SDO HMI 2014-07-09 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.60 | 398.84 | 50.69 | 304.15 | -19.15 | 254.52 | 44.61 | 240.75 | 0.7624 | 930.2 | 284.1 | |
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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 | 1.00 | 0.00 | 1.03 | -21.65 | 267.09 | 57.18 | 242.82 | 0.8800 | 358.0 | 241.0 | |
| 0.00 | 0.91 | 0.00 | 0.84 | -20.41 | 263.38 | 53.48 | 242.96 | 0.8477 | 430.0 | 390.3 | |
| 0.00 | 1.09 | 0.00 | 1.01 | -20.82 | 262.99 | 53.08 | 242.36 | 0.8457 | 537.0 | 463.5 | |
| 0.00 | 1.27 | 0.00 | 1.15 | -20.98 | 262.26 | 52.35 | 241.91 | 0.8401 | 424.0 | 351.2 | |
| 0.00 | 0.64 | 0.00 | 0.57 | -22.31 | 261.49 | 51.58 | 240.13 | 0.8380 | 278.0 | 235.4 | |
| 0.00 | 1.18 | 0.00 | 0.97 | -23.10 | 256.74 | 46.83 | 237.18 | 0.8005 | -657.0 | -508.1 | |
| 63.87 | 382.03 | 48.63 | 290.59 | -19.05 | 254.43 | 44.52 | 240.84 | 0.7612 | 1161.1 | 298.8 | |
| 2.18 | 3.82 | 1.65 | 2.90 | -21.31 | 253.19 | 43.29 | 237.50 | 0.7597 | 640.7 | 498.3 | |
| 0.00 | 1.18 | 0.00 | 0.90 | -22.23 | 252.77 | 42.86 | 236.18 | 0.7602 | -430.0 | -381.3 | |
| 0.55 | 1.54 | 0.41 | 1.15 | -22.12 | 251.74 | 41.84 | 235.75 | 0.7499 | -537.0 | -433.9 | |
| 0.00 | 1.73 | 0.00 | 1.25 | -20.31 | 251.03 | 41.13 | 237.53 | 0.7335 | -546.0 | -403.0 | |
| 0.00 | 2.45 | 0.00 | 1.79 | -20.58 | 251.08 | 41.17 | 237.23 | 0.7353 | -702.0 | -452.6 | |
| 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. | |