SDO HMI 2014-06-06 04:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.01 | 0.00 | 10.47 | 4.25 | 265.67 | -23.77 | 78.03 | 0.4062 | -326.5 | -323.5 | |
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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 | 2.08 | 0.00 | 1.08 | 4.28 | 273.47 | -15.97 | 74.58 | 0.2858 | -1073.0 | -869.0 | |
| 0.00 | 3.17 | 0.00 | 1.64 | 6.30 | 273.29 | -16.15 | 68.18 | 0.2991 | -960.0 | -657.7 | |
| 0.00 | 1.90 | 0.00 | 0.98 | 4.04 | 273.12 | -16.31 | 75.70 | 0.2904 | -826.0 | -719.2 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 3.18 | 272.82 | -16.62 | 78.80 | 0.2923 | -872.0 | -717.6 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 4.01 | 272.77 | -16.66 | 76.08 | 0.2960 | -860.0 | -695.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 2.97 | 270.32 | -19.11 | 80.81 | 0.3326 | -984.0 | -717.8 | |
| 0.00 | 2.44 | 0.00 | 1.28 | 2.49 | 270.01 | -19.43 | 82.39 | 0.3367 | -860.0 | -675.9 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 3.13 | 268.11 | -21.32 | 81.29 | 0.3689 | -743.0 | -602.6 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 6.27 | 255.35 | -34.08 | 78.83 | 0.5700 | 618.0 | 507.6 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 0.99 | 254.61 | -34.83 | 88.18 | 0.5734 | 709.0 | 556.7 | |
| 0.00 | 1.81 | 0.00 | 1.11 | 7.34 | 254.22 | -35.22 | 77.32 | 0.5884 | 619.0 | 516.2 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 10.06 | 251.65 | -37.79 | 73.78 | 0.6306 | 524.0 | 469.2 | |
| 0.00 | 1.00 | 0.00 | 0.70 | 1.37 | 243.92 | -45.51 | 88.01 | 0.7159 | 464.0 | 401.4 | |
| 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. | |