UT1

Universal Time No.1

Other
Introduced in Rel-9
UT1 is a precise form of Universal Time corrected for polar motion, representing the Earth's actual rotational angle. In 3GPP, it is used for high-accuracy timing in positioning and navigation systems, such as Assisted GNSS, to ensure precise location determination and network synchronization.

Description

Universal Time No.1 (UT1) is a specific realization of Universal Time that accounts for polar motion—the movement of the Earth's rotational axis relative to its crust. It is derived from observations of distant quasars using Very Long Baseline Interferometry (VLBI), providing a measure of the Earth's rotation angle with high precision. UT1 is essential because it represents true solar time, accounting for irregularities in the Earth's rotation, such as length-of-day variations and seasonal effects. Unlike Coordinated Universal Time (UTC), which uses leap seconds to stay close to UT1, UT1 itself is a continuous time scale without discontinuities, making it ideal for scientific and technical applications requiring smooth time progression. In 3GPP standards, UT1 is primarily referenced in specifications like 36.355 and 37.355 for location services, particularly in Assisted Global Navigation Satellite System (A-GNSS) protocols. It enables mobile devices to obtain accurate time information from the network, which is crucial for calculating position fixes by synchronizing with satellite signals. The integration of UT1 into 3GPP ensures that telecommunications networks can provide precise timing aids to user equipment, enhancing the accuracy of location-based services. This is achieved through network elements like Location Management Functions (LMF) that disseminate UT1 data as part of assistance information. The role of UT1 extends to network synchronization scenarios where Earth-relative timing is required, supporting applications in aviation, maritime, and other sectors dependent on exact rotational time.

Purpose & Motivation

UT1 exists to provide a high-precision, Earth-rotation-based time reference that corrects for polar motion, addressing the need for accurate astronomical timing in telecommunications. It solves the problem of aligning network timing with the Earth's actual rotation, which is critical for positioning systems like GNSS that rely on precise satellite synchronization. Historically, UT1 was developed to refine Universal Time by accounting for axial wobble, offering a more stable reference for scientific observations and navigation. In 3GPP, starting from Release 9, UT1 was incorporated to enhance location services, enabling networks to deliver precise time assistance to mobile devices for faster and more accurate position fixes. This addresses limitations in earlier timing methods that might not account for rotational variations, improving performance in urban canyons or indoor environments where satellite signals are weak. The motivation for including UT1 stems from the growing demand for reliable location-based applications, such as emergency services and asset tracking, which require robust time references to function effectively across global networks.

Key Features

  • Corrects Universal Time for polar motion
  • Provides continuous Earth-rotation angle measurement
  • Used in 3GPP for A-GNSS timing assistance
  • Enhances accuracy of location-based services
  • Supports network synchronization with astronomical time
  • Referenced in LTE and 5G positioning protocols

Evolution Across Releases

Rel-9 Initial

Introduced as a precise time reference for location services in 3GPP, specifically for Assisted GNSS (A-GNSS) to improve positioning accuracy. Initial architecture involved integrating UT1 data into network assistance information, allowing user equipment to synchronize with satellite systems using Earth-rotation-corrected time for faster and more reliable position fixes.

Defining Specifications

SpecificationTitle
TS 36.355 3GPP TR 36.355
TS 37.355 3GPP TR 37.355