NoRHTimeSeries

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

Bases: sunpy.timeseries.timeseriesbase.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 a 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 second).

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 TimeSeries.

peek(**kwargs)

Plot the NoRH lightcurve TimeSeries.

Methods Documentation

classmethod is_datasource_for(**kwargs)[source]

Determines if header corresponds to a Nobeyama Radioheliograph Correlation TimeSeries.

peek(**kwargs)[source]

Plot the NoRH lightcurve TimeSeries.

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

../_images/sunpy-timeseries-sources-NoRHTimeSeries-1.png
Parameters

**kwargs (dict) – Additional plot keyword arguments that are handed to plot functions.