SDO HMI 2014-12-11 12:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.33 | 258.70 | 28.99 | 165.34 | -4.04 | 1.10 | 39.12 | 264.15 | 0.6350 | 911.2 | 339.5 | |
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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 | 1.70 | 0.00 | 1.09 | -1.58 | 1.50 | 39.51 | 268.04 | 0.6387 | -805.0 | -646.3 | |
| 1.11 | 242.85 | 0.71 | 155.47 | -4.60 | 1.51 | 39.53 | 263.31 | 0.6410 | 745.1 | 353.2 | |
| 29.31 | -2.00 | 18.82 | -2.00 | -4.16 | 1.37 | 39.38 | 263.99 | 0.6387 | 1106.6 | 999999 | |
| 11.84 | -2.00 | 7.54 | -2.00 | -3.95 | 0.82 | 38.84 | 264.25 | 0.6311 | 1282.4 | 999999 | |
| 1.79 | 3.66 | 1.13 | 2.32 | -2.74 | 0.43 | 38.44 | 266.14 | 0.6247 | 810.0 | 608.1 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -3.22 | 359.13 | 37.14 | 265.25 | 0.6072 | 648.0 | 606.4 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -5.05 | 359.19 | 37.21 | 262.24 | 0.6102 | 624.0 | 490.3 | |
| 0.00 | 1.28 | 0.00 | 0.79 | -3.60 | 359.04 | 37.05 | 264.61 | 0.6063 | 800.0 | 634.2 | |
| 1.28 | 2.56 | 0.79 | 1.58 | -1.95 | 358.68 | 36.70 | 267.32 | 0.6001 | 717.3 | 544.4 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -4.93 | 358.81 | 36.83 | 262.37 | 0.6048 | 697.0 | 549.2 | |
| 0.00 | 1.62 | 0.00 | 1.00 | -2.54 | 358.51 | 36.53 | 266.32 | 0.5981 | -733.0 | -594.0 | |
| 0.00 | 1.53 | 0.00 | 0.94 | -3.34 | 358.07 | 36.08 | 264.93 | 0.5925 | -635.0 | -544.2 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -2.49 | 356.05 | 34.06 | 266.20 | 0.5629 | 605.0 | 433.6 | |
| 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. | |