SDO HMI 2014-05-31 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 |
| 13.09 | 32.15 | 11.08 | 27.33 | -13.76 | 62.11 | 53.27 | 253.54 | 0.8132 | -118.3 | 8.1 | |
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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 | 1.08 | 0.00 | 1.02 | -12.30 | 66.46 | 57.62 | 255.99 | 0.8525 | 519.0 | 451.3 | |
| 3.70 | 5.96 | 3.42 | 5.50 | -12.71 | 65.67 | 56.84 | 255.40 | 0.8459 | 562.9 | 377.6 | |
| 0.00 | 1.26 | 0.00 | 1.13 | -12.70 | 64.26 | 55.42 | 255.20 | 0.8329 | 535.0 | 426.2 | |
| 0.00 | 1.36 | 0.00 | 1.20 | -12.82 | 63.97 | 55.14 | 255.01 | 0.8304 | 503.0 | 479.6 | |
| 0.81 | 2.26 | 0.74 | 2.04 | -18.67 | 63.84 | 55.00 | 248.06 | 0.8387 | 450.9 | 328.9 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -18.76 | 63.66 | 54.82 | 247.91 | 0.8374 | 281.0 | 283.3 | |
| 0.00 | 1.81 | 0.00 | 1.62 | -18.67 | 63.39 | 54.55 | 247.95 | 0.8348 | 607.0 | 515.7 | |
| 8.58 | 11.38 | 6.92 | 9.18 | -13.11 | 59.98 | 51.14 | 253.93 | 0.7914 | -636.7 | -326.1 | |
| 0.00 | 0.81 | 0.00 | 0.65 | -12.30 | 59.60 | 50.77 | 254.87 | 0.7862 | -633.0 | -534.6 | |
| 0.00 | 2.44 | 0.00 | 1.94 | -12.59 | 59.38 | 50.55 | 254.47 | 0.7844 | -678.0 | -614.7 | |
| 0.00 | 0.54 | 0.00 | 0.43 | -12.68 | 59.07 | 50.23 | 254.29 | 0.7812 | -511.0 | -610.8 | |
| 0.00 | 1.26 | 0.00 | 1.00 | -12.78 | 58.95 | 50.11 | 254.14 | 0.7801 | -767.0 | -651.6 | |
| 0.00 | 1.72 | 0.00 | 1.38 | -14.49 | 59.45 | 50.61 | 252.09 | 0.7886 | -203.0 | -230.4 | |
| 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. | |