SDO HMI 2014-11-02 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.50 | 23.48 | 2.49 | 13.65 | -17.65 | 97.39 | -22.49 | 136.05 | 0.5200 | -274.6 | -72.8 | |
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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 | 3.72 | 0.00 | 2.06 | -16.34 | 103.04 | -16.84 | 141.48 | 0.4481 | 958.0 | 823.3 | |
| 4.50 | 7.79 | 2.49 | 4.32 | -16.22 | 102.73 | -17.15 | 140.79 | 0.4497 | 978.5 | 763.0 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -19.30 | 97.75 | -22.12 | 138.00 | 0.5333 | -725.0 | -572.5 | |
| 0.00 | 0.87 | 0.00 | 0.51 | -17.54 | 94.21 | -25.67 | 131.43 | 0.5531 | -750.0 | -612.0 | |
| 0.00 | 1.30 | 0.00 | 0.78 | -18.77 | 93.94 | -25.94 | 132.86 | 0.5672 | -876.0 | -750.1 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -17.74 | 94.00 | -25.88 | 131.50 | 0.5572 | -722.0 | -616.5 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -18.78 | 93.69 | -26.19 | 132.61 | 0.5699 | -777.0 | -654.6 | |
| 0.00 | 0.52 | 0.00 | 0.31 | -17.50 | 93.41 | -26.47 | 130.54 | 0.5615 | -675.0 | -564.5 | |
| 0.00 | 1.64 | 0.00 | 0.99 | -17.64 | 93.25 | -26.63 | 130.57 | 0.5644 | -663.0 | -478.6 | |
| 0.00 | 1.39 | 0.00 | 0.85 | -19.33 | 91.79 | -28.09 | 131.43 | 0.5949 | -739.0 | -622.1 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -17.04 | 91.91 | -27.97 | 128.39 | 0.5743 | -634.0 | -462.9 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -19.57 | 91.45 | -28.42 | 131.43 | 0.6004 | -244.0 | -280.7 | |
| 0.00 | 1.13 | 0.00 | 0.74 | -23.93 | 88.86 | -31.02 | 134.50 | 0.6627 | -656.0 | -498.4 | |
| 0.00 | 1.13 | 0.00 | 0.70 | -17.76 | 88.94 | -30.93 | 126.72 | 0.6130 | -187.0 | -232.6 | |
| 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. | |