SDO HMI 2014-06-08 04:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.15 | 0.00 | 8.67 | 5.85 | 255.85 | -7.11 | 94.44 | 0.2111 | 583.4 | 433.6 | |
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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 | 4.45 | 273.71 | 10.75 | 291.86 | 0.2012 | -844.0 | -671.9 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 5.19 | 272.98 | 10.01 | 296.76 | 0.1948 | -800.0 | -643.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 5.73 | 258.69 | -4.28 | 37.51 | 0.1224 | 770.0 | 620.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 11.45 | 256.91 | -6.05 | 27.85 | 0.2221 | 814.0 | 641.2 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 10.27 | 256.69 | -6.28 | 31.53 | 0.2066 | 796.0 | 558.5 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -1.82 | 256.71 | -6.25 | 107.80 | 0.1149 | 936.0 | 668.3 | |
| 0.00 | 1.81 | 0.00 | 0.91 | 1.65 | 255.00 | -7.97 | 79.53 | 0.1415 | 835.0 | 497.1 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 9.69 | 251.54 | -11.42 | 49.74 | 0.2569 | 751.0 | 645.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 8.28 | 251.49 | -11.47 | 54.40 | 0.2431 | 837.0 | 624.4 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 5.43 | 250.62 | -12.34 | 66.73 | 0.2327 | 874.0 | 689.8 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 5.00 | 250.38 | -12.58 | 68.82 | 0.2338 | 874.0 | 658.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 9.45 | 249.40 | -13.56 | 55.14 | 0.2831 | 695.0 | 532.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 8.46 | 248.55 | -14.41 | 59.65 | 0.2865 | 832.0 | 659.5 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 1.59 | 246.11 | -16.86 | 85.12 | 0.2922 | 797.0 | 631.7 | |
| 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. | |