SDO HMI 2011-07-24 17:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.86 | 35.09 | 8.37 | 18.53 | 24.13 | 79.03 | 6.68 | 341.76 | 0.3468 | -627.4 | -400.1 | |
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back to the solar disc SDO HMI 2011-07-24 17:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.43 | 8.07 | 3.92 | 4.26 | 23.48 | 81.20 | 8.85 | 335.88 | 0.3469 | -876.4 | -722.6 | |
| 4.62 | 5.17 | 2.44 | 2.73 | 23.58 | 80.70 | 8.35 | 337.21 | 0.3452 | -921.8 | -709.2 | |
| 3.81 | 4.26 | 2.01 | 2.25 | 23.62 | 80.27 | 7.92 | 338.31 | 0.3430 | -951.4 | -802.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 22.53 | 79.84 | 7.49 | 338.09 | 0.3240 | -850.0 | -607.8 | |
| 0.00 | 2.45 | 0.00 | 1.28 | 22.70 | 79.41 | 7.07 | 339.40 | 0.3240 | -907.0 | -619.4 | |
| 0.00 | 2.18 | 0.00 | 1.14 | 23.08 | 79.10 | 6.75 | 340.67 | 0.3282 | -1018.0 | -771.2 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 23.37 | 79.12 | 6.77 | 340.94 | 0.3327 | -806.0 | -609.4 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 24.67 | 78.54 | 6.20 | 343.65 | 0.3500 | -716.0 | -524.9 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 23.99 | 78.41 | 6.06 | 343.38 | 0.3388 | -786.0 | -549.3 | |
| 0.00 | 2.08 | 0.00 | 1.12 | 26.85 | 77.60 | 5.25 | 347.56 | 0.3805 | -760.0 | -603.7 | |
| 0.00 | 2.54 | 0.00 | 1.34 | 25.00 | 77.24 | 4.90 | 347.17 | 0.3499 | -860.0 | -861.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 27.27 | 74.05 | 1.70 | 355.99 | 0.3789 | 702.0 | 581.0 | |
| 0.00 | 1.81 | 0.00 | 0.96 | 26.51 | 73.39 | 1.04 | 357.44 | 0.3660 | 778.0 | 650.0 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 25.73 | 71.90 | -0.45 | 1.16 | 0.3530 | 668.0 | 547.4 | |
| 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. | |