SDO HMI 2014-09-29 02:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 33.07 | 0.53 | 16.41 | 7.80 | 207.58 | -2.44 | 120.83 | 0.0478 | -157.6 | 217.8 | |
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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 | 1.41 | 0.00 | 0.70 | 7.35 | 210.52 | 0.50 | 316.83 | 0.0127 | -976.0 | -733.2 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.71 | 210.06 | 0.05 | 357.02 | 0.0156 | -940.0 | -779.9 | |
| 0.00 | 2.73 | 0.00 | 1.35 | 7.41 | 209.61 | -0.41 | 34.42 | 0.0125 | -1088.0 | -887.8 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 6.93 | 209.40 | -0.62 | 79.86 | 0.0110 | -790.0 | -628.9 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 7.68 | 208.37 | -1.65 | 62.20 | 0.0324 | -1024.0 | -731.9 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 6.48 | 208.01 | -2.01 | 99.63 | 0.0355 | -810.0 | -606.7 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.20 | 207.91 | -2.10 | 79.62 | 0.0372 | -1140.0 | -943.5 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 7.11 | 207.76 | -2.25 | 82.56 | 0.0395 | -890.0 | -738.5 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.74 | 207.31 | -2.71 | 71.03 | 0.0498 | 719.0 | 519.8 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 6.30 | 207.22 | -2.80 | 100.56 | 0.0495 | 792.0 | 633.5 | |
| 0.00 | 1.59 | 0.00 | 0.79 | 8.70 | 207.09 | -2.93 | 56.94 | 0.0606 | 827.0 | 675.7 | |
| 0.00 | 11.29 | 0.00 | 5.60 | 8.04 | 206.79 | -3.23 | 69.04 | 0.0600 | 769.0 | 834.3 | |
| 1.06 | 3.53 | 0.53 | 1.75 | 8.67 | 206.54 | -3.48 | 61.63 | 0.0685 | 1179.0 | 883.0 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 7.71 | 206.49 | -3.53 | 75.65 | 0.0633 | 945.0 | 746.0 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 8.52 | 206.36 | -3.66 | 64.75 | 0.0701 | 691.0 | 548.1 | |
| 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. | |