SDO HMI 2014-03-06 11:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.06 | 132.90 | 30.94 | 132.77 | -9.98 | 359.65 | -61.03 | 97.40 | 0.8706 | 491.2 | 246.2 | |
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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 | 3.29 | 0.00 | 3.14 | -9.67 | 1.25 | -59.43 | 96.94 | 0.8571 | 286.0 | 230.8 | |
| 16.44 | 110.66 | 16.28 | 109.09 | -10.34 | 360.00 | -60.68 | 97.79 | 0.8677 | 697.3 | 312.6 | |
| 11.68 | -2.00 | 11.51 | -2.00 | -9.55 | 0.19 | -60.49 | 96.87 | 0.8664 | 697.6 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.60 | -8.34 | 359.85 | -60.83 | 95.49 | 0.8699 | -248.0 | -160.7 | |
| 0.00 | 0.52 | 0.00 | 0.52 | -8.10 | 359.85 | -60.83 | 95.22 | 0.8701 | -291.0 | -346.3 | |
| 0.00 | 0.87 | 0.00 | 0.88 | -9.86 | 359.21 | -61.47 | 97.28 | 0.8746 | 338.0 | 275.8 | |
| 0.00 | 1.38 | 0.00 | 1.47 | -10.94 | 357.78 | -62.90 | 98.59 | 0.8858 | 507.0 | 349.9 | |
| 0.00 | 0.26 | 0.00 | 0.28 | -9.28 | 357.76 | -62.91 | 96.71 | 0.8866 | 405.0 | 434.7 | |
| 2.94 | 7.01 | 3.15 | 7.50 | -9.05 | 357.57 | -63.10 | 96.46 | 0.8883 | 396.8 | 187.4 | |
| 0.00 | 0.52 | 0.00 | 0.56 | -10.33 | 357.13 | -63.54 | 97.92 | 0.8912 | 161.0 | 149.7 | |
| 0.00 | 5.10 | 0.00 | 5.63 | -10.17 | 356.56 | -64.11 | 97.78 | 0.8956 | -326.0 | -301.6 | |
| 0.00 | 0.95 | 0.00 | 1.05 | -9.29 | 356.74 | -63.93 | 96.78 | 0.8946 | 165.0 | 74.6 | |
| 0.00 | 0.69 | 0.00 | 0.78 | -9.58 | 355.86 | -64.81 | 97.17 | 0.9012 | -483.0 | -437.8 | |
| 0.00 | 1.04 | 0.00 | 1.27 | -14.39 | 353.54 | -67.14 | 102.58 | 0.9162 | -544.0 | -470.7 | |
| 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. | |