SDO HMI 2014-08-06 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.08 | 25.76 | 1.53 | 19.01 | -21.15 | 157.26 | -40.02 | 126.01 | 0.7427 | 216.1 | 95.8 | |
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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 | 1.27 | 0.00 | 0.82 | -17.50 | 164.73 | -32.55 | 126.88 | 0.6438 | 633.0 | 509.8 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -18.90 | 163.08 | -34.20 | 127.34 | 0.6712 | 370.0 | 271.0 | |
| 0.00 | 2.89 | 0.00 | 2.08 | -22.80 | 159.99 | -37.29 | 129.70 | 0.7282 | 616.0 | 461.9 | |
| 0.00 | 0.63 | 0.00 | 0.46 | -21.31 | 157.83 | -39.45 | 126.51 | 0.7388 | 221.0 | 316.6 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -17.92 | 158.73 | -38.55 | 123.03 | 0.7096 | 523.0 | 462.3 | |
| 2.08 | 6.06 | 1.53 | 4.45 | -21.26 | 157.59 | -39.69 | 126.29 | 0.7408 | 679.0 | 592.4 | |
| 0.00 | 0.81 | 0.00 | 0.60 | -21.51 | 157.33 | -39.95 | 126.43 | 0.7447 | 434.0 | 307.4 | |
| 0.00 | 0.72 | 0.00 | 0.52 | -19.19 | 157.68 | -39.60 | 123.91 | 0.7277 | 471.0 | 332.2 | |
| 0.00 | 1.45 | 0.00 | 1.08 | -21.57 | 156.54 | -40.74 | 125.99 | 0.7524 | 323.0 | 330.2 | |
| 0.00 | 1.08 | 0.00 | 0.83 | -22.34 | 155.39 | -41.89 | 126.17 | 0.7673 | -362.0 | -408.4 | |
| 0.00 | 4.16 | 0.00 | 3.13 | -20.91 | 155.81 | -41.47 | 124.78 | 0.7555 | -3.0 | 68.1 | |
| 0.00 | 3.53 | 0.00 | 2.72 | -21.49 | 154.81 | -42.47 | 124.86 | 0.7679 | -658.0 | -561.0 | |
| 0.00 | 1.99 | 0.00 | 1.53 | -21.20 | 154.65 | -42.63 | 124.43 | 0.7678 | -683.0 | -583.8 | |
| 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. | |