SDO HMI 2014-11-07 10:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.93 | 19.17 | 1.90 | 12.20 | -15.87 | 17.29 | -33.93 | 121.37 | 0.6284 | -252.0 | -222.3 | |
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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 | 1.04 | 0.00 | 0.60 | -14.55 | 25.42 | -25.80 | 126.10 | 0.5234 | 796.0 | 687.7 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -14.00 | 24.77 | -26.45 | 124.57 | 0.5269 | 715.0 | 611.2 | |
| 0.00 | 1.90 | 0.00 | 1.11 | -13.04 | 23.59 | -27.63 | 121.89 | 0.5343 | 387.0 | 401.7 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -14.03 | 22.69 | -28.52 | 122.69 | 0.5526 | 625.0 | 488.9 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -18.24 | 18.65 | -32.57 | 125.47 | 0.6300 | 502.0 | 460.3 | |
| 0.00 | 1.04 | 0.00 | 0.67 | -17.24 | 16.31 | -34.91 | 122.38 | 0.6495 | -518.0 | -447.2 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -16.48 | 16.36 | -34.86 | 121.37 | 0.6442 | -792.0 | -666.2 | |
| 0.00 | 1.47 | 0.00 | 0.95 | -16.58 | 16.19 | -35.03 | 121.39 | 0.6468 | -797.0 | -749.6 | |
| 0.00 | 1.04 | 0.00 | 0.68 | -17.16 | 15.91 | -35.31 | 121.99 | 0.6535 | -636.0 | -522.0 | |
| 2.93 | 4.66 | 1.90 | 3.02 | -16.18 | 16.01 | -35.21 | 120.71 | 0.6464 | -890.2 | -686.0 | |
| 0.00 | 0.69 | 0.00 | 0.46 | -18.82 | 15.17 | -36.05 | 123.70 | 0.6718 | -658.0 | -555.9 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -16.73 | 15.62 | -35.60 | 121.21 | 0.6541 | -449.0 | -416.0 | |
| 0.00 | 1.38 | 0.00 | 0.90 | -15.93 | 15.14 | -36.07 | 119.80 | 0.6548 | -507.0 | -371.9 | |
| 0.00 | 0.86 | 0.00 | 0.60 | -16.11 | 10.72 | -40.50 | 117.46 | 0.7055 | -490.0 | -439.8 | |
| 0.00 | 0.78 | 0.00 | 0.56 | -15.65 | 8.30 | -42.92 | 115.65 | 0.7297 | -493.0 | -353.9 | |
| 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. | |