SDO HMI 2011-06-01 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.69 | 68.52 | 11.83 | 37.61 | 17.08 | 40.94 | -18.37 | 44.35 | 0.4310 | -215.8 | -88.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.78 | 19.61 | 47.04 | -12.27 | 30.03 | 0.4017 | 927.0 | 745.9 | |
| 9.13 | 21.33 | 4.95 | 11.56 | 17.34 | 43.36 | -15.95 | 40.36 | 0.4068 | -1106.8 | -482.0 | |
| 2.89 | 9.40 | 1.57 | 5.09 | 16.92 | 43.13 | -16.18 | 41.46 | 0.4043 | -1127.7 | -857.3 | |
| 1.81 | -3.00 | 0.98 | -3.00 | 16.73 | 43.05 | -16.26 | 41.93 | 0.4030 | -1093.6 | 999999 | |
| 2.08 | 4.52 | 1.12 | 2.44 | 16.45 | 42.78 | -16.53 | 42.89 | 0.4027 | -822.5 | -823.8 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 15.53 | 41.80 | -17.51 | 46.16 | 0.4036 | -912.0 | -779.2 | |
| 3.25 | 11.12 | 1.77 | 6.05 | 15.98 | 41.26 | -18.05 | 46.18 | 0.4146 | -999.9 | -681.1 | |
| 0.00 | 7.32 | 0.00 | 4.11 | 17.55 | 37.64 | -21.67 | 48.46 | 0.4722 | 896.0 | 779.9 | |
| 0.00 | 1.90 | 0.00 | 1.06 | 17.30 | 37.61 | -21.70 | 48.94 | 0.4702 | 665.0 | 725.1 | |
| 0.00 | 2.26 | 0.00 | 1.29 | 19.23 | 36.27 | -23.04 | 47.43 | 0.5039 | 911.0 | 745.6 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 16.99 | 35.75 | -23.56 | 51.66 | 0.4894 | 882.0 | 718.4 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 16.29 | 35.36 | -23.96 | 53.28 | 0.4882 | 675.0 | 498.3 | |
| 2.53 | 2.89 | 1.44 | 1.65 | 16.96 | 35.13 | -24.18 | 52.40 | 0.4966 | 794.0 | 866.2 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 17.22 | 34.92 | -24.40 | 52.20 | 0.5013 | 693.0 | 613.4 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 17.96 | 34.07 | -25.24 | 51.88 | 0.5177 | 636.0 | 479.9 | |
| 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. | |