SDO HMI 2014-07-10 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.98 | 0.00 | 10.60 | -22.72 | 198.57 | 0.26 | 181.73 | 0.4593 | -45.9 | 129.0 | |
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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 |
| 0.00 | 1.27 | 0.00 | 0.69 | -18.40 | 204.99 | 6.68 | 196.27 | 0.3956 | 576.0 | 443.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -22.04 | 204.42 | 6.11 | 192.74 | 0.4490 | 736.0 | 676.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -22.04 | 203.92 | 5.61 | 191.74 | 0.4473 | 869.0 | 628.1 | |
| 0.00 | 5.81 | 0.00 | 3.22 | -22.03 | 203.56 | 5.25 | 191.00 | 0.4462 | 879.0 | 711.0 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -22.58 | 203.51 | 5.20 | 190.66 | 0.4544 | 667.0 | 552.1 | |
| 0.00 | 1.73 | 0.00 | 0.95 | -22.11 | 196.45 | -1.87 | 176.06 | 0.4405 | -630.0 | -516.0 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -20.76 | 195.91 | -2.40 | 174.62 | 0.4199 | -803.0 | -627.1 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.77 | 193.72 | -4.59 | 169.81 | 0.4247 | -725.0 | -534.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -20.50 | 193.70 | -4.61 | 169.64 | 0.4206 | -658.0 | -539.7 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -21.89 | 191.61 | -6.71 | 165.97 | 0.4490 | -793.0 | -567.7 | |
| 0.00 | 2.18 | 0.00 | 1.35 | -30.88 | 184.57 | -13.74 | 160.26 | 0.6057 | -623.0 | -494.5 | |
| 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. | |