I. Introduction
Ionospheric propagation delay is one of the most relevant error sources in low-frequency spaceborne synthetic aperture radar (SAR) interferograms. SAR interferometry is a successful technique used to measure the Earth's topography and to study geophysical processes such as earthquakes, volcanoes, landslides, and glacier movements. Unfortunately, the accuracy of these measurements is limited by distortions that the ionosphere causes in the propagation of microwaves. In SAR interferograms, topography and ground deformation signals are mixed with ionospheric disturbances [1]. In order to avoid that the ionospheric propagation delay is confused with ground signals, it has to be estimated and removed [2]. The ionospheric distortions on the propagation of microwaves cause an additional group delay and a phase advance on SAR images, whose magnitude is inversely proportional to the frequency of the system. For this reason, L-band SAR systems such as the Advanced Land Observing Satellite (ALOS) Phased-Array type L-band SAR (PALSAR), its follow-up, i.e., ALOS-2, or the future Tandem-L, due to the lower frequency, experience more severe ionospheric distortions compared with C-band or X-band systems.