Note: There are anomalous spikes in the flux plot that are probably due to the artifacts. Special care is necessary when using the given images in the archive.
EventID : 19940116_2317
Keyword : Flare
Start : 1994-01-16T22:59:35.000Z
Peak : 1994-01-16T23:17:30.000Z
End : 1994-01-16T23:45:01.000Z
Position: N07E71
X (arcsec) : -928
Y (arcsec) : 157
Maximum Correlation @17GHz (x10^-4) : 3419
Maximum Brightness Temperature @17GHz : 1.3e+08
Area_src/Area_beam @17GHz : 6.5
Maximum flux @17GHz (SFU) : 4662
Number of Impulsive fluctuation : 0
GOES: M6.1
NOAA Number:
Yohkoh HXT (L,M1,M2,H): (278,57,23,17)
Full sun 17GHz image. The flare region is indicated by the solid box.
movie
Partial 17GHz images. Color map shows brightness temperature,
contour shows 17GHz (r-l)/(r+l) levels,
where 'r' and 'l' indicates right- and
left-handed circularly-polarized components, respectively.
Field of View is 314. x 314. arcsec
Contour levels
of the thick lines are (r-l)/(r+l)=-0.1,-0.2,..
and those of the thin lines are (r-l)/(r+l)= +0.1,+0.2,...
Orange circle at top-left indicates the half-max. beam size
(top) NoRH 17 GHz correlation plot; Diamonds indicate the data points of event mode (50ms/100ms cadence):
(white line) 17 GHz
(bottom) Temporal derivative of correlation plot. Unit is (s^-1). Dotted line indicate 1 %/sec boundary.
SXT image overlaid with NoRH contours.
(green) NoRH 17GHz brightness temperature
in logarithmic scale.
Field of View is the same as Partial Image above
Contour levels
are log10(Tb) = 5,6,7,8,...
HXT image overlaid with NoRH contours.
(green) NoRH 17GHz brightness temperature
in logarithmic scale.
Field of View is the same as Partial Image above
Contour levels
are log10(Tb) = 5,6,7,8,...