SDO HMI 2014-10-05 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.10 | 22.94 | 4.10 | 20.05 | -19.32 | 76.15 | -49.77 | 118.94 | 0.8235 | 284.5 | 101.2 | |
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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 | 0.79 | 0.00 | 0.66 | -22.39 | 80.10 | -45.81 | 124.25 | 0.8043 | 440.0 | 380.0 | |
| 5.10 | 9.14 | 4.10 | 7.36 | -18.25 | 79.58 | -46.33 | 119.29 | 0.7899 | 729.1 | 536.6 | |
| 0.00 | 0.88 | 0.00 | 0.75 | -21.08 | 77.77 | -48.15 | 121.61 | 0.8183 | 312.0 | 265.0 | |
| 0.00 | 0.88 | 0.00 | 0.70 | -15.97 | 79.28 | -46.64 | 116.47 | 0.7831 | 578.0 | 528.6 | |
| 0.00 | 1.14 | 0.00 | 0.96 | -16.79 | 76.57 | -49.35 | 116.21 | 0.8118 | 439.0 | 375.8 | |
| 0.00 | 3.16 | 0.00 | 2.77 | -18.09 | 75.49 | -50.43 | 117.22 | 0.8262 | 263.0 | 237.1 | |
| 0.00 | 0.53 | 0.00 | 0.48 | -19.55 | 74.15 | -51.76 | 118.30 | 0.8427 | 377.0 | 371.2 | |
| 0.00 | 2.64 | 0.00 | 2.68 | -22.69 | 71.27 | -54.65 | 120.52 | 0.8755 | -530.0 | -416.5 | |
| 0.00 | 2.37 | 0.00 | 2.26 | -19.41 | 72.48 | -53.44 | 117.47 | 0.8558 | -124.0 | -244.0 | |
| 0.00 | 0.53 | 0.00 | 0.51 | -20.20 | 71.82 | -54.10 | 118.07 | 0.8635 | -439.0 | -456.5 | |
| 0.00 | 0.88 | 0.00 | 0.92 | -22.45 | 70.33 | -55.58 | 119.90 | 0.8815 | -293.0 | -269.5 | |
| 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. | |