SDO HMI 2014-07-09 07:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.35 | 216.87 | 36.67 | 208.03 | -11.90 | 268.02 | 57.02 | 253.64 | 0.8574 | 91.2 | -76.7 | |
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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 | 1.45 | 0.00 | 1.58 | -13.15 | 272.01 | 61.01 | 253.16 | 0.8918 | 509.0 | 426.8 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -13.65 | 271.90 | 60.90 | 252.58 | 0.8917 | 562.0 | 543.0 | |
| 4.82 | 101.76 | 4.74 | 100.75 | -10.29 | 269.37 | 58.37 | 255.81 | 0.8661 | 822.0 | 149.6 | |
| 1.91 | 3.36 | 1.94 | 3.42 | -12.40 | 270.01 | 59.01 | 253.56 | 0.8749 | 471.3 | 355.7 | |
| 12.27 | -3.00 | 12.07 | -3.00 | -10.63 | 269.29 | 58.29 | 255.40 | 0.8660 | 829.6 | 999999 | |
| 0.00 | 1.18 | 0.00 | 1.20 | -12.65 | 269.98 | 58.98 | 253.27 | 0.8751 | 338.0 | 246.6 | |
| 1.36 | 3.00 | 1.31 | 2.89 | -10.52 | 268.56 | 57.56 | 255.36 | 0.8596 | 722.5 | 593.6 | |
| 0.00 | 1.00 | 0.00 | 0.96 | -10.77 | 268.45 | 57.45 | 255.06 | 0.8591 | 625.0 | 539.0 | |
| 0.00 | 1.91 | 0.00 | 1.89 | -13.94 | 268.79 | 57.79 | 251.53 | 0.8677 | -306.0 | -252.4 | |
| 0.00 | 1.73 | 0.00 | 1.67 | -12.67 | 268.20 | 57.20 | 252.83 | 0.8604 | 340.0 | 338.1 | |
| 0.00 | 1.00 | 0.00 | 0.95 | -12.27 | 267.83 | 56.83 | 253.19 | 0.8565 | 439.0 | 397.3 | |
| 0.00 | 1.73 | 0.00 | 1.57 | -8.73 | 266.73 | 55.73 | 257.05 | 0.8403 | 614.0 | 478.8 | |
| 0.00 | 0.45 | 0.00 | 0.42 | -10.95 | 267.25 | 56.25 | 254.58 | 0.8489 | 464.0 | 410.2 | |
| 0.00 | 1.73 | 0.00 | 1.64 | -13.99 | 267.29 | 56.29 | 251.10 | 0.8553 | -512.0 | -393.9 | |
| 17.99 | 96.30 | 16.61 | 88.79 | -13.42 | 266.36 | 55.36 | 251.50 | 0.8460 | -878.2 | -409.4 | |
| 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. | |