SDO HMI 2014-11-30 14:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.62 | 50.17 | 7.73 | 26.47 | -19.07 | 108.24 | 2.39 | 186.50 | 0.3472 | 304.2 | 139.9 | |
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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 |
| 4.70 | 25.64 | 2.49 | 13.56 | -19.34 | 109.65 | 3.81 | 190.23 | 0.3542 | 1117.6 | 539.6 | |
| 0.00 | 1.79 | 0.00 | 0.95 | -19.59 | 109.25 | 3.40 | 189.05 | 0.3571 | 695.0 | 578.7 | |
| 6.24 | -1.00 | 3.30 | -1.00 | -19.31 | 109.21 | 3.37 | 189.09 | 0.3524 | 977.3 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.23 | -18.80 | 108.67 | 2.82 | 187.85 | 0.3429 | -717.0 | -642.8 | |
| 1.97 | 3.59 | 1.04 | 1.89 | -18.93 | 108.08 | 2.23 | 186.18 | 0.3438 | 1075.9 | 884.1 | |
| 0.00 | 2.91 | 0.00 | 1.52 | -18.24 | 107.91 | 2.07 | 185.95 | 0.3321 | -997.0 | -723.9 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -18.93 | 107.86 | 2.01 | 185.58 | 0.3434 | 549.0 | 518.3 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -18.86 | 107.70 | 1.86 | 185.16 | 0.3421 | 377.0 | 167.1 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -18.20 | 106.98 | 1.13 | 183.28 | 0.3304 | -867.0 | -658.4 | |
| 0.00 | 2.05 | 0.00 | 1.08 | -19.24 | 106.67 | 0.83 | 182.26 | 0.3472 | -794.0 | -592.0 | |
| 0.00 | 1.88 | 0.00 | 0.99 | -18.17 | 106.67 | 0.82 | 182.38 | 0.3296 | 783.0 | 571.7 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -17.70 | 106.57 | 0.73 | 182.17 | 0.3217 | 911.0 | 609.4 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -18.83 | 106.55 | 0.70 | 181.96 | 0.3404 | -791.0 | -643.2 | |
| 0.00 | 0.26 | 0.00 | 0.14 | -18.99 | 106.14 | 0.29 | 180.82 | 0.3428 | 304.0 | 387.3 | |
| 1.71 | 5.38 | 0.90 | 2.84 | -19.17 | 105.17 | -0.68 | 178.15 | 0.3460 | -979.4 | -804.2 | |
| 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. | |