SDO HMI 2014-04-10 09:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.98 | 33.87 | 12.61 | 41.31 | -8.14 | 26.75 | 66.51 | 263.69 | 0.9137 | 258.5 | 242.7 | |
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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 |
| 3.18 | 7.23 | 4.12 | 9.38 | -7.22 | 28.28 | 68.04 | 264.63 | 0.9258 | 459.2 | 306.0 | |
| 0.00 | 5.03 | 0.00 | 6.37 | -7.55 | 27.74 | 67.50 | 264.31 | 0.9221 | 596.0 | 523.1 | |
| 0.00 | 1.15 | 0.00 | 1.44 | -7.17 | 27.54 | 67.30 | 264.73 | 0.9209 | 371.0 | 354.8 | |
| 3.71 | 6.18 | 4.69 | 7.82 | -8.58 | 27.77 | 67.53 | 263.19 | 0.9219 | 411.8 | 245.2 | |
| 0.00 | 1.32 | 0.00 | 1.66 | -9.09 | 27.56 | 67.32 | 262.65 | 0.9203 | 551.0 | 413.0 | |
| 0.00 | 0.79 | 0.00 | 0.97 | -7.01 | 26.71 | 66.47 | 264.96 | 0.9153 | -181.0 | -69.9 | |
| 3.09 | 4.76 | 3.80 | 5.87 | -8.31 | 27.04 | 66.80 | 263.52 | 0.9171 | 598.4 | 414.3 | |
| 0.00 | 0.97 | 0.00 | 1.20 | -9.73 | 27.18 | 66.94 | 261.96 | 0.9175 | 460.0 | 418.5 | |
| 0.00 | 0.97 | 0.00 | 1.17 | -8.02 | 26.56 | 66.32 | 263.86 | 0.9138 | 361.0 | 401.1 | |
| 0.00 | 1.76 | 0.00 | 2.04 | -8.32 | 25.38 | 65.14 | 263.60 | 0.9052 | -212.0 | -189.1 | |
| 0.00 | 1.06 | 0.00 | 1.23 | -9.18 | 25.60 | 65.36 | 262.64 | 0.9065 | -193.0 | -148.2 | |
| 0.00 | 1.24 | 0.00 | 1.04 | -10.08 | 14.69 | 54.45 | 261.85 | 0.8114 | -601.0 | -528.4 | |
| 0.00 | 0.53 | 0.00 | 0.43 | -10.64 | 13.12 | 52.88 | 261.15 | 0.7953 | -553.0 | -502.2 | |
| 0.00 | 0.88 | 0.00 | 0.69 | -11.57 | 11.30 | 51.06 | 259.91 | 0.7763 | -592.0 | -528.5 | |
| 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. | |