class sunpy.lightcurve.NoRHLightCurve(data, meta=None)[source] [edit on github]

Bases: sunpy.lightcurve.LightCurve

Nobeyama Radioheliograph Correlation LightCurve.

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.


>>> import sunpy.lightcurve
>>> norh = sunpy.lightcurve.NoRHLightCurve.create('~/Data/norh/tca110607')  # doctest: +SKIP
>>> norh = sunpy.lightcurve.NoRHLightCurve.create('2011/08/10')  # doctest: +SKIP
>>> norh = sunpy.lightcurve.NoRHLightCurve.create('2011/08/10',wavelength='34')  # doctest: +SKIP
>>> norh.peek()   # doctest: +SKIP


Methods Summary

peek(**kwargs) Plots the NoRH lightcurve

Methods Documentation

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

Plots the NoRH lightcurve

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

Parameters:**kwargs (dict) – Any additional plot arguments that should be used when plotting.