SDO HMI 2014-08-11 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.15 | 67.96 | 11.46 | 42.84 | -17.87 | 161.54 | 29.82 | 229.96 | 0.6208 | 692.0 | 464.2 | |
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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 |
| 16.43 | 43.78 | 10.38 | 27.61 | -17.07 | 162.38 | 30.66 | 231.78 | 0.6227 | 927.0 | 498.4 | |
| 1.72 | -1.00 | 1.08 | -1.00 | -16.98 | 161.92 | 30.20 | 231.49 | 0.6171 | 970.0 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.98 | -18.60 | 161.89 | 30.17 | 229.36 | 0.6300 | 635.0 | 595.2 | |
| 0.00 | 3.43 | 0.00 | 2.17 | -18.59 | 161.19 | 29.47 | 228.72 | 0.6227 | 782.0 | 687.3 | |
| 0.00 | 1.99 | 0.00 | 1.25 | -18.45 | 161.01 | 29.29 | 228.74 | 0.6196 | 759.0 | 537.5 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -19.58 | 160.94 | 29.22 | 227.24 | 0.6286 | 586.0 | 368.0 | |
| 0.00 | 1.62 | 0.00 | 1.01 | -17.32 | 160.48 | 28.76 | 229.69 | 0.6045 | 714.0 | 643.2 | |
| 0.00 | 1.62 | 0.00 | 1.03 | -20.04 | 160.62 | 28.90 | 226.38 | 0.6294 | 666.0 | 500.9 | |
| 0.00 | 1.62 | 0.00 | 1.03 | -19.68 | 160.37 | 28.64 | 226.57 | 0.6238 | 723.0 | 630.5 | |
| 0.00 | 1.99 | 0.00 | 1.26 | -19.92 | 160.38 | 28.65 | 226.29 | 0.6260 | 692.0 | 561.9 | |
| 0.00 | 3.25 | 0.00 | 2.04 | -19.52 | 159.86 | 28.14 | 226.27 | 0.6173 | 811.0 | 697.9 | |
| 0.00 | 1.81 | 0.00 | 1.14 | -20.48 | 159.49 | 27.77 | 224.73 | 0.6224 | 871.0 | 650.7 | |
| 0.00 | 1.08 | 0.00 | 0.67 | -18.83 | 159.00 | 27.28 | 226.27 | 0.6026 | 600.0 | 425.8 | |
| 0.00 | 1.17 | 0.00 | 0.73 | -19.92 | 158.04 | 26.32 | 223.90 | 0.6033 | -673.0 | -570.3 | |
| 0.00 | 2.26 | 0.00 | 1.40 | -20.60 | 157.33 | 25.61 | 222.33 | 0.6031 | -910.0 | -699.8 | |
| 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. | |