SDO HMI 2014-09-20 05:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.03 | 0.00 | 8.57 | 9.11 | 333.08 | 5.92 | 251.10 | 0.1356 | 383.2 | 86.2 | |
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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 | 3.55 | 0.00 | 1.84 | 9.21 | 344.00 | 16.84 | 278.31 | 0.2903 | -658.0 | -575.3 | |
| 0.00 | 2.66 | 0.00 | 1.35 | 9.96 | 339.45 | 12.30 | 284.01 | 0.2172 | -615.0 | -674.9 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 9.89 | 334.27 | 7.12 | 292.00 | 0.1323 | -860.0 | -676.3 | |
| 0.00 | 0.71 | 0.00 | 0.35 | 9.95 | 334.03 | 6.87 | 293.14 | 0.1288 | -689.0 | -439.6 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 7.90 | 329.08 | 1.92 | 292.40 | 0.0361 | 850.0 | 678.8 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 7.72 | 328.59 | 1.43 | 293.04 | 0.0271 | 1015.0 | 871.7 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 7.72 | 328.13 | 0.98 | 301.96 | 0.0200 | 1032.0 | 883.0 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.75 | 327.89 | 0.74 | 311.08 | 0.0170 | 953.0 | 805.8 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 7.57 | 327.71 | 0.55 | 309.70 | 0.0125 | 920.0 | 641.6 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 7.60 | 326.68 | -0.48 | 44.33 | 0.0119 | 937.0 | 715.6 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 11.99 | 320.10 | -7.05 | 54.44 | 0.1483 | 790.0 | 538.9 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 14.54 | 317.07 | -10.08 | 52.27 | 0.2152 | 924.0 | 683.2 | |
| 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. | |