SDO HMI 2014-09-25 07:00:34 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 129.23 | 409.75 | 64.54 | 204.84 | 13.77 | 262.88 | 2.82 | 338.26 | 0.1325 | 60.2 | -55.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-25 07:00:34 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 |
| 9.02 | 142.04 | 4.52 | 71.06 | 13.52 | 265.10 | 5.04 | 323.35 | 0.1436 | -1392.7 | -526.7 | |
| 11.59 | -1.00 | 5.79 | -1.00 | 13.22 | 265.03 | 4.97 | 322.41 | 0.1388 | -1271.5 | 999999 | |
| 12.82 | -1.00 | 6.42 | -1.00 | 13.85 | 264.89 | 4.83 | 325.87 | 0.1462 | -1090.9 | 999999 | |
| 4.16 | -1.00 | 2.08 | -1.00 | 13.04 | 264.84 | 4.78 | 322.65 | 0.1344 | -1289.2 | 999999 | |
| 1.42 | -1.00 | 0.71 | -1.00 | 12.77 | 264.59 | 4.52 | 322.87 | 0.1280 | -1069.5 | 999999 | |
| 6.37 | -1.00 | 3.18 | -1.00 | 12.77 | 264.37 | 4.31 | 324.21 | 0.1258 | -1208.5 | 999999 | |
| 0.00 | 4.07 | 0.00 | 2.04 | 14.56 | 264.38 | 4.31 | 331.24 | 0.1519 | -695.0 | -764.9 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 13.65 | 264.20 | 4.14 | 329.03 | 0.1369 | 878.0 | 653.4 | |
| 0.00 | 2.83 | 0.00 | 1.42 | 14.68 | 264.19 | 4.13 | 332.66 | 0.1523 | -1104.0 | -809.9 | |
| 0.00 | 5.93 | 0.00 | 2.96 | 13.11 | 264.04 | 3.97 | 327.85 | 0.1274 | -118.0 | 87.4 | |
| 3.89 | 12.74 | 1.95 | 6.39 | 14.95 | 264.01 | 3.95 | 334.50 | 0.1552 | -1125.5 | -540.0 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 13.56 | 263.80 | 3.73 | 331.22 | 0.1321 | 467.0 | 283.1 | |
| 5.22 | 59.26 | 2.60 | 29.53 | 12.78 | 263.38 | 3.32 | 330.94 | 0.1168 | -1171.0 | -457.3 | |
| 0.00 | 3.10 | 0.00 | 1.55 | 13.23 | 263.33 | 3.26 | 333.15 | 0.1233 | 123.0 | 175.7 | |
| 0.00 | 7.25 | 0.00 | 3.62 | 13.51 | 263.27 | 3.21 | 334.54 | 0.1271 | 430.0 | 459.7 | |
| 0.00 | 2.03 | 0.00 | 1.02 | 14.63 | 263.01 | 2.94 | 339.61 | 0.1432 | 776.0 | 584.7 | |
| 1.06 | 2.56 | 0.53 | 1.28 | 14.24 | 262.97 | 2.91 | 338.82 | 0.1367 | 922.0 | 677.9 | |
| 11.50 | -13.00 | 5.73 | -13.00 | 12.66 | 262.83 | 2.76 | 334.72 | 0.1106 | -1266.0 | 999999 | |
| 1.68 | 19.46 | 0.84 | 9.73 | 14.06 | 262.69 | 2.63 | 340.24 | 0.1320 | 982.4 | 375.6 | |
| 0.97 | 2.03 | 0.49 | 1.02 | 15.00 | 262.61 | 2.54 | 342.97 | 0.1471 | 922.8 | 712.1 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 13.45 | 262.44 | 2.37 | 340.44 | 0.1207 | 820.0 | 630.4 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 13.91 | 262.41 | 2.34 | 341.84 | 0.1280 | -380.0 | -183.2 | |
| 4.25 | -13.00 | 2.11 | -13.00 | 12.45 | 262.33 | 2.27 | 338.06 | 0.1038 | -1086.1 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 15.70 | 262.34 | 2.27 | 345.91 | 0.1575 | 901.0 | 706.5 | |
| 2.92 | -19.00 | 1.46 | -19.00 | 14.42 | 262.23 | 2.16 | 344.29 | 0.1357 | 990.5 | 999999 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 12.70 | 262.03 | 1.96 | 341.56 | 0.1060 | -847.0 | -539.8 | |
| 0.00 | 0.62 | 0.00 | 0.31 | 15.73 | 262.06 | 1.99 | 347.63 | 0.1569 | -270.0 | -487.3 | |
| 0.00 | 1.77 | 0.00 | 0.88 | 14.45 | 261.89 | 1.82 | 346.73 | 0.1347 | 408.0 | 134.6 | |
| 0.00 | 1.86 | 0.00 | 0.93 | 12.76 | 261.81 | 1.75 | 343.63 | 0.1059 | -579.0 | -286.6 | |
| 0.00 | 3.54 | 0.00 | 1.77 | 15.70 | 261.77 | 1.71 | 349.30 | 0.1554 | -1075.0 | -651.7 | |
| 0.71 | 2.12 | 0.35 | 1.06 | 15.58 | 261.49 | 1.43 | 350.91 | 0.1526 | 932.9 | 695.4 | |
| 41.48 | 79.07 | 20.71 | 39.48 | 14.06 | 261.11 | 1.04 | 351.87 | 0.1256 | 1207.3 | 443.6 | |
| 0.00 | 1.06 | 0.00 | 0.53 | 12.34 | 261.10 | 1.03 | 349.36 | 0.0959 | 754.0 | 493.4 | |
| 2.12 | -32.00 | 1.06 | -32.00 | 14.58 | 260.83 | 0.77 | 354.42 | 0.1339 | 1032.8 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.57 | 14.76 | 260.43 | 0.36 | 357.41 | 0.1366 | 976.0 | 673.6 | |
| 0.00 | 2.12 | 0.00 | 1.07 | 16.56 | 260.40 | 0.34 | 358.06 | 0.1676 | 931.0 | 722.2 | |
| 0.00 | 1.95 | 0.00 | 0.98 | 16.25 | 260.40 | 0.34 | 358.00 | 0.1624 | 879.0 | 733.9 | |
| 1.77 | 4.07 | 0.88 | 2.03 | 12.79 | 260.33 | 0.27 | 357.45 | 0.1023 | 1164.5 | 899.0 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 15.28 | 260.21 | 0.15 | 359.02 | 0.1454 | 332.0 | 581.5 | |
| 1.59 | 11.67 | 0.79 | 5.82 | 13.64 | 260.18 | 0.11 | 359.06 | 0.1169 | 1188.0 | 819.5 | |
| 0.00 | 2.12 | 0.00 | 1.06 | 15.16 | 260.18 | 0.12 | 359.22 | 0.1433 | 1141.0 | 909.9 | |
| 1.15 | -40.00 | 0.57 | -40.00 | 13.55 | 259.87 | -0.20 | 1.66 | 0.1154 | 1180.5 | 999999 | |
| 1.33 | 5.57 | 0.66 | 2.79 | 15.49 | 259.84 | -0.23 | 1.47 | 0.1491 | 1117.1 | 919.0 | |
| 0.00 | 1.33 | 0.00 | 0.66 | 13.28 | 259.56 | -0.51 | 4.46 | 0.1110 | 1003.0 | 800.3 | |
| 0.00 | 4.42 | 0.00 | 2.22 | 15.77 | 259.53 | -0.54 | 3.38 | 0.1541 | 1105.0 | 934.5 | |
| 0.00 | 0.71 | 0.00 | 0.36 | 17.20 | 259.37 | -0.70 | 3.75 | 0.1790 | 968.0 | 771.1 | |
| 0.00 | 1.86 | 0.00 | 0.94 | 17.35 | 259.30 | -0.76 | 4.02 | 0.1817 | 920.0 | 705.9 | |
| 2.21 | 6.63 | 1.11 | 3.33 | 15.74 | 258.90 | -1.16 | 7.30 | 0.1546 | 1171.5 | 977.3 | |
| 0.00 | 1.59 | 0.00 | 0.80 | 16.86 | 258.64 | -1.42 | 7.85 | 0.1745 | 823.0 | 695.4 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 14.37 | 258.60 | -1.47 | 10.89 | 0.1320 | 939.0 | 727.3 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 15.67 | 258.59 | -1.48 | 9.29 | 0.1543 | 878.0 | 762.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 15.07 | 258.44 | -1.63 | 11.00 | 0.1444 | 995.0 | 753.6 | |
| 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. | |