SDO HMI 2014-11-08 06:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.58 | 55.07 | 17.59 | 43.85 | -5.12 | 90.99 | 50.77 | 260.45 | 0.7838 | 214.1 | 76.1 | |
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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 |
| 5.61 | 29.95 | 4.70 | 24.96 | -4.81 | 93.36 | 53.14 | 261.33 | 0.8088 | 477.8 | 347.9 | |
| 9.84 | -1.00 | 8.17 | -1.00 | -4.73 | 92.95 | 52.73 | 261.36 | 0.8045 | 797.3 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.51 | -3.48 | 91.28 | 51.07 | 262.64 | 0.7852 | 609.0 | 484.1 | |
| 2.16 | 7.85 | 1.69 | 6.13 | -5.99 | 90.03 | 49.81 | 259.20 | 0.7757 | 666.8 | 555.4 | |
| 1.90 | -4.00 | 1.48 | -4.00 | -5.72 | 89.99 | 49.78 | 259.54 | 0.7749 | 702.2 | 999999 | |
| 0.00 | 2.42 | 0.00 | 1.84 | -6.35 | 88.65 | 48.43 | 258.44 | 0.7613 | -357.0 | -277.3 | |
| 0.00 | 1.47 | 0.00 | 1.11 | -6.18 | 88.31 | 48.09 | 258.58 | 0.7572 | -539.0 | -366.6 | |
| 2.07 | 4.75 | 1.55 | 3.56 | -6.28 | 87.97 | 47.75 | 258.36 | 0.7535 | -726.7 | -510.4 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -4.85 | 86.24 | 46.02 | 259.86 | 0.7307 | -527.0 | -407.9 | |
| 0.00 | 1.12 | 0.00 | 0.80 | -4.41 | 85.77 | 45.55 | 260.36 | 0.7244 | -668.0 | -498.8 | |
| 0.00 | 2.24 | 0.00 | 1.60 | -4.58 | 85.57 | 45.35 | 260.08 | 0.7223 | -815.0 | -616.1 | |
| 0.00 | 0.60 | 0.00 | 0.43 | -4.51 | 85.35 | 45.14 | 260.13 | 0.7196 | -381.0 | -517.4 | |
| 0.00 | 1.04 | 0.00 | 0.73 | -4.50 | 85.23 | 45.01 | 260.11 | 0.7180 | -809.0 | -641.6 | |
| 0.00 | 0.95 | 0.00 | 0.62 | -8.05 | 79.66 | 39.44 | 253.34 | 0.6589 | -619.0 | -537.5 | |
| 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. | |