SDO HMI 2014-08-07 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.53 | 22.05 | 1.68 | 14.61 | -20.48 | 158.11 | -32.54 | 130.70 | 0.6664 | 363.8 | 264.6 | |
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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 | 0.65 | -16.35 | 163.74 | -26.91 | 130.60 | 0.5741 | 710.0 | 598.6 | |
| 0.00 | 1.27 | 0.00 | 0.84 | -22.60 | 160.15 | -30.49 | 134.96 | 0.6644 | 693.0 | 469.3 | |
| 0.00 | 1.54 | 0.00 | 1.00 | -20.45 | 159.60 | -31.05 | 131.91 | 0.6517 | 743.0 | 606.7 | |
| 0.00 | 2.26 | 0.00 | 1.49 | -21.21 | 159.23 | -31.42 | 132.51 | 0.6616 | 749.0 | 547.2 | |
| 0.00 | 1.54 | 0.00 | 1.00 | -20.22 | 159.34 | -31.30 | 131.42 | 0.6524 | 723.0 | 473.4 | |
| 0.00 | 0.90 | 0.00 | 0.57 | -17.28 | 159.43 | -31.21 | 127.76 | 0.6282 | 478.0 | 368.1 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -22.65 | 158.08 | -32.56 | 133.22 | 0.6839 | 528.0 | 453.5 | |
| 0.00 | 1.27 | 0.00 | 0.82 | -19.28 | 158.75 | -31.89 | 129.75 | 0.6508 | 810.0 | 663.3 | |
| 2.53 | 4.07 | 1.68 | 2.70 | -20.82 | 158.36 | -32.29 | 131.30 | 0.6668 | 774.3 | 573.6 | |
| 0.00 | 0.36 | 0.00 | 0.24 | -20.61 | 157.48 | -33.16 | 130.31 | 0.6737 | 338.0 | 426.5 | |
| 0.00 | 2.89 | 0.00 | 1.94 | -20.57 | 156.99 | -33.66 | 129.86 | 0.6783 | 30.0 | 128.3 | |
| 0.00 | 0.45 | 0.00 | 0.28 | -12.72 | 157.34 | -33.31 | 119.80 | 0.6195 | 619.0 | 588.2 | |
| 0.00 | 0.63 | 0.00 | 0.45 | -22.14 | 154.36 | -36.29 | 129.70 | 0.7148 | -650.0 | -554.9 | |
| 0.00 | 0.81 | 0.00 | 0.57 | -21.80 | 154.29 | -36.35 | 129.26 | 0.7131 | -535.0 | -423.9 | |
| 0.00 | 1.99 | 0.00 | 1.39 | -21.18 | 154.31 | -36.33 | 128.55 | 0.7087 | -833.0 | -668.0 | |
| 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. | |