SDO HMI 2014-08-03 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.67 | 0.00 | 10.46 | 14.06 | 258.96 | 18.71 | 296.14 | 0.3549 | 446.4 | 360.8 | |
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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 | 1.00 | 0.00 | 0.57 | 17.17 | 268.59 | 28.34 | 294.49 | 0.5004 | -595.0 | -514.1 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 15.88 | 267.60 | 27.35 | 292.58 | 0.4805 | -754.0 | -640.9 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 15.82 | 266.10 | 25.85 | 293.41 | 0.4591 | -726.0 | -594.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 9.26 | 260.74 | 20.49 | 280.55 | 0.3530 | 759.0 | 616.8 | |
| 0.00 | 2.44 | 0.00 | 1.29 | 11.72 | 260.15 | 19.90 | 287.77 | 0.3516 | 814.0 | 639.5 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 11.91 | 260.04 | 19.79 | 288.38 | 0.3505 | 582.0 | 396.7 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 9.47 | 258.89 | 18.64 | 282.01 | 0.3237 | 864.0 | 636.4 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 10.53 | 258.40 | 18.15 | 285.53 | 0.3192 | 508.0 | 558.6 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 2.87 | 257.68 | 17.43 | 260.76 | 0.3044 | 692.0 | 555.2 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 30.83 | 259.18 | 18.93 | 326.79 | 0.5107 | 721.0 | 592.3 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 13.18 | 256.72 | 16.47 | 295.27 | 0.3065 | 663.0 | 583.2 | |
| 0.00 | 2.72 | 0.00 | 1.43 | 17.59 | 257.05 | 16.80 | 306.81 | 0.3457 | 797.0 | 618.1 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 13.44 | 256.38 | 16.13 | 296.47 | 0.3031 | 701.0 | 479.5 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 12.57 | 253.32 | 13.07 | 298.15 | 0.2515 | 809.0 | 606.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.89 | 242.87 | 2.62 | 345.72 | 0.1793 | 861.0 | 583.7 | |
| 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. | |