SDO HMI 2014-05-17 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.61 | 67.57 | 13.05 | 34.43 | -15.75 | 194.26 | -2.01 | 171.53 | 0.2338 | 416.3 | 262.2 | |
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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 |
| 2.43 | 19.76 | 1.24 | 10.10 | -16.61 | 195.32 | -0.94 | 176.32 | 0.2459 | 1130.6 | 710.3 | |
| 0.90 | -1.00 | 0.46 | -1.00 | -16.39 | 195.29 | -0.97 | 176.14 | 0.2422 | 1101.3 | 999999 | |
| 4.22 | 6.65 | 2.15 | 3.39 | -15.86 | 195.23 | -1.03 | 175.73 | 0.2333 | 1088.2 | 762.0 | |
| 7.01 | -1.00 | 3.58 | -1.00 | -16.67 | 195.16 | -1.10 | 175.72 | 0.2471 | 1061.0 | 999999 | |
| 0.00 | 3.05 | 0.00 | 1.56 | -16.61 | 194.78 | -1.48 | 174.23 | 0.2466 | 418.0 | 390.3 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -12.92 | 194.69 | -1.57 | 171.61 | 0.1841 | -728.0 | -510.7 | |
| 0.00 | 2.52 | 0.00 | 1.28 | -15.33 | 194.57 | -1.69 | 172.73 | 0.2254 | 601.0 | 384.7 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -16.74 | 194.53 | -1.73 | 173.30 | 0.2492 | 908.0 | 807.3 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -12.58 | 194.47 | -1.79 | 170.16 | 0.1789 | -931.0 | -766.7 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -15.67 | 194.26 | -2.00 | 171.61 | 0.2319 | -503.0 | -394.9 | |
| 0.00 | 1.71 | 0.00 | 0.87 | -15.08 | 193.79 | -2.47 | 169.21 | 0.2233 | 504.0 | 528.2 | |
| 1.80 | 19.94 | 0.91 | 10.15 | -15.58 | 193.56 | -2.70 | 168.70 | 0.2323 | -755.9 | 58.7 | |
| 5.48 | -12.00 | 2.79 | -12.00 | -15.24 | 193.54 | -2.72 | 168.28 | 0.2267 | 949.2 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -15.83 | 193.21 | -3.05 | 167.52 | 0.2377 | -699.0 | -521.4 | |
| 0.00 | 1.80 | 0.00 | 0.91 | -14.92 | 192.88 | -3.38 | 165.21 | 0.2241 | 837.0 | 752.2 | |
| 3.77 | 5.93 | 1.92 | 3.02 | -15.33 | 192.44 | -3.83 | 163.87 | 0.2327 | -999.8 | -688.6 | |
| 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. | |