Single-frequency total flux observations at 127MHz

Solar Radio Emission
DAILY DATA                     NOVEMBER 2007

DATE
/UT/		OBS.
START		PERIOD
END		FLUX DENSITY 
9-12  12-15
/SU/
9-15		VARIABILITY
9-12  12-15  9-15
106301500
           2         2
2
    0        0       0
20630*1400
           2         2
2
    0        0        0
30630*1500
           2         2
2
    0        0        0
406301500
           2         2
2
    0        0        0
506401120
           2         -
2
    0        -        0
606401120
           3         -
3
    0        -        0
706401440
           2         2
2
    0        0        0
806401340
           2         2
2
    0        0        0
906401440
           2         2
2
    0        0        0
1006401440
           2         2
2
    0        0        0
1106501430
           2         2
2
    0        0        0
1206501430
           2         2
2
    0        0        0
1307001430
           3         2
2
    0        0        0
1407001430
           2         2
2
    0        0        0
1507001430
           2         2
2
    0        0        0
1607001430
           3         2
3
    0        0        0
17 - - 
           -         -
-
    -        -        -
18 - - 
           -         -
-
    -        -        -
1912101430
           -         4
4
    -        0        0
2007001430
           3         3
3
    0        0        0
2107201430
           3         3
3
    0        0        0
2207201430
           2         3
2
    0        0        0
2307201430
           2         3
2
    0        0        0
2407201430
           2         3
2
    0        0        0
2507201430
           2         4
3
    0        0        0
2607301430
           2         3
3
    0        0        0
2707301430
           2         3
3
    0        0       0
2807301410
           2         3
3
    0        0        0
290730*1410
           2         3
2
300730*1410
           3         4
3
    0        0        0


INTERRUPTIONS GREATER THAN 10 MIN:
* SOMETIMES DISTURBED
MEAN: 2.4