SDO HMI 2014-09-24 14:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.05 | 0.00 | 14.06 | -15.46 | 246.30 | -23.13 | 134.51 | 0.5330 | -728.8 | -648.1 | |
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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 |
| 0.00 | 3.01 | 0.00 | 1.75 | -15.72 | 247.24 | -22.18 | 136.05 | 0.5258 | -802.0 | -723.3 | |
| 0.00 | 1.15 | 0.00 | 0.67 | -15.66 | 247.01 | -22.42 | 135.69 | 0.5276 | -807.0 | -673.3 | |
| 0.00 | 2.03 | 0.00 | 1.18 | -15.31 | 246.81 | -22.61 | 134.96 | 0.5261 | -826.0 | -769.5 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -15.87 | 246.71 | -22.71 | 135.60 | 0.5329 | -632.0 | -501.4 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -15.85 | 246.58 | -22.84 | 135.40 | 0.5340 | -495.0 | -500.0 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -15.17 | 246.46 | -22.97 | 134.31 | 0.5284 | -814.0 | -622.4 | |
| 0.00 | 1.50 | 0.00 | 0.88 | -15.25 | 246.21 | -23.21 | 134.11 | 0.5318 | -890.0 | -740.6 | |
| 0.00 | 2.39 | 0.00 | 1.39 | -14.76 | 246.27 | -23.16 | 133.50 | 0.5263 | -387.0 | -388.5 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -15.06 | 246.03 | -23.39 | 133.63 | 0.5318 | -887.0 | -774.7 | |
| 0.00 | 3.18 | 0.00 | 1.86 | -15.29 | 245.97 | -23.46 | 133.88 | 0.5348 | -896.0 | -801.2 | |
| 0.00 | 3.80 | 0.00 | 2.24 | -15.95 | 245.85 | -23.57 | 134.64 | 0.5425 | -792.0 | -596.0 | |
| 0.00 | 1.95 | 0.00 | 1.14 | -15.40 | 245.79 | -23.64 | 133.81 | 0.5378 | -787.0 | -693.6 | |
| 0.00 | 1.77 | 0.00 | 1.04 | -15.44 | 245.64 | -23.78 | 133.69 | 0.5397 | -460.0 | -497.0 | |
| 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. | |