SDO HMI 2014-09-19 15:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.04 | 0.00 | 11.97 | 7.93 | 333.86 | -1.01 | 176.11 | 0.1124 | -157.2 | 78.1 | |
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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 | 2.22 | 0.00 | 1.12 | 6.24 | 344.97 | 10.11 | 265.63 | 0.1757 | -829.0 | -692.2 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 11.69 | 342.40 | 7.53 | 302.19 | 0.1523 | -753.0 | -594.9 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 10.79 | 341.57 | 6.70 | 299.56 | 0.1324 | -888.0 | -665.1 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 1.90 | 339.81 | 4.94 | 223.58 | 0.1254 | -813.0 | -753.9 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 8.45 | 338.89 | 4.02 | 288.76 | 0.0736 | -803.0 | -596.1 | |
| 0.00 | 0.89 | 0.00 | 0.44 | 9.27 | 337.96 | 3.09 | 305.41 | 0.0655 | -839.0 | -667.6 | |
| 0.00 | 0.98 | 0.00 | 0.48 | 8.16 | 337.73 | 2.86 | 290.35 | 0.0530 | -951.0 | -768.0 | |
| 0.00 | 2.04 | 0.00 | 1.01 | 8.46 | 337.58 | 2.71 | 296.75 | 0.0527 | -906.0 | -644.4 | |
| 0.00 | 1.42 | 0.00 | 0.70 | 6.06 | 331.78 | -3.09 | 108.87 | 0.0569 | 830.0 | 594.1 | |
| 0.00 | 1.60 | 0.00 | 0.79 | 8.73 | 330.79 | -4.08 | 67.96 | 0.0762 | 761.0 | 670.3 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 7.77 | 327.96 | -6.91 | 84.14 | 0.1204 | 973.0 | 763.5 | |
| 0.00 | 4.43 | 0.00 | 2.21 | 7.55 | 327.81 | -7.06 | 85.98 | 0.1227 | 257.0 | 699.8 | |
| 0.00 | 1.86 | 0.00 | 0.93 | 7.60 | 327.11 | -7.76 | 85.89 | 0.1349 | 895.0 | 658.2 | |
| 0.00 | 2.75 | 0.00 | 1.37 | 8.14 | 326.76 | -8.11 | 82.22 | 0.1416 | 865.0 | 760.3 | |
| 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. | |