SDO HMI 2011-05-31 19:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.87 | 194.32 | 24.78 | 146.38 | -20.16 | 20.00 | -45.93 | 116.48 | 0.7556 | 443.9 | 255.0 | |
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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 | 1.17 | 0.00 | 0.83 | -19.02 | 23.29 | -42.63 | 116.32 | 0.7167 | -654.0 | -596.2 | |
| 0.00 | 4.97 | 0.00 | 3.48 | -17.71 | 23.56 | -42.36 | 114.68 | 0.7087 | -890.0 | -596.7 | |
| 0.00 | 1.35 | 0.00 | 0.95 | -17.45 | 23.59 | -42.33 | 114.34 | 0.7074 | -692.0 | -591.9 | |
| 0.00 | 1.26 | 0.00 | 0.90 | -19.50 | 22.96 | -42.96 | 116.81 | 0.7221 | -549.0 | -518.7 | |
| 1.35 | 2.71 | 0.95 | 1.91 | -17.87 | 23.26 | -42.67 | 114.76 | 0.7127 | -615.9 | -479.5 | |
| 0.00 | 2.08 | 0.00 | 1.49 | -18.79 | 22.40 | -43.53 | 115.64 | 0.7256 | -696.0 | -521.2 | |
| 0.00 | 0.99 | 0.00 | 0.72 | -19.36 | 22.16 | -43.76 | 116.30 | 0.7302 | -587.0 | -480.2 | |
| 3.79 | 13.73 | 2.76 | 10.00 | -18.55 | 21.53 | -44.39 | 115.00 | 0.7341 | -671.5 | -197.2 | |
| 0.00 | 1.72 | 0.00 | 1.26 | -18.97 | 20.85 | -45.08 | 115.28 | 0.7428 | 682.0 | 541.9 | |
| 0.00 | 0.90 | 0.00 | 0.67 | -18.80 | 20.49 | -45.43 | 114.94 | 0.7460 | 479.0 | 392.9 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -21.67 | 19.35 | -46.58 | 118.13 | 0.7677 | 233.0 | 199.6 | |
| 22.85 | 162.45 | 17.32 | 123.41 | -20.41 | 19.72 | -46.21 | 116.69 | 0.7595 | 1014.0 | 356.8 | |
| 4.88 | -12.00 | 3.75 | -12.00 | -20.69 | 19.08 | -46.84 | 116.81 | 0.7669 | 678.2 | 999999 | |
| 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. | |