SDO HMI 2011-07-01 22:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.54 | 32.05 | 4.92 | 16.55 | 16.12 | 22.96 | 9.02 | 326.83 | 0.2789 | -80.6 | -29.5 | |
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back to the solar disc SDO HMI 2011-07-01 22:59:11 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.82 | 5.81 | 0.94 | 3.00 | 13.49 | 26.59 | 12.65 | 310.93 | 0.2830 | 1068.6 | 794.8 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 15.65 | 25.39 | 11.45 | 319.19 | 0.2936 | -857.0 | -724.7 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.34 | 25.43 | 11.49 | 320.64 | 0.3026 | -800.0 | -541.9 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 15.59 | 25.22 | 11.28 | 319.45 | 0.2911 | -891.0 | -711.9 | |
| 0.00 | 1.73 | 0.00 | 0.90 | 16.56 | 24.86 | 10.92 | 322.52 | 0.2996 | -911.0 | -693.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.70 | 23.67 | 9.73 | 325.88 | 0.2898 | -1008.0 | -884.9 | |
| 0.00 | 2.54 | 0.00 | 1.31 | 15.89 | 22.70 | 8.76 | 326.95 | 0.2696 | -1029.0 | -776.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.27 | 22.40 | 8.45 | 328.62 | 0.2722 | -875.0 | -693.1 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.43 | 21.89 | 7.95 | 330.47 | 0.2702 | -870.0 | -648.5 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 17.85 | 21.27 | 7.33 | 334.79 | 0.2864 | 491.0 | 254.7 | |
| 1.54 | 1.91 | 0.80 | 0.98 | 17.38 | 20.96 | 7.02 | 334.99 | 0.2771 | 744.2 | 810.5 | |
| 2.91 | 4.54 | 1.50 | 2.34 | 17.00 | 20.88 | 6.94 | 334.62 | 0.2708 | 969.4 | 842.4 | |
| 3.27 | 3.72 | 1.68 | 1.91 | 16.66 | 20.55 | 6.61 | 335.12 | 0.2632 | 960.7 | 905.2 | |
| 0.00 | 3.36 | 0.00 | 1.73 | 17.50 | 20.52 | 6.57 | 336.58 | 0.2760 | 879.0 | 659.9 | |
| 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. | |