SDO HMI 2014-09-19 19:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.74 | 27.65 | 4.14 | 16.85 | -21.03 | 310.52 | -22.14 | 142.86 | 0.5837 | -285.1 | -192.9 | |
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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 | 1.86 | 0.00 | 1.09 | -19.32 | 313.85 | -18.81 | 145.27 | 0.5362 | 790.0 | 677.3 | |
| 0.00 | 3.28 | 0.00 | 1.92 | -18.93 | 313.49 | -19.17 | 144.33 | 0.5347 | 882.0 | 712.5 | |
| 0.00 | 0.89 | 0.00 | 0.53 | -19.97 | 312.72 | -19.94 | 144.44 | 0.5534 | 718.0 | 617.4 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -18.64 | 312.52 | -20.14 | 142.64 | 0.5398 | 738.0 | 572.7 | |
| 1.60 | 3.28 | 0.98 | 2.01 | -21.72 | 310.28 | -22.38 | 143.25 | 0.5934 | -907.6 | -671.3 | |
| 1.33 | 2.57 | 0.81 | 1.57 | -21.05 | 310.04 | -22.62 | 142.22 | 0.5882 | -865.2 | -710.1 | |
| 0.00 | 1.06 | 0.00 | 0.66 | -21.92 | 309.72 | -22.94 | 142.79 | 0.6003 | -810.0 | -720.1 | |
| 0.00 | 1.51 | 0.00 | 0.94 | -22.31 | 309.44 | -23.23 | 142.88 | 0.6068 | -442.0 | -383.5 | |
| 0.00 | 2.57 | 0.00 | 1.59 | -22.03 | 309.45 | -23.21 | 142.60 | 0.6038 | -822.0 | -586.7 | |
| 2.30 | 3.63 | 1.42 | 2.24 | -21.66 | 309.44 | -23.22 | 142.19 | 0.5998 | -913.0 | -702.1 | |
| 0.00 | 1.95 | 0.00 | 1.20 | -21.25 | 309.37 | -23.29 | 141.65 | 0.5962 | -717.0 | -674.2 | |
| 0.00 | 0.89 | 0.00 | 0.55 | -21.42 | 309.34 | -23.32 | 141.81 | 0.5982 | -544.0 | -475.1 | |
| 1.51 | 3.19 | 0.93 | 1.98 | -21.64 | 309.16 | -23.50 | 141.84 | 0.6020 | -702.4 | -539.6 | |
| 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. | |