SDO HMI 2014-04-10 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.11 | 36.69 | 13.67 | 43.31 | -8.24 | 26.43 | 65.64 | 263.62 | 0.9072 | 298.2 | 282.8 | |
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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 |
| 3.62 | 6.79 | 4.57 | 8.59 | -7.23 | 28.19 | 67.40 | 264.67 | 0.9215 | 452.2 | 334.7 | |
| 0.00 | 0.26 | 0.00 | 0.33 | -7.17 | 27.54 | 66.76 | 264.77 | 0.9172 | 359.0 | 367.0 | |
| 0.00 | 7.94 | 0.00 | 9.77 | -7.62 | 27.60 | 66.81 | 264.28 | 0.9174 | 581.0 | 523.6 | |
| 3.26 | 4.68 | 4.03 | 5.77 | -8.61 | 27.70 | 66.91 | 263.19 | 0.9177 | 435.0 | 405.8 | |
| 0.44 | 1.41 | 0.54 | 1.73 | -9.08 | 27.55 | 66.77 | 262.68 | 0.9166 | 474.6 | 374.4 | |
| 3.26 | 5.03 | 3.93 | 6.06 | -8.34 | 27.06 | 66.27 | 263.52 | 0.9134 | 587.1 | 431.9 | |
| 0.00 | 1.32 | 0.00 | 1.57 | -7.22 | 26.64 | 65.86 | 264.77 | 0.9108 | -314.0 | -168.5 | |
| 0.00 | 1.15 | 0.00 | 1.39 | -9.62 | 27.29 | 66.51 | 262.10 | 0.9146 | 485.0 | 359.5 | |
| 0.00 | 1.06 | 0.00 | 1.28 | -9.78 | 27.20 | 66.42 | 261.93 | 0.9139 | 495.0 | 421.8 | |
| 0.00 | 1.32 | 0.00 | 1.55 | -8.80 | 26.31 | 65.53 | 263.05 | 0.9079 | 374.0 | 335.5 | |
| 0.53 | 1.94 | 0.60 | 2.20 | -8.31 | 25.42 | 64.64 | 263.64 | 0.9015 | -242.3 | -133.4 | |
| 0.00 | 1.50 | 0.00 | 1.25 | -10.10 | 14.67 | 53.88 | 261.83 | 0.8057 | -628.0 | -473.5 | |
| 0.00 | 0.88 | 0.00 | 0.73 | -10.26 | 14.19 | 53.40 | 261.63 | 0.8008 | -165.0 | -264.6 | |
| 0.00 | 1.41 | 0.00 | 1.09 | -11.62 | 11.33 | 50.54 | 259.83 | 0.7706 | -664.0 | -519.8 | |
| 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. | |