SDO HMI 2014-10-02 06:00:33 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 |
| 23.08 | 126.26 | 15.51 | 83.60 | 7.18 | 210.10 | 41.86 | 273.30 | 0.6652 | -141.8 | -40.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-02 06:00:33 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 | 1.06 | 0.00 | 0.73 | 6.78 | 212.38 | 44.14 | 272.86 | 0.6947 | -552.0 | -458.1 | |
| 0.00 | 0.70 | 0.00 | 0.48 | 4.95 | 211.90 | 43.66 | 270.17 | 0.6901 | -332.0 | -302.1 | |
| 16.65 | 55.94 | 11.34 | 38.07 | 7.66 | 211.89 | 43.66 | 274.11 | 0.6883 | -923.3 | -425.4 | |
| 1.32 | -3.00 | 0.90 | -3.00 | 7.32 | 211.60 | 43.36 | 273.60 | 0.6847 | -857.5 | 999999 | |
| 0.62 | 2.03 | 0.41 | 1.35 | 6.61 | 210.69 | 42.45 | 272.50 | 0.6734 | -798.0 | -671.0 | |
| 0.00 | 6.78 | 0.00 | 4.54 | 7.15 | 210.75 | 42.51 | 273.31 | 0.6739 | -886.0 | -668.8 | |
| 0.00 | 0.97 | 0.00 | 0.64 | 5.67 | 210.39 | 42.15 | 271.07 | 0.6703 | -480.0 | -377.7 | |
| 0.00 | 1.59 | 0.00 | 1.05 | 7.51 | 210.42 | 42.19 | 273.82 | 0.6696 | -771.0 | -624.1 | |
| 0.00 | 1.59 | 0.00 | 1.05 | 7.69 | 210.08 | 41.84 | 274.08 | 0.6650 | -386.0 | -418.6 | |
| 0.00 | 2.91 | 0.00 | 1.92 | 6.46 | 209.94 | 41.70 | 272.22 | 0.6638 | -367.0 | -362.1 | |
| 0.00 | 1.41 | 0.00 | 0.93 | 5.57 | 209.73 | 41.50 | 270.86 | 0.6618 | -520.0 | -444.2 | |
| 0.00 | 0.62 | 0.00 | 0.41 | 9.38 | 210.10 | 41.87 | 276.63 | 0.6652 | -268.0 | -327.3 | |
| 0.00 | 1.59 | 0.00 | 1.04 | 6.84 | 209.33 | 41.09 | 272.75 | 0.6557 | 512.0 | 301.1 | |
| 0.00 | 1.94 | 0.00 | 1.26 | 6.27 | 208.95 | 40.72 | 271.85 | 0.6510 | 540.0 | 444.9 | |
| 0.97 | 5.90 | 0.63 | 3.84 | 6.78 | 208.92 | 40.69 | 272.64 | 0.6504 | 623.5 | 459.9 | |
| 0.00 | 1.59 | 0.00 | 1.03 | 7.10 | 208.64 | 40.40 | 273.12 | 0.6464 | -298.0 | -244.7 | |
| 0.00 | 1.06 | 0.00 | 0.68 | 6.89 | 208.26 | 40.02 | 272.77 | 0.6415 | 638.0 | 551.8 | |
| 0.00 | 2.11 | 0.00 | 1.36 | 7.05 | 208.20 | 39.96 | 273.01 | 0.6406 | 519.0 | 407.4 | |
| 0.00 | 0.70 | 0.00 | 0.45 | 6.90 | 208.10 | 39.86 | 272.78 | 0.6394 | 640.0 | 554.1 | |
| 0.00 | 1.59 | 0.00 | 1.02 | 7.21 | 208.01 | 39.78 | 273.26 | 0.6381 | 579.0 | 473.9 | |
| 0.44 | 9.60 | 0.28 | 6.14 | 6.47 | 207.86 | 39.62 | 272.08 | 0.6364 | 558.0 | 541.3 | |
| 0.00 | 1.15 | 0.00 | 0.73 | 6.92 | 207.91 | 39.67 | 272.79 | 0.6367 | 532.0 | 504.9 | |
| 0.00 | 0.79 | 0.00 | 0.51 | 6.82 | 207.66 | 39.42 | 272.62 | 0.6335 | 822.0 | 703.2 | |
| 0.00 | 6.43 | 0.00 | 4.10 | 7.06 | 207.61 | 39.37 | 273.00 | 0.6326 | 364.0 | 559.3 | |
| 0.00 | 1.15 | 0.00 | 0.73 | 6.71 | 207.49 | 39.26 | 272.43 | 0.6313 | 767.0 | 676.7 | |
| 0.00 | 4.84 | 0.00 | 3.08 | 6.27 | 207.29 | 39.06 | 271.72 | 0.6289 | 552.0 | 610.5 | |
| 3.08 | 7.31 | 1.95 | 4.64 | 7.34 | 207.09 | 38.85 | 273.42 | 0.6255 | 899.9 | 620.0 | |
| 0.00 | 1.06 | 0.00 | 0.66 | 5.98 | 206.34 | 38.10 | 271.17 | 0.6161 | 680.0 | 518.5 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 7.18 | 206.41 | 38.17 | 273.13 | 0.6164 | 577.0 | 520.2 | |
| 0.00 | 1.06 | 0.00 | 0.66 | 6.26 | 205.83 | 37.59 | 271.58 | 0.6088 | 759.0 | 571.6 | |
| 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. | |