SDO HMI 2014-11-01 00:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.06 | 29.63 | 5.15 | 19.55 | -16.55 | 99.88 | -35.93 | 121.60 | 0.6603 | 208.7 | 202.4 | |
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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 | 1.65 | 0.00 | 1.03 | -16.97 | 104.14 | -31.66 | 125.16 | 0.6164 | -652.0 | -506.4 | |
| 0.00 | 1.30 | 0.00 | 0.83 | -16.41 | 102.41 | -33.40 | 123.02 | 0.6321 | 579.0 | 537.9 | |
| 2.34 | 3.90 | 1.49 | 2.48 | -16.13 | 102.28 | -33.53 | 122.54 | 0.6318 | 993.4 | 814.8 | |
| 0.00 | 1.56 | 0.00 | 0.99 | -15.87 | 102.32 | -33.48 | 122.22 | 0.6295 | 1008.0 | 890.1 | |
| 0.61 | 1.65 | 0.39 | 1.05 | -16.48 | 102.17 | -33.64 | 122.95 | 0.6353 | 691.6 | 562.2 | |
| 5.11 | 11.08 | 3.27 | 7.10 | -16.05 | 101.84 | -33.97 | 122.11 | 0.6362 | 808.3 | 580.2 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -16.13 | 101.56 | -34.24 | 122.02 | 0.6399 | 586.0 | 449.1 | |
| 0.00 | 0.95 | 0.00 | 0.63 | -15.68 | 99.53 | -36.28 | 120.02 | 0.6603 | 602.0 | 464.9 | |
| 0.00 | 0.78 | 0.00 | 0.53 | -15.52 | 96.90 | -38.90 | 118.20 | 0.6890 | -600.0 | -489.4 | |
| 0.00 | 0.78 | 0.00 | 0.57 | -18.63 | 94.03 | -41.78 | 120.57 | 0.7356 | -586.0 | -500.7 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -18.10 | 93.81 | -42.00 | 119.79 | 0.7351 | -373.0 | -395.4 | |
| 0.00 | 0.69 | 0.00 | 0.50 | -17.16 | 93.37 | -42.44 | 118.39 | 0.7353 | -457.0 | -322.0 | |
| 0.00 | 1.04 | 0.00 | 0.79 | -19.53 | 91.76 | -44.05 | 120.46 | 0.7626 | -595.0 | -470.6 | |
| 0.00 | 0.78 | 0.00 | 0.60 | -19.67 | 91.53 | -44.28 | 120.51 | 0.7654 | -578.0 | -495.9 | |
| 0.00 | 1.65 | 0.00 | 1.23 | -16.62 | 91.68 | -44.13 | 116.87 | 0.7503 | -231.0 | -312.1 | |
| 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. | |