SDO HMI 2014-10-15 18:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.87 | 413.29 | 39.41 | 258.94 | -21.26 | 16.85 | 26.71 | 223.22 | 0.6142 | 919.6 | 318.6 | |
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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 | 1.22 | 0.00 | 0.76 | -19.85 | 17.13 | 26.99 | 225.26 | 0.6033 | 704.0 | 538.3 | |
| 31.78 | 401.84 | 19.99 | 251.93 | -21.22 | 17.36 | 27.22 | 223.81 | 0.6182 | 1135.6 | 335.9 | |
| 29.43 | -2.00 | 18.38 | -2.00 | -21.06 | 16.79 | 26.65 | 223.42 | 0.6112 | 1369.0 | 999999 | |
| 0.79 | -2.00 | 0.49 | -2.00 | -21.45 | 16.61 | 26.47 | 222.77 | 0.6133 | 909.0 | 999999 | |
| 0.87 | -2.00 | 0.55 | -2.00 | -21.51 | 16.48 | 26.34 | 222.55 | 0.6127 | 781.6 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -21.86 | 14.66 | 24.52 | 220.16 | 0.5994 | 708.0 | 596.5 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -22.44 | 14.58 | 24.45 | 219.43 | 0.6046 | 679.0 | 546.5 | |
| 0.00 | 1.31 | 0.00 | 0.77 | -19.54 | 10.93 | 20.79 | 218.38 | 0.5409 | -651.0 | -481.4 | |
| 0.00 | 0.96 | 0.00 | 0.58 | -23.04 | 10.51 | 20.37 | 213.88 | 0.5769 | -679.0 | -515.7 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -25.60 | 7.71 | 17.58 | 207.77 | 0.5868 | -621.0 | -489.6 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -28.33 | 7.52 | 17.38 | 205.25 | 0.6187 | -14.0 | -52.8 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -27.84 | 4.76 | 14.62 | 202.03 | 0.5974 | -518.0 | -504.2 | |
| 0.00 | 1.22 | 0.00 | 0.76 | -28.91 | 4.17 | 14.03 | 200.52 | 0.6080 | -487.0 | -385.1 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -28.29 | 3.95 | 13.81 | 200.63 | 0.5989 | -771.0 | -574.8 | |
| 0.00 | 1.14 | 0.00 | 0.70 | -28.35 | 3.71 | 13.57 | 200.26 | 0.5986 | -719.0 | -588.4 | |
| 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. | |