SDO HMI 2014-05-29 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.13 | 48.55 | 11.30 | 27.03 | -19.69 | 50.47 | 19.56 | 223.89 | 0.4563 | 101.0 | -3.6 | |
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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 | 1.08 | 0.00 | 0.61 | -18.76 | 54.00 | 23.08 | 230.44 | 0.4834 | 716.0 | 617.2 | |
| 14.53 | 21.58 | 8.23 | 12.21 | -19.31 | 53.76 | 22.85 | 229.26 | 0.4856 | 988.8 | 734.6 | |
| 0.00 | 1.99 | 0.00 | 1.09 | -14.85 | 53.09 | 22.18 | 236.57 | 0.4390 | 685.0 | 555.8 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -19.32 | 50.89 | 19.97 | 225.61 | 0.4530 | -611.0 | -573.4 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -20.48 | 50.77 | 19.85 | 223.55 | 0.4636 | 825.0 | 734.6 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -20.29 | 50.64 | 19.72 | 223.68 | 0.4602 | 547.0 | 470.6 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -20.51 | 50.53 | 19.61 | 223.17 | 0.4614 | 821.0 | 664.2 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -19.59 | 48.84 | 17.93 | 222.21 | 0.4335 | -973.0 | -883.5 | |
| 5.60 | 8.76 | 3.07 | 4.81 | -19.81 | 48.60 | 17.68 | 221.46 | 0.4334 | -996.9 | -710.9 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -19.63 | 46.29 | 15.37 | 217.94 | 0.4077 | -808.0 | -615.6 | |
| 0.00 | 1.53 | 0.00 | 0.83 | -19.76 | 45.90 | 14.98 | 217.05 | 0.4055 | -933.0 | -789.8 | |
| 0.00 | 1.90 | 0.00 | 1.03 | -21.87 | 42.38 | 11.46 | 207.33 | 0.4032 | -792.0 | -624.0 | |
| 0.00 | 1.35 | 0.00 | 0.73 | -22.62 | 40.86 | 9.95 | 203.38 | 0.4036 | -618.0 | -469.3 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -22.10 | 40.29 | 9.38 | 202.73 | 0.3924 | -746.0 | -605.1 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -23.87 | 39.71 | 8.79 | 199.77 | 0.4151 | -737.0 | -633.2 | |
| 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. | |