SDO HMI 2014-07-09 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.78 | 394.73 | 48.23 | 303.42 | -19.15 | 254.42 | 45.06 | 240.98 | 0.7670 | 878.6 | 271.4 | |
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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 | 1.09 | 0.00 | 1.02 | -20.81 | 262.99 | 53.63 | 242.56 | 0.8502 | 513.0 | 488.1 | |
| 0.00 | 1.00 | 0.00 | 0.84 | -23.49 | 257.21 | 47.85 | 237.21 | 0.8110 | -521.0 | -403.6 | |
| 0.00 | 0.82 | 0.00 | 0.68 | -23.06 | 256.71 | 47.35 | 237.47 | 0.8049 | -502.0 | -445.6 | |
| 0.00 | 1.00 | 0.00 | 0.84 | -23.81 | 256.77 | 47.41 | 236.64 | 0.8086 | -443.0 | -300.4 | |
| 3.36 | 378.83 | 2.57 | 290.93 | -18.35 | 254.33 | 44.97 | 241.91 | 0.7626 | 979.8 | 290.5 | |
| 57.60 | -5.00 | 44.27 | -5.00 | -19.07 | 254.44 | 45.08 | 241.08 | 0.7668 | 1165.3 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.78 | -21.70 | 253.80 | 44.44 | 237.63 | 0.7725 | -141.0 | -85.3 | |
| 1.82 | 4.27 | 1.39 | 3.27 | -21.33 | 253.15 | 43.80 | 237.73 | 0.7647 | 694.2 | 502.7 | |
| 0.00 | 2.00 | 0.00 | 1.53 | -22.25 | 252.73 | 43.37 | 236.42 | 0.7651 | -395.0 | -380.0 | |
| 0.00 | 1.00 | 0.00 | 0.76 | -22.34 | 252.35 | 43.00 | 236.12 | 0.7620 | -474.0 | -395.2 | |
| 0.00 | 1.36 | 0.00 | 1.03 | -22.14 | 251.74 | 42.38 | 236.02 | 0.7552 | -751.0 | -528.7 | |
| 0.00 | 1.18 | 0.00 | 0.87 | -20.37 | 251.03 | 41.67 | 237.76 | 0.7392 | -587.0 | -454.3 | |
| 0.00 | 1.18 | 0.00 | 0.87 | -20.67 | 251.04 | 41.68 | 237.40 | 0.7408 | -613.0 | -359.8 | |
| 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. | |