NoRHTimeSeries

class sunpy.timeseries.NoRHTimeSeries(data, header, units, **kwargs)[source] [edit on github]

Bases: sunpy.timeseries.GenericTimeSeries

Nobeyama Radioheliograph Correlation Lightcurve TimeSeries.

Nobeyama Radioheliograph (NoRH) is a radio telescope dedicated to observing the Sun. It consists of 84 parabolic antennas with 80 cm diameter, sitting on lines of 490 m long in the east/west and of 220 m long in the north/south. It observes the full solar disk at 17 GHz and 34 GHz with a temporal resolution down to 0.1 second resolution (typically 1 s). It is located in Japan at 35.941667, 138.475833.

Its first observation was in April, 1992 and daily 8-hour observations are available starting June, 1992.

Examples

>>> import sunpy.data.sample
>>> import sunpy.timeseries
>>> norh = sunpy.timeseries.TimeSeries(sunpy.data.sample.NORH_TIMESERIES, source='NoRH')
>>> norh.peek()   

References

Methods Summary

is_datasource_for(**kwargs) Determines if header corresponds to a Nobeyama Radioheliograph Correlation lightcurve
peek(**kwargs) Plots the NoRH lightcurve TimeSeries

Methods Documentation

classmethod is_datasource_for(**kwargs)[source] [edit on github]

Determines if header corresponds to a Nobeyama Radioheliograph Correlation lightcurve

peek(**kwargs)[source] [edit on github]

Plots the NoRH lightcurve TimeSeries

(Source code, png, hires.png, pdf)

../_images/sunpy-timeseries-NoRHTimeSeries-1.png
Parameters:**kwargs (dict) – Any additional plot arguments that should be used when plotting.
Returns:fig (Figure) – A plot figure.