  MASER (Measurements, Analysis, and Simulation of Emission in the Radio range)
is a comprehensive infrastructure dedicated to time-dependent low frequency
radio astronomy (up to about 50 MHz). The main radio sources observed in this
spectral range are the Sun, the magnetized planets (Earth, Jupiter, Saturn),
and our Galaxy, which are observed either from ground or space. Ground
observatories can capture high resolution data streams with a high sensitivity.
Conversely, space-borne instruments can observe below the ionospheric cut-off
(at about 10 MHz) and can be placed closer to the studied object. Several tools
have been developed in the last decade for sharing space physics data. Data
visualization tools developed by various institutes are available to share,
display and analyse space physics time series and spectrograms. The MASER team
has selected a sub-set of those tools and applied them to low frequency radio
astronomy. MASER also includes a Python software library for reading raw data
from agency archives.
