SDO HMI 2014-09-26 06:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.74 | 20.93 | 1.83 | 13.96 | 8.64 | 289.51 | 42.09 | 275.27 | 0.6664 | -463.6 | -393.1 | |
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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 |
| 0.53 | 2.65 | 0.37 | 1.87 | 5.17 | 292.96 | 45.54 | 270.43 | 0.7132 | -669.7 | -513.5 | |
| 0.00 | 1.50 | 0.00 | 1.05 | 5.28 | 292.75 | 45.34 | 270.56 | 0.7106 | -739.0 | -576.3 | |
| 0.00 | 3.09 | 0.00 | 2.15 | 7.96 | 292.47 | 45.05 | 274.34 | 0.7052 | -676.0 | -470.3 | |
| 0.00 | 2.30 | 0.00 | 1.60 | 9.92 | 292.61 | 45.19 | 277.12 | 0.7066 | -355.0 | -362.7 | |
| 0.00 | 0.88 | 0.00 | 0.59 | 13.04 | 290.23 | 42.81 | 281.76 | 0.6786 | -634.0 | -482.0 | |
| 2.21 | 4.77 | 1.46 | 3.14 | 10.95 | 288.99 | 41.57 | 278.72 | 0.6614 | -843.2 | -619.4 | |
| 0.00 | 1.94 | 0.00 | 1.26 | 11.94 | 287.94 | 40.52 | 280.32 | 0.6484 | -743.0 | -669.1 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 12.07 | 287.84 | 40.43 | 280.53 | 0.6473 | -768.0 | -653.3 | |
| 0.00 | 1.59 | 0.00 | 1.02 | 2.64 | 286.69 | 39.27 | 265.70 | 0.6364 | 315.0 | 391.3 | |
| 0.00 | 0.53 | 0.00 | 0.34 | 12.71 | 287.51 | 40.10 | 281.54 | 0.6436 | -533.0 | -513.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 7.07 | 266.34 | 18.92 | 271.60 | 0.3233 | 797.0 | 614.1 | |
| 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. | |