SDO HMI 2014-03-02 13:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.10 | 85.29 | 24.94 | 97.12 | 12.84 | 50.86 | -61.41 | 71.93 | 0.9019 | -222.7 | -39.0 | |
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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 |
| 14.59 | 49.12 | 15.97 | 53.72 | 12.70 | 52.03 | -60.24 | 71.77 | 0.8935 | -576.8 | -240.0 | |
| 3.28 | 5.44 | 3.67 | 6.07 | 13.41 | 51.55 | -60.72 | 71.14 | 0.8985 | -404.9 | -231.2 | |
| 0.00 | 0.78 | 0.00 | 0.89 | 13.52 | 50.87 | -61.41 | 71.22 | 0.9036 | -158.0 | -180.6 | |
| 0.00 | 1.55 | 0.00 | 1.76 | 12.93 | 51.05 | -61.22 | 71.79 | 0.9011 | -279.0 | -176.4 | |
| 0.00 | 0.86 | 0.00 | 0.98 | 12.65 | 51.04 | -61.23 | 72.10 | 0.9007 | -277.0 | -253.3 | |
| 0.00 | 4.58 | 0.00 | 5.25 | 12.73 | 50.62 | -61.65 | 72.12 | 0.9038 | 114.0 | 113.5 | |
| 0.00 | 5.44 | 0.00 | 6.32 | 13.17 | 50.37 | -61.90 | 71.73 | 0.9064 | 359.0 | 248.7 | |
| 0.00 | 1.38 | 0.00 | 1.64 | 12.42 | 49.57 | -62.70 | 72.74 | 0.9105 | 630.0 | 573.8 | |
| 0.00 | 0.86 | 0.00 | 1.06 | 12.19 | 48.58 | -63.69 | 73.24 | 0.9168 | 227.0 | 222.3 | |
| 3.71 | 5.35 | 4.63 | 6.67 | 12.63 | 48.31 | -63.96 | 72.84 | 0.9193 | 494.3 | 384.8 | |
| 0.52 | 8.03 | 0.67 | 10.32 | 13.33 | 47.62 | -64.66 | 72.27 | 0.9249 | 128.2 | 297.0 | |
| 0.00 | 1.90 | 0.00 | 2.44 | 12.87 | 47.56 | -64.72 | 72.77 | 0.9245 | 373.0 | 214.3 | |
| 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. | |