SDO HMI 2014-09-07 15:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.71 | 33.17 | 10.35 | 32.12 | -20.49 | 80.04 | -53.27 | 119.12 | 0.8609 | 200.0 | 31.7 | |
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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 | 0.98 | 0.00 | 0.86 | -21.31 | 84.66 | -48.65 | 122.07 | 0.8274 | 480.0 | 360.9 | |
| 1.43 | 2.85 | 1.30 | 2.61 | -20.58 | 82.53 | -50.78 | 120.28 | 0.8419 | 594.8 | 490.2 | |
| 0.80 | 1.78 | 0.74 | 1.64 | -20.30 | 82.05 | -51.26 | 119.75 | 0.8447 | 539.6 | 431.4 | |
| 1.61 | 2.59 | 1.49 | 2.39 | -20.55 | 81.88 | -51.43 | 119.95 | 0.8470 | 233.8 | 183.6 | |
| 0.00 | 0.27 | 0.00 | 0.25 | -21.08 | 81.36 | -51.95 | 120.29 | 0.8530 | 303.0 | 416.7 | |
| 0.00 | 1.34 | 0.00 | 1.18 | -17.88 | 82.64 | -50.67 | 117.34 | 0.8309 | 543.0 | 375.7 | |
| 0.00 | 1.16 | 0.00 | 1.11 | -21.22 | 80.97 | -52.34 | 120.27 | 0.8566 | 510.0 | 418.4 | |
| 0.00 | 0.98 | 0.00 | 0.93 | -20.73 | 81.16 | -52.15 | 119.83 | 0.8533 | 401.0 | 331.3 | |
| 0.00 | 0.89 | 0.00 | 0.86 | -21.62 | 80.71 | -52.60 | 120.59 | 0.8600 | 132.0 | 232.1 | |
| 0.00 | 2.50 | 0.00 | 2.44 | -21.42 | 80.06 | -53.25 | 120.10 | 0.8642 | 561.0 | 477.9 | |
| 3.39 | 5.08 | 3.30 | 4.95 | -20.98 | 80.07 | -53.24 | 119.63 | 0.8626 | 376.6 | 237.7 | |
| 0.00 | 0.62 | 0.00 | 0.69 | -24.04 | 77.00 | -56.31 | 121.62 | 0.8943 | 307.0 | 273.6 | |
| 0.00 | 1.16 | 0.00 | 1.15 | -19.98 | 79.05 | -54.26 | 118.15 | 0.8671 | -558.0 | -569.2 | |
| 3.48 | 10.97 | 3.52 | 11.06 | -19.91 | 78.13 | -55.18 | 117.71 | 0.8738 | -447.0 | -454.8 | |
| 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. | |