The deviation of Universal Time from atomic time, expressed as UT1-UTC, reflects the irregularities of the Earth rotation speed and is key to precise geodetic applications which depend on the transformation between celestial and terrestrial reference frames. A rapidly varying quantity such as UT1-UTC demands observation scenarios enabling fast delivery of good results. These criteria are currently met only by the Very Long Baseline Interferometry (VLBI) Intensive sessions. Due to stringent requirements of a fast UT1-UTC turnaround, the observations are limited to a few baselines and a duration of one hour. Hence, the estimation of UT1-UTC from Intensives is liable to constraints and prone to errors introduced by inaccurate a priori informat...
The latency of UT1 measurement with Very Long Baseline Interferometry (VLBI) has been greatly reduce...
Geodetic Very Long Baseline Interferometry (VLBI) is an essential technique for space geodesy. It is...
VLBI is the only space-geodetic technique which gives direct access to the Earth's phase of rotation...
The deviation of Universal Time from atomic time, expressed as UT1-UTC, reflects the irregularities ...
One hour single baseline VLBI sessions, so-called Intensives, are routinely observed to derive UT1-U...
Very Long Baseline Interferometry (VLBI) Intensives are one-hour single baseline sessions to provide...
One of the main tasks of Very Long Baseline Interferometry (VLBI) is the rapid determination of the ...
Very Long Baseline Interferometry (VLBI) is a unique space-geodetic technique capable of direct obse...
The time-dependent variations in the rotation and orientation of the Earth are represented by a set ...
Very Long Baseline Interferometry (VLBI) is a space-geodetic technique that is uniquely capable of d...
We present earth rotation results from the ultra-rapid operations during the continuous VLBI campaig...
We present first results for the determination of UT1-UTC using the VLBI Global Observing System (VG...
In principle, we can use geodetic Very Long Baseline Interferometry (VLBI) measurements to calculate...
Very Long Baseline Interferometry (VLBI) is an essential technique forspace-geodesy. It realizes the...
A series of experiments was conducted during the last decade to explore the capability of very long ...
The latency of UT1 measurement with Very Long Baseline Interferometry (VLBI) has been greatly reduce...
Geodetic Very Long Baseline Interferometry (VLBI) is an essential technique for space geodesy. It is...
VLBI is the only space-geodetic technique which gives direct access to the Earth's phase of rotation...
The deviation of Universal Time from atomic time, expressed as UT1-UTC, reflects the irregularities ...
One hour single baseline VLBI sessions, so-called Intensives, are routinely observed to derive UT1-U...
Very Long Baseline Interferometry (VLBI) Intensives are one-hour single baseline sessions to provide...
One of the main tasks of Very Long Baseline Interferometry (VLBI) is the rapid determination of the ...
Very Long Baseline Interferometry (VLBI) is a unique space-geodetic technique capable of direct obse...
The time-dependent variations in the rotation and orientation of the Earth are represented by a set ...
Very Long Baseline Interferometry (VLBI) is a space-geodetic technique that is uniquely capable of d...
We present earth rotation results from the ultra-rapid operations during the continuous VLBI campaig...
We present first results for the determination of UT1-UTC using the VLBI Global Observing System (VG...
In principle, we can use geodetic Very Long Baseline Interferometry (VLBI) measurements to calculate...
Very Long Baseline Interferometry (VLBI) is an essential technique forspace-geodesy. It realizes the...
A series of experiments was conducted during the last decade to explore the capability of very long ...
The latency of UT1 measurement with Very Long Baseline Interferometry (VLBI) has been greatly reduce...
Geodetic Very Long Baseline Interferometry (VLBI) is an essential technique for space geodesy. It is...
VLBI is the only space-geodetic technique which gives direct access to the Earth's phase of rotation...