SDO HMI 2014-06-05 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.43 | 0.00 | 12.56 | 4.04 | 268.68 | -26.84 | 80.52 | 0.4556 | -360.1 | -446.0 | |
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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 | 3.26 | 0.00 | 1.75 | 4.22 | 273.30 | -22.23 | 78.65 | 0.3864 | -631.0 | -647.2 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 5.81 | 273.17 | -22.35 | 74.72 | 0.3938 | -873.0 | -685.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 4.01 | 273.07 | -22.45 | 79.30 | 0.3893 | -773.0 | -624.2 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 3.76 | 273.04 | -22.48 | 79.93 | 0.3891 | -880.0 | -711.8 | |
| 0.00 | 1.81 | 0.00 | 0.98 | 5.93 | 272.90 | -22.62 | 74.59 | 0.3985 | -885.0 | -690.8 | |
| 0.00 | 2.62 | 0.00 | 1.41 | 3.43 | 272.85 | -22.67 | 80.86 | 0.3913 | -1012.0 | -805.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 3.77 | 270.95 | -24.57 | 80.72 | 0.4222 | -692.0 | -608.9 | |
| 0.00 | 5.52 | 0.00 | 3.03 | 3.16 | 270.22 | -25.30 | 82.36 | 0.4323 | -588.0 | -682.9 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 1.80 | 265.47 | -30.05 | 86.18 | 0.5037 | -787.0 | -585.4 | |
| 0.00 | 0.90 | 0.00 | 0.56 | 5.84 | 259.12 | -36.40 | 80.04 | 0.6016 | 769.0 | 660.9 | |
| 0.00 | 0.99 | 0.00 | 0.62 | 5.51 | 258.42 | -37.10 | 80.75 | 0.6106 | 683.0 | 640.3 | |
| 0.00 | 0.63 | 0.00 | 0.40 | 4.99 | 257.29 | -38.23 | 81.80 | 0.6251 | 549.0 | 505.3 | |
| 0.00 | 1.27 | 0.00 | 0.85 | 4.05 | 253.55 | -41.97 | 83.80 | 0.6733 | 439.0 | 405.4 | |
| 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. | |