PAZ Satellite Mission Summary

CEOS EO HANDBOOK – MISSION SUMMARY - PAZ -

Full Name

PAZ
aka SEOSAR

Status

Operational (extended)

Mission Agencies

HISDESAT, CDTI , INTA

Launch Date

22 Feb 2018

Mission Links

mission site

EOL Date

Sep 2028

EO Portal Info

NORAD Catalog #

43215 (TLE)

International Designator

2018-020A

Orbit Type

Sun-synchronous

Orbit Period

95 minutes

Orbit Sense

Ascending

Orbit Inclination

97.44 deg

Orbit Altitude

514 km

Orbit Longitude

Orbit LST

18:00

Repeat Cycle

11 days

Objectives and Applications

Security, land use, urban management, environmental monitoring, risk management.

Mission Measurements

Category	Parameter	Instrument(s)
Atmosphere	Atmospheric Winds	Paz SAR-X
Land	Vegetation	Paz SAR-X
	Multi-purpose imagery (land)	Paz SAR-X

Mission Instruments

Paz SAR-X - X Band Synthetic Aperture Radar

Featured Datasets
More Datasets

PAZ Full Archive and New Tasking
Jan-2018

The PAZ (Spanish for “peace”) satellite, launched on 22 February 2018, is owned and operated by Hisdesat, and is based on the use of a high-resolution X-band Synthetic Aperture Radar (SAR). The satellite operates in the same orbit as its twin satellites TerraSAR-X and TanDEM-X, and the three satellites work together as a constellation. The objective of the PAZ mission is to provide imagery for both civilian and security and defence requirements. ESA offers worldwide access to PAZ data (both archive and new tasking) via the TPM scheme. Read more

PAZ ESA Archive
Jan-2018

OpenSearch Datasets

Selected IDN OpenSearch Results (search all 4 )
GPS Radio Occultation Boundary Layer Depth Annual L3 V2 (GPSROZPBLA) at GES DISC $This dataset provides an annual average climatology of planetary boundary layer (PBL) height derived from COSMIC/FORMOSAT-3, TerraSAR-X, KOMPSAT-5, and PAZ Global Positioning System (GPS) radio occultation (RO) measurements. The COSMIC/FORMOSAT-3 mission consists of a six-satellite constellation launched in 2006. Each satellite carries an Integrated GPS Occultation Receiver (IGOR) GPS receiver and is equipped with fore and aft looking antenna to track both setting and rising occultations. The constellation provides globally distributed measurements across different local times. The instrument tracks the L-band microwave signal broadcast by a GPS satellite in a limb-viewing geometry. The IGOR receivers are capable of tracking the GPS signals in open loop through the middle to lower troposphere, which is essential for obtaining data with high quality for PBL height estimation, especially at low latitudes. The refractivity profiles form the basis for this PBL height product. For each occultation, the PBL height is calculated as the height where the vertical gradient of the refractivity (dN/dz) is minimum. This algorithm is designed to locate the height where a large vertical change in refractivity occurs, corresponding to the transition from the free troposphere to the PBL. More details can be found in Ao et al. (2012). This is the latest version of this collection which supercedes previous versions.$
GPS Radio Occultation Boundary Layer Depth Seasonal L3 V2 (GPSROZPBLS) at GES DISC $This dataset provides a seasonal average climatology of global planetary boundary layer (PBL) height derived from COSMIC/FORMOSAT-3, TerraSAR-X, KOMPSAT-5, and PAZ Global Positioning System (GPS) radio occultation (RO) measurements. The COSMIC/FORMOSAT-3 mission consists of a six-satellite constellation launched in 2006. Each satellite carries an Integrated GPS Occultation Receiver (IGOR) GPS receiver and is equipped with fore and aft looking antenna to track both setting and rising occultations. The constellation provides globally distributed measurements across different local times. The instrument tracks the L-band microwave signal broadcast by a GPS satellite in a limb-viewing geometry. The IGOR receivers are capable of tracking the GPS signals in open loop through the middle to lower troposphere, which is essential for obtaining data with high quality for PBL height estimation, especially at low latitudes. The refractivity profiles form the basis for this PBL height product. For each occultation, the PBL height is calculated as the height where the vertical gradient of the refractivity (dN/dz) is minimum. This algorithm is designed to locate the height where a large vertical change in refractivity occurs, corresponding to the transition from the free troposphere to the PBL. More details can be found in Ao et al. (2012). This is the latest version of this collection which supersedes previous versions.$
PAZ ESA archive

PAZ Full Archive and New Tasking

Selected FedEO OpenSearch Results (view all 2 results: browser , table )
PAZ Full Archive and New Tasking

PAZ ESA archive

Want to explore more? Read about FedEO by ESA or click here to search FedEO or CMR OpenSearch by NASA