SDO HMI 2014-03-30 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.35 | 0.00 | 12.14 | 4.40 | 139.64 | 32.07 | 288.23 | 0.5593 | 24.2 | 1.1 | |
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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 | 2.02 | 0.00 | 1.24 | 4.33 | 142.26 | 34.69 | 286.67 | 0.5947 | -442.0 | -512.6 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 4.69 | 142.18 | 34.60 | 287.30 | 0.5950 | -672.0 | -477.5 | |
| 0.00 | 2.37 | 0.00 | 1.46 | 5.05 | 142.09 | 34.51 | 287.92 | 0.5954 | -632.0 | -582.2 | |
| 0.00 | 1.67 | 0.00 | 1.01 | 3.05 | 141.69 | 34.12 | 284.85 | 0.5817 | -614.0 | -533.4 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 4.59 | 141.08 | 33.51 | 287.71 | 0.5798 | -642.0 | -534.6 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 7.06 | 140.82 | 33.24 | 291.85 | 0.5884 | -600.0 | -485.4 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 6.43 | 140.59 | 33.01 | 290.99 | 0.5821 | -671.0 | -479.5 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 5.86 | 139.44 | 31.87 | 290.78 | 0.5639 | -424.0 | -367.9 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 2.98 | 138.63 | 31.05 | 286.31 | 0.5388 | 762.0 | 627.8 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 3.44 | 138.64 | 31.07 | 287.11 | 0.5411 | 585.0 | 401.5 | |
| 0.00 | 2.02 | 0.00 | 1.18 | 4.59 | 137.61 | 30.04 | 289.78 | 0.5323 | 759.0 | 642.9 | |
| 0.00 | 1.67 | 0.00 | 0.96 | 2.27 | 137.49 | 29.92 | 285.66 | 0.5196 | 777.0 | 608.4 | |
| 0.00 | 1.75 | 0.00 | 1.02 | 4.37 | 137.39 | 29.82 | 289.52 | 0.5281 | 753.0 | 684.2 | |
| 0.00 | 0.96 | 0.00 | 0.56 | 3.86 | 137.09 | 29.52 | 288.81 | 0.5214 | 793.0 | 624.5 | |
| 0.00 | 1.05 | 0.00 | 0.61 | 5.22 | 135.82 | 28.24 | 292.17 | 0.5109 | 631.0 | 498.8 | |
| 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. | |