SDO HMI 2014-03-02 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.50 | 79.59 | 15.86 | 47.30 | -7.74 | 151.47 | 33.73 | 266.93 | 0.5530 | 419.5 | 288.1 | |
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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 | 1.21 | 0.00 | 0.73 | -7.17 | 153.09 | 35.35 | 267.83 | 0.5767 | 490.0 | 415.3 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -6.83 | 152.74 | 34.99 | 268.44 | 0.5718 | -248.0 | -226.1 | |
| 0.00 | 1.81 | 0.00 | 1.09 | -8.15 | 152.27 | 34.53 | 266.14 | 0.5645 | 608.0 | 499.2 | |
| 26.50 | 62.15 | 15.86 | 37.21 | -7.77 | 152.16 | 34.42 | 266.82 | 0.5631 | 891.0 | 440.5 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -8.95 | 152.28 | 34.53 | 264.71 | 0.5646 | -359.0 | -293.9 | |
| 0.00 | 2.33 | 0.00 | 1.39 | -8.35 | 151.96 | 34.22 | 265.79 | 0.5601 | 259.0 | 351.5 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -7.62 | 150.42 | 32.67 | 267.18 | 0.5379 | 586.0 | 455.9 | |
| 0.00 | 1.99 | 0.00 | 1.14 | -7.80 | 148.49 | 30.75 | 266.90 | 0.5093 | -726.0 | -534.7 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -8.55 | 146.54 | 28.80 | 265.41 | 0.4799 | 721.0 | 611.3 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -9.48 | 145.42 | 27.68 | 263.37 | 0.4632 | -617.0 | -462.7 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -6.19 | 145.09 | 27.35 | 270.54 | 0.4586 | -489.0 | -427.4 | |
| 0.00 | 1.47 | 0.00 | 0.82 | -6.02 | 144.88 | 27.14 | 270.94 | 0.4556 | -705.0 | -544.5 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -5.98 | 144.54 | 26.80 | 271.08 | 0.4504 | -699.0 | -547.7 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -5.76 | 144.36 | 26.62 | 271.62 | 0.4479 | -846.0 | -741.5 | |
| 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. | |