SDO HMI 2011-07-18 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.49 | 246.27 | 17.96 | 128.25 | 16.81 | 168.89 | 13.29 | 314.05 | 0.3092 | -611.4 | -378.2 | |
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back to the solar disc SDO HMI 2011-07-18 10:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.97 | 232.92 | 11.44 | 121.27 | 16.60 | 169.29 | 13.69 | 312.77 | 0.3102 | -1363.9 | -442.1 | |
| 7.35 | -1.00 | 3.82 | -1.00 | 16.26 | 169.07 | 13.46 | 312.37 | 0.3039 | -1399.0 | 999999 | |
| 1.82 | -1.00 | 0.95 | -1.00 | 16.88 | 169.08 | 13.48 | 313.89 | 0.3108 | -993.6 | 999999 | |
| 1.63 | -1.00 | 0.85 | -1.00 | 16.57 | 168.80 | 13.19 | 313.73 | 0.3040 | -1368.9 | 999999 | |
| 1.72 | -1.00 | 0.90 | -1.00 | 16.82 | 168.82 | 13.21 | 314.30 | 0.3070 | -940.3 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.21 | 167.96 | 12.36 | 314.63 | 0.2900 | -774.0 | -560.0 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 21.43 | 166.22 | 10.61 | 329.46 | 0.3389 | 889.0 | 760.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 20.29 | 165.97 | 10.37 | 328.13 | 0.3210 | 879.0 | 708.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.11 | 164.87 | 9.27 | 319.68 | 0.2413 | 776.0 | 616.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 22.86 | 164.21 | 8.61 | 336.28 | 0.3444 | 851.0 | 688.4 | |
| 0.00 | 2.36 | 0.00 | 1.25 | 23.74 | 163.83 | 8.23 | 338.24 | 0.3551 | 775.0 | 610.4 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 22.89 | 162.08 | 6.48 | 341.69 | 0.3322 | 922.0 | 728.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 21.55 | 161.56 | 5.95 | 341.70 | 0.3085 | 967.0 | 791.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 23.70 | 161.35 | 5.75 | 344.35 | 0.3414 | 702.0 | 473.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 21.87 | 160.94 | 5.34 | 343.78 | 0.3106 | 820.0 | 685.3 | |
| 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. | |