SDO HMI 2014-11-01 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.92 | 26.41 | 5.36 | 16.72 | -17.17 | 98.34 | -31.99 | 125.41 | 0.6194 | -38.9 | -118.0 | |
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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 | 1.04 | 0.00 | 0.62 | -17.02 | 104.04 | -26.29 | 130.11 | 0.5560 | -638.0 | -394.0 | |
| 3.55 | 13.85 | 2.13 | 8.33 | -16.15 | 102.46 | -27.87 | 127.27 | 0.5665 | 993.6 | 688.2 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -15.97 | 102.21 | -28.12 | 126.77 | 0.5679 | 729.0 | 590.8 | |
| 5.37 | -2.00 | 3.23 | -2.00 | -16.26 | 102.09 | -28.24 | 127.08 | 0.5716 | 781.4 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.55 | -15.89 | 96.99 | -33.34 | 122.28 | 0.6275 | -570.0 | -439.1 | |
| 0.00 | 1.21 | 0.00 | 0.79 | -17.46 | 96.08 | -34.26 | 123.75 | 0.6482 | -634.0 | -519.1 | |
| 0.00 | 0.87 | 0.00 | 0.58 | -18.81 | 94.49 | -35.84 | 124.41 | 0.6741 | -726.0 | -493.3 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -17.06 | 94.29 | -36.04 | 121.97 | 0.6654 | -660.0 | -560.0 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -18.15 | 93.45 | -36.89 | 122.85 | 0.6812 | -537.0 | -484.0 | |
| 0.00 | 0.61 | 0.00 | 0.41 | -17.19 | 93.45 | -36.89 | 121.59 | 0.6755 | -330.0 | -350.3 | |
| 0.00 | 0.95 | 0.00 | 0.67 | -19.59 | 91.58 | -38.75 | 123.49 | 0.7094 | -487.0 | -544.8 | |
| 0.00 | 1.82 | 0.00 | 1.28 | -19.90 | 91.25 | -39.09 | 123.66 | 0.7146 | -594.0 | -476.0 | |
| 0.00 | 1.21 | 0.00 | 0.83 | -16.73 | 91.82 | -38.51 | 119.96 | 0.6907 | -300.0 | -428.4 | |
| 0.00 | 1.04 | 0.00 | 0.76 | -21.02 | 89.73 | -40.60 | 124.11 | 0.7360 | -568.0 | -493.8 | |
| 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. | |