SDO HMI 2014-10-09 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.29 | 0.00 | 10.89 | -17.18 | 104.32 | 28.99 | 228.80 | 0.6120 | 168.6 | 142.9 | |
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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 | 0.96 | 0.00 | 0.64 | -13.02 | 112.79 | 37.46 | 242.51 | 0.6704 | 681.0 | 569.7 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -15.65 | 112.21 | 36.88 | 238.63 | 0.6792 | 407.0 | 383.3 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -16.53 | 110.96 | 35.63 | 236.62 | 0.6712 | 619.0 | 534.6 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -13.35 | 110.29 | 34.96 | 240.40 | 0.6434 | 650.0 | 551.6 | |
| 0.00 | 0.96 | 0.00 | 0.64 | -15.61 | 110.58 | 35.25 | 237.56 | 0.6610 | 581.0 | 428.0 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -16.67 | 110.61 | 35.28 | 236.19 | 0.6682 | 649.0 | 526.6 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -13.36 | 109.87 | 34.54 | 240.10 | 0.6387 | 694.0 | 637.3 | |
| 0.00 | 1.58 | 0.00 | 1.04 | -15.90 | 110.18 | 34.85 | 236.88 | 0.6585 | 578.0 | 423.5 | |
| 0.00 | 2.11 | 0.00 | 1.38 | -18.94 | 107.87 | 32.54 | 231.15 | 0.6555 | 731.0 | 565.5 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -22.31 | 108.38 | 33.05 | 227.51 | 0.6865 | 469.0 | 467.0 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -18.04 | 97.20 | 21.88 | 221.24 | 0.5396 | -661.0 | -493.2 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -19.28 | 93.68 | 18.35 | 214.90 | 0.5215 | -696.0 | -558.6 | |
| 0.00 | 2.28 | 0.00 | 1.32 | -19.44 | 92.70 | 17.37 | 213.27 | 0.5153 | -791.0 | -615.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -20.10 | 92.41 | 17.08 | 212.10 | 0.5210 | -642.0 | -492.1 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -19.78 | 88.74 | 13.41 | 206.57 | 0.4899 | -740.0 | -583.9 | |
| 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. | |