SDO HMI 2014-01-11 12:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.45 | 437.89 | 42.21 | 278.52 | -16.27 | 13.67 | -37.56 | 110.96 | 0.6288 | 894.4 | 312.0 | |
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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 |
| 40.46 | 427.97 | 25.50 | 271.46 | -16.32 | 14.32 | -36.91 | 111.27 | 0.6208 | 1213.1 | 332.5 | |
| 0.93 | -1.00 | 0.59 | -1.00 | -16.42 | 13.87 | -37.36 | 111.26 | 0.6269 | 759.6 | 999999 | |
| 1.78 | -1.00 | 1.14 | -1.00 | -16.22 | 13.45 | -37.78 | 110.79 | 0.6315 | 1138.8 | 999999 | |
| 2.38 | -1.00 | 1.52 | -1.00 | -16.37 | 13.37 | -37.85 | 111.00 | 0.6329 | 921.6 | 999999 | |
| 18.53 | -1.00 | 11.87 | -1.00 | -16.11 | 13.08 | -38.14 | 110.50 | 0.6358 | 980.9 | 999999 | |
| 1.61 | -1.00 | 1.04 | -1.00 | -16.09 | 12.58 | -38.65 | 110.29 | 0.6421 | 435.1 | 999999 | |
| 0.00 | 1.10 | 0.00 | 0.73 | -18.05 | 10.91 | -40.31 | 112.62 | 0.6688 | 458.0 | 368.2 | |
| 0.00 | 1.44 | 0.00 | 1.01 | -16.55 | 7.46 | -43.77 | 109.41 | 0.7054 | -655.0 | -570.4 | |
| 0.00 | 2.04 | 0.00 | 1.43 | -14.49 | 6.82 | -44.41 | 106.38 | 0.7085 | -680.0 | -482.5 | |
| 0.00 | 1.10 | 0.00 | 0.81 | -19.36 | 5.08 | -46.14 | 112.60 | 0.7392 | -692.0 | -483.1 | |
| 0.00 | 1.02 | 0.00 | 0.75 | -19.06 | 4.56 | -46.67 | 112.05 | 0.7441 | -619.0 | -478.8 | |
| 0.76 | 2.12 | 0.55 | 1.52 | -15.42 | 5.66 | -45.57 | 107.43 | 0.7239 | -716.8 | -599.5 | |
| 0.00 | 1.10 | 0.00 | 0.81 | -17.31 | 4.45 | -46.78 | 109.70 | 0.7413 | -474.0 | -426.6 | |
| 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. | |