SDO HMI 2014-10-05 20:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.32 | 0.00 | 11.33 | -18.73 | 101.63 | -19.33 | 144.50 | 0.5320 | 183.7 | 17.8 | |
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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 | 0.97 | 0.00 | 0.54 | -19.90 | 110.96 | -10.00 | 159.76 | 0.4739 | 663.0 | 540.1 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -22.79 | 110.45 | -10.50 | 160.97 | 0.5175 | 697.0 | 569.5 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -14.75 | 110.74 | -10.22 | 154.56 | 0.4010 | 724.0 | 607.5 | |
| 0.00 | 1.67 | 0.00 | 0.98 | -24.18 | 108.60 | -12.36 | 158.96 | 0.5461 | 729.0 | 546.1 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -15.34 | 109.16 | -11.80 | 151.91 | 0.4206 | 826.0 | 680.0 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -16.02 | 106.30 | -14.66 | 147.34 | 0.4525 | 720.0 | 567.1 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -17.37 | 106.09 | -14.86 | 148.58 | 0.4717 | 748.0 | 586.1 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -17.11 | 106.02 | -14.94 | 148.15 | 0.4689 | 925.0 | 768.8 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -16.95 | 105.77 | -15.19 | 147.55 | 0.4689 | 853.0 | 675.8 | |
| 0.00 | 3.07 | 0.00 | 1.80 | -17.57 | 99.45 | -21.51 | 138.87 | 0.5335 | -890.0 | -755.6 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -18.79 | 96.53 | -24.42 | 136.85 | 0.5745 | -751.0 | -624.2 | |
| 0.00 | 1.23 | 0.00 | 0.79 | -22.56 | 93.22 | -27.74 | 137.77 | 0.6418 | -645.0 | -464.8 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -20.27 | 93.15 | -27.80 | 135.02 | 0.6214 | -590.0 | -487.9 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -19.07 | 90.73 | -30.23 | 131.23 | 0.6349 | -674.0 | -577.7 | |
| 0.00 | 1.58 | 0.00 | 1.01 | -17.51 | 89.42 | -31.53 | 128.08 | 0.6359 | -579.0 | -517.1 | |
| 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. | |