SDO HMI 2014-12-05 21:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.28 | 0.00 | 8.95 | 16.49 | 16.75 | -19.34 | 48.26 | 0.4270 | -546.9 | -486.7 | |
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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 | 1.28 | 0.00 | 0.67 | 15.38 | 24.84 | -11.25 | 35.85 | 0.3225 | -891.0 | -619.0 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 20.81 | 22.80 | -13.28 | 31.50 | 0.4128 | -509.0 | -492.6 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 19.52 | 20.42 | -15.66 | 37.69 | 0.4180 | -787.0 | -543.4 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 17.28 | 20.05 | -16.04 | 42.07 | 0.3954 | -868.0 | -595.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 13.89 | 18.70 | -17.39 | 50.98 | 0.3750 | -984.0 | -826.5 | |
| 0.00 | 1.62 | 0.00 | 0.89 | 18.59 | 17.81 | -18.28 | 43.43 | 0.4342 | -823.0 | -624.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 7.72 | 17.68 | -18.41 | 67.53 | 0.3401 | -631.0 | -565.2 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 13.25 | 16.92 | -19.16 | 54.93 | 0.3921 | -798.0 | -727.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 13.10 | 16.61 | -19.47 | 55.67 | 0.3949 | -875.0 | -676.2 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 16.27 | 14.18 | -21.91 | 52.44 | 0.4537 | -700.0 | -540.2 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 16.36 | 13.34 | -22.75 | 53.26 | 0.4650 | -456.0 | -460.4 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 16.82 | 13.11 | -22.98 | 52.69 | 0.4717 | -719.0 | -623.8 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 19.61 | 9.29 | -26.80 | 52.05 | 0.5407 | 731.0 | 546.5 | |
| 0.00 | 0.77 | 0.00 | 0.48 | 21.31 | 4.45 | -31.64 | 53.68 | 0.6088 | 654.0 | 538.7 | |
| 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. | |