SDO HMI 2014-09-26 07:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.65 | 18.74 | 1.74 | 12.03 | 7.15 | 207.17 | -39.70 | 87.19 | 0.6366 | -61.6 | -1.1 | |
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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 | 1.24 | 0.00 | 0.76 | 6.85 | 210.45 | -36.42 | 87.84 | 0.5920 | -728.0 | -552.5 | |
| 0.00 | 1.15 | 0.00 | 0.71 | 5.84 | 209.78 | -37.09 | 89.48 | 0.6022 | -683.0 | -526.8 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 6.37 | 209.58 | -37.28 | 88.59 | 0.6044 | -838.0 | -645.3 | |
| 0.00 | 1.41 | 0.00 | 0.88 | 6.94 | 209.50 | -37.37 | 87.64 | 0.6053 | -642.0 | -468.8 | |
| 0.00 | 0.71 | 0.00 | 0.44 | 5.71 | 209.60 | -37.27 | 89.69 | 0.6048 | -547.0 | -467.2 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 6.66 | 209.44 | -37.42 | 88.09 | 0.6062 | -515.0 | -402.3 | |
| 0.00 | 1.77 | 0.00 | 1.12 | 6.91 | 207.91 | -38.95 | 87.57 | 0.6269 | -709.0 | -429.0 | |
| 0.00 | 0.88 | 0.00 | 0.58 | 7.76 | 206.00 | -40.87 | 86.14 | 0.6521 | 613.0 | 558.8 | |
| 0.00 | 0.88 | 0.00 | 0.58 | 8.91 | 205.53 | -41.33 | 84.37 | 0.6580 | 603.0 | 510.0 | |
| 2.65 | 5.57 | 1.74 | 3.66 | 7.03 | 205.52 | -41.35 | 87.23 | 0.6588 | 737.7 | 560.3 | |
| 0.00 | 1.24 | 0.00 | 0.82 | 8.73 | 204.90 | -41.97 | 84.62 | 0.6662 | 710.0 | 581.3 | |
| 0.00 | 1.41 | 0.00 | 0.94 | 8.20 | 204.60 | -42.26 | 85.42 | 0.6701 | 667.0 | 549.8 | |
| 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. | |