SDO HMI 2014-01-13 19:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 102.22 | 471.33 | 52.25 | 241.14 | -16.50 | 13.02 | -8.01 | 147.76 | 0.2510 | 1091.8 | 379.0 | |
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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 | 1.61 | 0.00 | 0.83 | -18.97 | 18.14 | -2.89 | 169.26 | 0.2573 | 806.0 | 614.6 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -16.72 | 17.31 | -3.72 | 163.79 | 0.2234 | 898.0 | 758.6 | |
| 63.81 | 285.47 | 32.59 | 145.76 | -16.60 | 13.73 | -7.30 | 150.13 | 0.2455 | 1430.6 | 453.1 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -16.14 | 12.70 | -8.33 | 145.72 | 0.2483 | 864.0 | 720.7 | |
| 0.00 | 1.87 | 0.00 | 0.95 | -15.60 | 12.69 | -8.34 | 144.37 | 0.2409 | 971.0 | 706.6 | |
| 6.80 | 167.46 | 3.48 | 85.83 | -16.71 | 12.42 | -8.61 | 146.18 | 0.2587 | 1107.4 | 316.2 | |
| 0.00 | 3.14 | 0.00 | 1.60 | -15.30 | 12.49 | -8.54 | 142.95 | 0.2389 | 925.0 | 811.7 | |
| 31.61 | -6.00 | 16.18 | -6.00 | -16.25 | 12.17 | -8.86 | 144.35 | 0.2550 | 1314.5 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -15.31 | 7.38 | -13.65 | 130.03 | 0.2987 | -994.0 | -813.3 | |
| 0.00 | 1.78 | 0.00 | 0.93 | -15.30 | 7.00 | -14.03 | 129.28 | 0.3034 | -843.0 | -776.7 | |
| 0.00 | 0.76 | 0.00 | 0.40 | -15.91 | 6.13 | -14.90 | 129.26 | 0.3207 | -724.0 | -615.7 | |
| 0.00 | 1.61 | 0.00 | 0.84 | -14.91 | 5.51 | -15.52 | 125.60 | 0.3193 | -882.0 | -695.2 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -14.84 | 5.23 | -15.80 | 124.97 | 0.3225 | -903.0 | -696.0 | |
| 0.00 | 1.87 | 0.00 | 0.99 | -18.36 | 4.73 | -16.30 | 132.52 | 0.3629 | -836.0 | -745.0 | |
| 0.00 | 1.78 | 0.00 | 0.95 | -19.18 | 4.59 | -16.44 | 133.99 | 0.3733 | -877.0 | -617.0 | |
| 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. | |