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Table 1 Characteristics of different types of satellites with SLR retroreflectors used in the analysis

From: Determination of SLR station coordinates based on LEO, LARES, LAGEOS, and Galileo satellites

Satellite

Type

Main mission objective

Launch date (mission end)

Altitude (km)

Retroreflector characteristics

POD techniques

Attitude information

LARES

Spherical geodetic

Relativistic effects, gravity field

02.2012

1450

Surface covered with 92 corner cubes

SLR

LAGEOS-1 LAGEOS-2

Spherical geodetic

ITRF, geocenter, gravity field, ERPs

05.1976 10.1992

5850 5625

Surface covered with 426 corner cubes

SLR

GRACE-A GRACE-B

LEO

Gravity field, Ocean and Sea monitoring

03.2002 (10.2017)

450–330

Pyramid-shaped array,4 cubes

SLR, GNSS

Quaternions, 5-s interval

SWARM-A SWARM-B SWARM-C

LEO

Earth Magnetic field, gravity field

11.2013

460

Pyramid-shaped array,4 cubes

SLR, GNSS

Quaternions, 1-s interval

530

460

TerraSAR-X

LEO

Remote sensing

06.2007

514

Pyramid-shaped array,4 cubes

SLR, GNSS

Quaternions, 10-s interval

Jason-2

LEO

Ocean surface topography

06.2008 (10.2019)

1336

Hemispherical surface, 9 cubes

SLR, GNSS, DORIS

Quaternions, 30-s interval

Sentinel-3A

LEO

Ocean and land monitoring, ocean topography

02.2016

815

Spherical surface, 7 cubes

SLR, GNSS, DORIS

Quaternions, 1-s interval

Galileo (3 IOV 10 FOC)

GNSS

Positioning, navigation, timing

IOV 10.2011 FOC 08.2014

17 178– 23 222

Arrays of 84 cubes (IOV) and 60 cubes (FOC)

SLR, GNSS

Yaw-steering