| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 117.86 | 698.36 | 81.49 | 482.87 | 7.86 | 344.10 | 44.59 | 274.02 | 0.6994 | -386.5 | -283.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-26 01:00:37 UT
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 | 0.45 | 0.00 | 0.34 | 12.39 | 348.64 | 49.13 | 280.30 | 0.7530 | -496.0 | -434.0 | |
| 0.00 | 1.35 | 0.00 | 0.99 | 7.51 | 347.38 | 47.87 | 273.73 | 0.7391 | -602.0 | -497.0 | |
| 2.87 | 8.17 | 2.10 | 5.96 | 7.93 | 347.17 | 47.66 | 274.28 | 0.7364 | -503.7 | -349.2 | |
| 0.00 | 1.17 | 0.00 | 0.85 | 8.35 | 347.19 | 47.68 | 274.86 | 0.7365 | -267.0 | -230.0 | |
| 0.00 | 1.17 | 0.00 | 0.85 | 7.52 | 346.92 | 47.42 | 273.71 | 0.7338 | -679.0 | -600.6 | |
| 0.00 | 0.99 | 0.00 | 0.73 | 13.00 | 347.95 | 48.44 | 281.15 | 0.7454 | -649.0 | -467.0 | |
| 3.41 | 7.90 | 2.46 | 5.70 | 8.20 | 346.57 | 47.07 | 274.62 | 0.7293 | -733.3 | -520.9 | |
| 0.00 | 3.68 | 0.00 | 2.64 | 6.76 | 346.28 | 46.77 | 272.62 | 0.7266 | 30.0 | -117.4 | |
| 0.00 | 1.62 | 0.00 | 1.16 | 7.88 | 346.39 | 46.88 | 274.17 | 0.7273 | -572.0 | -468.7 | |
| 0.00 | 1.97 | 0.00 | 1.43 | 9.90 | 346.64 | 47.14 | 276.96 | 0.7297 | 620.0 | 495.7 | |
| 1.71 | 638.62 | 1.22 | 441.42 | 7.57 | 346.07 | 46.57 | 273.73 | 0.7237 | -649.4 | -304.5 | |
| 2.42 | -11.00 | 1.73 | -11.00 | 7.27 | 346.03 | 46.53 | 273.31 | 0.7233 | -842.4 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.45 | 10.17 | 346.42 | 46.91 | 277.32 | 0.7271 | 609.0 | 583.6 | |
| 4.85 | -11.00 | 3.45 | -11.00 | 7.50 | 345.80 | 46.29 | 273.62 | 0.7204 | -996.1 | 999999 | |
| 1.97 | -11.00 | 1.39 | -11.00 | 7.01 | 345.16 | 45.65 | 272.89 | 0.7130 | 68.7 | 999999 | |
| 23.07 | -11.00 | 16.07 | -11.00 | 6.67 | 344.51 | 45.00 | 272.36 | 0.7052 | 762.8 | 999999 | |
| 1.97 | -11.00 | 1.38 | -11.00 | 8.54 | 344.76 | 45.25 | 275.02 | 0.7074 | -169.8 | 999999 | |
| 1.17 | -11.00 | 0.81 | -11.00 | 6.71 | 344.04 | 44.53 | 272.38 | 0.6994 | 568.5 | 999999 | |
| 62.83 | -11.00 | 43.13 | -11.00 | 8.33 | 343.73 | 44.23 | 274.67 | 0.6947 | -1041.2 | 999999 | |
| 1.53 | -11.00 | 1.04 | -11.00 | 6.71 | 343.44 | 43.93 | 272.31 | 0.6919 | 171.8 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.92 | 6.64 | 343.13 | 43.63 | 272.20 | 0.6881 | 429.0 | 362.1 | |
| 0.00 | 1.44 | 0.00 | 0.98 | 6.94 | 343.17 | 43.66 | 272.64 | 0.6883 | -553.0 | -489.0 | |
| 4.76 | -11.00 | 3.19 | -11.00 | 7.23 | 342.32 | 42.81 | 273.00 | 0.6774 | 500.1 | 999999 | |
| 0.63 | 4.49 | 0.42 | 3.01 | 11.11 | 342.19 | 42.69 | 278.76 | 0.6754 | 752.4 | 584.8 | |
| 0.00 | 1.17 | 0.00 | 0.78 | 10.30 | 342.01 | 42.50 | 277.56 | 0.6728 | -607.0 | -495.8 | |
| 4.67 | 8.62 | 3.10 | 5.72 | 8.54 | 341.57 | 42.06 | 274.92 | 0.6673 | -741.3 | -557.1 | |
| 0.00 | 6.55 | 0.00 | 4.34 | 9.58 | 341.47 | 41.97 | 276.49 | 0.6659 | 75.0 | 158.0 | |
| 0.00 | 1.17 | 0.00 | 0.77 | 8.77 | 341.02 | 41.52 | 275.25 | 0.6602 | 547.0 | 507.5 | |
| 0.00 | 1.17 | 0.00 | 0.77 | 9.61 | 341.15 | 41.64 | 276.53 | 0.6617 | 599.0 | 494.2 | |
| 0.00 | 0.90 | 0.00 | 0.59 | 11.30 | 341.39 | 41.88 | 279.08 | 0.6652 | 603.0 | 549.0 | |
| 0.00 | 1.08 | 0.00 | 0.71 | 7.93 | 340.83 | 41.33 | 273.97 | 0.6579 | 667.0 | 552.6 | |
| 0.00 | 1.53 | 0.00 | 1.00 | 8.18 | 340.78 | 41.28 | 274.34 | 0.6571 | 808.0 | 639.5 | |
| 0.00 | 1.17 | 0.00 | 0.76 | 7.64 | 340.63 | 41.13 | 273.52 | 0.6554 | 545.0 | 472.3 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |