SDO HMI 2014-09-18 02:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.49 | 0.00 | 9.23 | 7.59 | 336.47 | -18.73 | 86.41 | 0.3188 | -43.4 | 4.1 | |
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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 | 1.51 | 0.00 | 0.76 | 10.01 | 345.54 | -9.66 | 72.73 | 0.1738 | 782.0 | 616.4 | |
| 0.00 | 2.22 | 0.00 | 1.12 | 7.29 | 345.12 | -10.08 | 88.66 | 0.1745 | -995.0 | -613.2 | |
| 0.00 | 1.69 | 0.00 | 0.85 | 6.77 | 344.85 | -10.35 | 91.57 | 0.1793 | -912.0 | -665.1 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 8.37 | 343.48 | -11.72 | 83.32 | 0.2033 | -861.0 | -748.1 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 8.77 | 342.69 | -12.51 | 81.79 | 0.2173 | -957.0 | -729.8 | |
| 0.00 | 1.24 | 0.00 | 0.64 | 10.93 | 339.06 | -16.14 | 75.54 | 0.2831 | -860.0 | -693.8 | |
| 0.00 | 0.62 | 0.00 | 0.33 | 6.39 | 335.43 | -19.77 | 91.07 | 0.3377 | -607.0 | -452.9 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 4.87 | 335.10 | -20.11 | 95.43 | 0.3455 | 501.0 | 413.1 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 7.68 | 329.43 | -25.77 | 87.18 | 0.4332 | 803.0 | 561.2 | |
| 0.00 | 1.69 | 0.00 | 0.93 | 7.58 | 328.79 | -26.41 | 87.38 | 0.4431 | 640.0 | 488.4 | |
| 0.00 | 1.60 | 0.00 | 0.90 | 7.96 | 326.88 | -28.32 | 86.52 | 0.4726 | 662.0 | 549.7 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 8.14 | 326.80 | -28.40 | 86.14 | 0.4738 | 647.0 | 502.4 | |
| 0.00 | 1.33 | 0.00 | 0.75 | 4.28 | 326.95 | -28.25 | 94.31 | 0.4752 | 593.0 | 608.2 | |
| 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. | |