SDO HMI 2014-11-02 22:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.91 | 0.00 | 11.49 | -19.86 | 78.84 | -31.70 | 129.09 | 0.6366 | 509.4 | 447.1 | |
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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 |
| 0.00 | 1.04 | 0.00 | 0.60 | -17.31 | 87.32 | -23.22 | 133.83 | 0.5239 | -648.0 | -419.3 | |
| 0.00 | 1.04 | 0.00 | 0.63 | -20.88 | 84.77 | -25.77 | 135.78 | 0.5847 | 758.0 | 656.8 | |
| 0.00 | 2.68 | 0.00 | 1.62 | -19.62 | 84.47 | -26.07 | 133.82 | 0.5759 | 507.0 | 456.5 | |
| 0.00 | 0.52 | 0.00 | 0.32 | -19.87 | 81.13 | -29.41 | 130.85 | 0.6127 | 638.0 | 578.8 | |
| 0.00 | 0.86 | 0.00 | 0.55 | -20.00 | 79.38 | -31.16 | 129.46 | 0.6321 | 746.0 | 625.0 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -21.64 | 78.39 | -32.15 | 130.72 | 0.6549 | 61.0 | 124.4 | |
| 0.00 | 0.86 | 0.00 | 0.57 | -20.04 | 76.85 | -33.68 | 127.46 | 0.6587 | 696.0 | 608.9 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -20.34 | 76.70 | -33.84 | 127.73 | 0.6624 | 673.0 | 473.2 | |
| 0.00 | 2.08 | 0.00 | 1.37 | -20.11 | 76.61 | -33.93 | 127.37 | 0.6619 | 628.0 | 507.2 | |
| 0.00 | 1.21 | 0.00 | 0.80 | -20.00 | 76.17 | -34.36 | 126.90 | 0.6656 | 501.0 | 411.6 | |
| 0.00 | 1.73 | 0.00 | 1.14 | -19.45 | 76.16 | -34.38 | 126.17 | 0.6620 | 714.0 | 518.2 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -19.75 | 75.97 | -34.57 | 126.42 | 0.6660 | 743.0 | 666.9 | |
| 0.00 | 1.82 | 0.00 | 1.21 | -19.66 | 75.72 | -34.82 | 126.13 | 0.6680 | 617.0 | 503.3 | |
| 0.00 | 0.95 | 0.00 | 0.63 | -19.70 | 75.52 | -35.02 | 126.03 | 0.6704 | 497.0 | 429.7 | |
| 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. | |