IPL description

Wellcome to the IPL web portal

The Image Processing Laboratory (IPL) of the University of Valencia consists of research groups with a common technological mission: imaging from satellite data and remote sensing.

The 3rd International Symposium on Recent Advances in Quantitative Remote Sensing: RAQRS'III

This symposium hosted in Torrent (Valencia)-Spain, is THE THIRD INTERNATIONAL SYMPOSIUM ON “RECENT ADVANCES IN QUANTITATIVE REMOTE SENSING” organised by the Global Change Unit, University of Valencia. More info in http://ipl.uv.es/raqrs

Gustau Camps-Valls, “Distinguished Lecturer” de la IEEE Geoscience and Remote Sensing Society


Gustau impartirá lecciones magistrales sobre tratamiento avanzado de datos y métodos automáticos ( «machine learning») en todo el mundo.

La IEEE Geoscience and Remote Sensing Society (http://www.grss-ieee.org/) es una de las sociedades profesionales de expertos en teledetección, Geociencia y observación de la tierra más importantes en el mundo.

First XIPE Science Meeting

The first science conference on the  XIPE mission will be in Valencia, Spain (24-26 May 2016)
All information about the first XIPE science meeting are available HERE.


The FLuorescence EXplorer (FLEX) mission proposes a satellite for the global monitoring of steady-state chlorophyll fluorescence in terrestrial vegetation.


UFFO stands for Ultra Fast Flash Observatory and it is a dedicated mission to study the early stages of Gamma-Ray Bursts (GRBs). The GACE  has developed  UBAT, the X-ray trigger detector for UFFO.

To see the launch:

Observations of Magnetic Elements in the Quiet Sun Internetwork

We present here the analysis of high-resolution images of the quiet Sun at disk center taken with the Solar Optical Telescope (SOT) on board Hinode in the CN bandhead (388.35 nm) and magnetograms in the Mg I line (517.27 nm). These observations are complemented with data from the Swedish 1m Solar Telescope (SST). All data sets were obtained during the Hinode/Canary Islands joint campaign (HOP 0014) in September, 2007. In particular, we investigate the morphology, radiative and magnetic properties of small-scale elements in the solar atmosphere.

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