SDO HMI 2014-10-03 01:00:32 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 |
| 20.25 | 85.07 | 10.34 | 43.35 | 12.65 | 169.35 | 11.56 | 301.27 | 0.2282 | -153.9 | -193.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-03 01:00:32 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 | 1.32 | 0.00 | 0.69 | 9.40 | 175.71 | 17.93 | 280.04 | 0.3097 | -664.0 | -461.0 | |
| 0.00 | 4.14 | 0.00 | 2.14 | 10.63 | 174.12 | 16.34 | 285.02 | 0.2875 | -955.0 | -821.7 | |
| 0.00 | 2.11 | 0.00 | 1.09 | 10.31 | 173.88 | 16.10 | 284.08 | 0.2825 | -816.0 | -720.0 | |
| 0.00 | 2.46 | 0.00 | 1.28 | 13.82 | 173.46 | 15.68 | 296.21 | 0.2938 | -671.0 | -646.5 | |
| 1.06 | 3.08 | 0.54 | 1.58 | 12.58 | 171.41 | 13.62 | 294.90 | 0.2546 | -895.6 | -790.4 | |
| 1.41 | 5.98 | 0.72 | 3.07 | 13.10 | 171.41 | 13.62 | 296.75 | 0.2580 | -929.2 | -735.4 | |
| 0.00 | 2.11 | 0.00 | 1.08 | 13.40 | 171.26 | 13.48 | 298.05 | 0.2581 | -624.0 | -572.8 | |
| 15.58 | 28.16 | 7.96 | 14.40 | 12.96 | 170.77 | 12.98 | 297.30 | 0.2475 | -1148.7 | -755.6 | |
| 2.20 | -8.00 | 1.12 | -8.00 | 13.27 | 170.69 | 12.90 | 298.54 | 0.2485 | -982.7 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 11.61 | 170.48 | 12.69 | 292.57 | 0.2341 | -810.0 | -705.9 | |
| 0.00 | 1.58 | 0.00 | 0.81 | 11.68 | 170.23 | 12.44 | 293.21 | 0.2307 | -866.0 | -712.4 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 11.47 | 170.19 | 12.40 | 292.42 | 0.2287 | -1073.0 | -922.9 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 14.58 | 170.10 | 12.31 | 304.29 | 0.2509 | 651.0 | 538.8 | |
| 0.00 | 4.75 | 0.00 | 2.42 | 12.65 | 169.90 | 12.11 | 297.64 | 0.2322 | -860.0 | -816.7 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 14.98 | 169.90 | 12.11 | 306.05 | 0.2519 | -996.0 | -764.1 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 10.78 | 168.97 | 11.19 | 291.29 | 0.2055 | 738.0 | 623.1 | |
| 0.00 | 1.50 | 0.00 | 0.76 | 11.26 | 168.90 | 11.11 | 293.62 | 0.2073 | 696.0 | 568.7 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 10.96 | 168.82 | 11.04 | 292.39 | 0.2042 | 805.0 | 682.5 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 8.85 | 167.85 | 10.07 | 283.13 | 0.1782 | 798.0 | 643.1 | |
| 0.00 | 0.62 | 0.00 | 0.31 | 12.58 | 167.92 | 10.14 | 301.48 | 0.2023 | -704.0 | -527.9 | |
| 0.00 | 1.58 | 0.00 | 0.80 | 12.30 | 167.01 | 9.22 | 302.56 | 0.1866 | 947.0 | 747.8 | |
| 0.00 | 2.46 | 0.00 | 1.24 | 14.04 | 165.86 | 8.07 | 313.63 | 0.1890 | 899.0 | 662.3 | |
| 0.00 | 1.32 | 0.00 | 0.67 | 14.34 | 165.80 | 8.02 | 314.98 | 0.1920 | 792.0 | 603.3 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 13.74 | 165.69 | 7.90 | 313.01 | 0.1835 | 800.0 | 583.3 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 12.87 | 165.29 | 7.50 | 310.69 | 0.1686 | 806.0 | 540.4 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 15.08 | 162.43 | 4.64 | 332.04 | 0.1674 | 820.0 | 669.3 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 12.91 | 162.13 | 4.35 | 325.98 | 0.1327 | 908.0 | 738.4 | |
| 0.00 | 2.73 | 0.00 | 1.36 | 12.82 | 161.95 | 4.16 | 326.75 | 0.1297 | 1116.0 | 857.6 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 12.73 | 161.79 | 4.01 | 327.35 | 0.1269 | 877.0 | 685.2 | |
| 0.00 | 1.58 | 0.00 | 0.79 | 13.16 | 161.37 | 3.58 | 331.86 | 0.1295 | 1005.0 | 941.8 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 13.31 | 160.90 | 3.12 | 335.52 | 0.1284 | 990.0 | 876.6 | |
| 0.00 | 2.55 | 0.00 | 1.27 | 13.22 | 160.69 | 2.90 | 336.75 | 0.1255 | 888.0 | 591.6 | |
| 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. | |