SDO HMI 2014-04-22 01:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.54 | 0.00 | 12.14 | -19.50 | 163.19 | -2.98 | 166.83 | 0.2671 | -744.4 | -656.3 | |
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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 | 4.35 | 0.00 | 2.23 | -18.82 | 170.84 | 4.67 | 197.92 | 0.2516 | -893.0 | -691.2 | |
| 0.00 | 1.60 | 0.00 | 0.84 | -23.89 | 166.91 | 0.74 | 182.09 | 0.3245 | -642.0 | -517.1 | |
| 0.00 | 1.69 | 0.00 | 0.91 | -27.79 | 166.24 | 0.08 | 180.17 | 0.3882 | -736.0 | -625.4 | |
| 0.00 | 1.42 | 0.00 | 0.71 | -9.44 | 162.74 | -3.42 | 142.48 | 0.0972 | -909.0 | -771.1 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -19.74 | 161.89 | -4.28 | 164.55 | 0.2646 | -774.0 | -596.4 | |
| 0.00 | 0.89 | 0.00 | 0.45 | -18.81 | 161.57 | -4.60 | 162.31 | 0.2510 | -344.0 | -543.1 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -19.83 | 161.54 | -4.63 | 163.44 | 0.2677 | -773.0 | -676.2 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -20.02 | 161.53 | -4.64 | 163.63 | 0.2707 | -700.0 | -556.1 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -19.58 | 161.29 | -4.88 | 162.30 | 0.2649 | -852.0 | -768.5 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -13.86 | 161.44 | -4.73 | 152.45 | 0.1739 | -883.0 | -684.0 | |
| 0.00 | 2.13 | 0.00 | 1.09 | -19.45 | 160.71 | -5.45 | 160.21 | 0.2659 | -790.0 | -642.8 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -18.17 | 159.26 | -6.91 | 153.33 | 0.2558 | -688.0 | -515.9 | |
| 0.00 | 1.33 | 0.00 | 0.67 | -10.01 | 159.33 | -6.84 | 126.62 | 0.1468 | -920.0 | -746.8 | |
| 0.00 | 3.73 | 0.00 | 1.96 | -23.39 | 158.18 | -7.99 | 157.98 | 0.3417 | -518.0 | -690.8 | |
| 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. | |