SDO HMI 2014-04-10 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.71 | 42.29 | 14.57 | 45.77 | -8.66 | 25.65 | 63.22 | 263.26 | 0.8885 | 187.9 | 184.5 | |
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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 |
| 3.00 | 6.09 | 3.54 | 7.18 | -7.32 | 28.08 | 65.65 | 264.69 | 0.9093 | 460.4 | 399.2 | |
| 2.03 | 6.26 | 2.32 | 7.18 | -7.84 | 27.35 | 64.92 | 264.15 | 0.9038 | 526.2 | 479.4 | |
| 3.00 | 5.21 | 3.45 | 6.00 | -8.64 | 27.53 | 65.10 | 263.25 | 0.9048 | 381.0 | 232.0 | |
| 0.88 | 3.26 | 1.01 | 3.74 | -9.21 | 27.35 | 64.92 | 262.64 | 0.9033 | 523.5 | 386.6 | |
| 3.09 | 6.53 | 3.49 | 7.36 | -8.42 | 26.95 | 64.52 | 263.53 | 0.9006 | 590.9 | 456.4 | |
| 0.00 | 1.59 | 0.00 | 1.77 | -7.22 | 26.47 | 64.04 | 264.89 | 0.8974 | -116.0 | -147.9 | |
| 0.00 | 1.24 | 0.00 | 1.38 | -9.70 | 26.66 | 64.24 | 262.12 | 0.8980 | 248.0 | 299.1 | |
| 0.00 | 1.06 | 0.00 | 1.16 | -8.74 | 26.14 | 63.71 | 263.21 | 0.8943 | 408.0 | 382.2 | |
| 0.71 | 1.59 | 0.76 | 1.71 | -8.31 | 25.53 | 63.10 | 263.72 | 0.8897 | -197.8 | -157.9 | |
| 0.00 | 3.18 | 0.00 | 3.28 | -10.52 | 24.30 | 61.87 | 261.26 | 0.8792 | 128.0 | 178.8 | |
| 0.00 | 1.15 | 0.00 | 0.96 | -13.28 | 16.47 | 54.04 | 257.90 | 0.8079 | -487.0 | -401.1 | |
| 0.00 | 1.15 | 0.00 | 0.92 | -9.64 | 14.72 | 52.29 | 262.42 | 0.7891 | -498.0 | -424.9 | |
| 0.00 | 1.15 | 0.00 | 0.92 | -10.22 | 14.65 | 52.22 | 261.68 | 0.7883 | -558.0 | -529.8 | |
| 0.00 | 1.15 | 0.00 | 0.91 | -10.32 | 14.27 | 51.84 | 261.56 | 0.7843 | -632.0 | -521.5 | |
| 0.00 | 1.68 | 0.00 | 1.30 | -10.65 | 13.17 | 50.74 | 261.12 | 0.7725 | -671.0 | -562.5 | |
| 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. | |