SDO HMI 2014-10-10 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.06 | 371.30 | 47.73 | 295.78 | -20.53 | 18.50 | -44.73 | 122.56 | 0.7841 | 850.4 | 213.8 | |
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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 | 0.88 | 0.00 | 0.68 | -21.86 | 20.97 | -42.26 | 125.47 | 0.7686 | -342.0 | -391.6 | |
| 0.00 | 0.61 | 0.00 | 0.47 | -20.16 | 20.62 | -42.61 | 123.29 | 0.7627 | 643.0 | 606.7 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -22.83 | 19.39 | -43.84 | 125.64 | 0.7878 | -611.0 | -545.3 | |
| 3.07 | 354.66 | 2.40 | 282.73 | -20.45 | 19.41 | -43.81 | 122.95 | 0.7754 | 988.6 | 220.6 | |
| 0.00 | 1.75 | 0.00 | 1.35 | -19.35 | 19.53 | -43.69 | 121.74 | 0.7687 | 608.0 | 485.1 | |
| 0.00 | 1.49 | 0.00 | 1.13 | -17.80 | 19.69 | -43.54 | 120.00 | 0.7597 | 636.0 | 626.4 | |
| 55.59 | -4.00 | 44.26 | -4.00 | -20.62 | 18.45 | -44.78 | 122.63 | 0.7850 | 1060.4 | 999999 | |
| 1.40 | 4.47 | 1.07 | 3.41 | -17.76 | 19.35 | -43.88 | 119.77 | 0.7628 | 657.9 | 491.6 | |
| 0.00 | 0.79 | 0.00 | 0.68 | -23.83 | 16.29 | -46.94 | 125.08 | 0.8188 | 567.0 | 414.9 | |
| 0.00 | 1.05 | 0.00 | 0.82 | -17.81 | 17.87 | -45.36 | 119.07 | 0.7773 | 261.0 | 240.4 | |
| 0.00 | 2.19 | 0.00 | 1.70 | -16.70 | 18.04 | -45.19 | 117.83 | 0.7707 | -611.0 | -535.2 | |
| 0.00 | 1.93 | 0.00 | 1.52 | -17.90 | 17.61 | -45.61 | 119.04 | 0.7801 | -453.0 | -405.4 | |
| 0.00 | 0.61 | 0.00 | 0.52 | -21.43 | 15.46 | -47.76 | 122.02 | 0.8151 | -290.0 | -320.1 | |
| 0.00 | 0.61 | 0.00 | 0.56 | -22.77 | 12.80 | -50.43 | 122.24 | 0.8425 | -475.0 | -462.9 | |
| 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. | |