SDO HMI 2014-07-10 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.08 | 0.00 | 6.99 | -21.12 | 220.66 | 25.09 | 220.59 | 0.6107 | -268.7 | -172.6 | |
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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 | 0.64 | 0.00 | 0.48 | -13.99 | 241.31 | 45.74 | 247.58 | 0.7540 | 610.0 | 526.0 | |
| 0.00 | 0.45 | 0.00 | 0.35 | -16.83 | 241.66 | 46.09 | 244.19 | 0.7683 | 459.0 | 387.8 | |
| 0.00 | 2.18 | 0.00 | 1.54 | -14.29 | 237.74 | 42.17 | 245.64 | 0.7164 | 563.0 | 446.3 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -17.33 | 230.77 | 35.20 | 237.56 | 0.6542 | -465.0 | -546.0 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -19.58 | 216.50 | 20.93 | 220.54 | 0.5198 | -683.0 | -473.9 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -21.91 | 216.17 | 20.60 | 217.16 | 0.5425 | -707.0 | -581.8 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -22.25 | 216.19 | 20.62 | 216.77 | 0.5465 | -723.0 | -603.4 | |
| 0.00 | 0.64 | 0.00 | 0.38 | -28.74 | 204.73 | 9.16 | 194.54 | 0.5579 | -250.0 | -230.9 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -28.70 | 204.23 | 8.66 | 193.80 | 0.5556 | -552.0 | -388.5 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -28.48 | 204.14 | 8.57 | 193.78 | 0.5522 | -528.0 | -476.5 | |
| 0.00 | 0.82 | 0.00 | 0.48 | -28.44 | 203.82 | 8.25 | 193.30 | 0.5506 | -680.0 | -571.3 | |
| 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. | |