SDO HMI 2014-06-06 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.37 | 0.00 | 10.98 | 5.11 | 262.91 | -21.58 | 75.23 | 0.3764 | -181.2 | 28.8 | |
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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 | 1.45 | 0.00 | 0.73 | 4.89 | 273.57 | -10.93 | 65.61 | 0.2083 | -817.0 | -660.2 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 3.19 | 273.00 | -11.49 | 74.30 | 0.2076 | -810.0 | -665.5 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 3.67 | 272.38 | -12.12 | 72.91 | 0.2202 | -736.0 | -591.8 | |
| 0.00 | 1.99 | 0.00 | 1.01 | 3.58 | 271.78 | -12.71 | 74.03 | 0.2295 | -841.0 | -624.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 5.20 | 271.41 | -13.09 | 68.02 | 0.2442 | -859.0 | -651.4 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 5.20 | 270.85 | -13.65 | 68.83 | 0.2532 | -799.0 | -642.6 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 2.37 | 270.11 | -14.39 | 80.48 | 0.2529 | -852.0 | -624.8 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 2.43 | 267.67 | -16.83 | 81.59 | 0.2937 | -780.0 | -605.8 | |
| 0.00 | 2.44 | 0.00 | 1.34 | 8.13 | 260.39 | -24.11 | 70.69 | 0.4303 | 749.0 | 616.6 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 5.74 | 259.27 | -25.23 | 76.70 | 0.4376 | 703.0 | 598.0 | |
| 0.00 | 1.90 | 0.00 | 1.06 | 5.37 | 258.10 | -26.40 | 78.02 | 0.4544 | 742.0 | 635.9 | |
| 0.00 | 2.99 | 0.00 | 1.69 | 6.41 | 255.97 | -28.53 | 76.72 | 0.4896 | 395.0 | 329.2 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 4.46 | 253.86 | -30.64 | 81.26 | 0.5161 | 664.0 | 515.2 | |
| 0.00 | 1.27 | 0.00 | 0.76 | 4.44 | 249.94 | -34.56 | 82.18 | 0.5730 | 704.0 | 501.1 | |
| 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. | |