.3575 | -931.1 | 999999 | |
| 1.97 | -3.00 | 1.04 | -3.00 | 13.24 | 291.69 | 19.87 | 288.74 | 0.3509 | -1199.3 | 999999 | |
| 11.28 | -3.00 | 5.97 | -3.00 | 13.57 | 291.72 | 19.90 | 289.64 | 0.3528 | -1123.8 | 999999 | |
| 2.33 | -3.00 | 1.23 | -3.00 | 13.25 | 291.40 | 19.57 | 288.99 | 0.3464 | -1260.3 | 999999 | |
| 0.00 | 2.60 | 0.00 | 1.37 | 13.58 | 290.90 | 19.07 | 290.30 | 0.3402 | -695.0 | -625.7 | |
| 0.00 | 1.16 | 0.00 | 0.60 | 15.19 | 287.75 | 15.93 | 298.43 | 0.3025 | 862.0 | 635.5 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 15.62 | 287.56 | 15.73 | 300.00 | 0.3029 | 627.0 | 524.8 | |
| 0.00 | 1.43 | 0.00 | 0.74 | 15.32 | 287.50 | 15.68 | 299.17 | 0.2998 | 809.0 | 635.4 | |
| 0.00 | 1.34 | 0.00 | 0.70 | 16.16 | 287.04 | 15.22 | 302.35 | 0.2998 | 811.0 | 614.4 | |
| 0.00 | 1.34 | 0.00 | 0.70 | 16.63 | 286.79 | 14.96 | 304.12 | 0.3002 | 953.0 | 767.2 | |
| 0.00 | 2.24 | 0.00 | 1.16 | 16.29 | 286.73 | 14.90 | 303.25 | 0.2965 | 889.0 | 695.8 | |
| 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. | |