SDO HMI 2014-11-03 17:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.09 | 0.00 | 12.36 | -20.14 | 79.24 | -20.88 | 141.38 | 0.5286 | 535.4 | 466.3 | |
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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 | 0.95 | 0.00 | 0.52 | -16.22 | 86.62 | -13.50 | 147.05 | 0.4138 | 816.0 | 573.8 | |
| 0.00 | 2.25 | 0.00 | 1.27 | -20.85 | 85.41 | -14.70 | 150.55 | 0.4844 | 380.0 | 479.2 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -16.72 | 84.95 | -15.17 | 144.67 | 0.4352 | 788.0 | 515.6 | |
| 0.00 | 2.25 | 0.00 | 1.24 | -17.43 | 84.57 | -15.55 | 144.98 | 0.4476 | 819.0 | 569.3 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -20.93 | 82.82 | -17.30 | 146.56 | 0.5060 | 477.0 | 476.1 | |
| 0.00 | 2.77 | 0.00 | 1.61 | -20.15 | 79.77 | -20.35 | 141.27 | 0.5239 | 654.0 | 620.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -20.33 | 79.13 | -20.99 | 140.65 | 0.5318 | 665.0 | 582.7 | |
| 0.00 | 1.47 | 0.00 | 0.86 | -20.46 | 79.04 | -21.07 | 140.71 | 0.5341 | 686.0 | 554.1 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -20.43 | 78.02 | -22.09 | 139.36 | 0.5433 | 208.0 | 323.4 | |
| 0.00 | 2.25 | 0.00 | 1.32 | -20.26 | 77.98 | -22.14 | 139.10 | 0.5420 | 669.0 | 590.0 | |
| 0.00 | 1.04 | 0.00 | 0.62 | -20.27 | 76.60 | -23.51 | 137.43 | 0.5555 | 565.0 | 491.4 | |
| 0.00 | 1.73 | 0.00 | 1.04 | -20.76 | 75.41 | -24.71 | 136.70 | 0.5722 | 323.0 | 312.8 | |
| 0.00 | 0.95 | 0.00 | 0.61 | -24.47 | 72.85 | -27.27 | 138.50 | 0.6317 | 536.0 | 472.5 | |
| 0.00 | 1.47 | 0.00 | 1.02 | -23.61 | 64.59 | -35.53 | 130.41 | 0.7016 | -91.0 | -145.6 | |
| 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. | |