Add to ORKGThis presentation will discuss the results of an investigation looking into the physical causes of the observed annual variations in Aqua's mean local time and inclination. This provides a deeper insight into the forces driving Aqua's orbit. It was found that the Sun and the Moon's gravitational effects combine to cause Aqua's inclination rate to vary, peaking around December of each year, and reaching a minimum around August of each year
Continuous observations of solar oscillations over the last twenty years have provided an opportuni...
The purpose of this resource is to understand what causes the Earth's seasons with a focus on the Ea...
The Earth’s revolution is modified by changes in inclination of its rotation axis. Its trajectory is...
Using Greenwich and SOON sunspot group data during the period 1874 -- 2005, we find that the sums of...
Significant error has been observed in the long term prediction of the Mean Local Time of the Ascend...
This will be presented at the International Earth Science Constellation Mission Operations Working G...
Context. Solar active longitudes and their rotation have been studied for a long time usin...
We investigate the relationship between interdiurnal variation geomagnetic activity indices, IDV and...
Each Inclination Adjust Maneuver (IAM) series requires a post-series analysis along with a long term...
Earth’s orbit and rotation produces systematic variations in geomagnetic activity, most notably via ...
Information on the rotation rate of the corona, and its variation over latitude and solar cycle, is ...
International audienceVarious manifestations of solar activity are not uniformly distributed with he...
We analyse the widely-used international/ Zürich sunspot number record, R, with a view to quantifyin...
International audienceThe tendency of the atmospheric angular momentum (AAM) is investigated using a...
Aims. We seek the long-term variations close to the length of a solar cycle in the mean meridiona...
Continuous observations of solar oscillations over the last twenty years have provided an opportuni...
The purpose of this resource is to understand what causes the Earth's seasons with a focus on the Ea...
The Earth’s revolution is modified by changes in inclination of its rotation axis. Its trajectory is...
Using Greenwich and SOON sunspot group data during the period 1874 -- 2005, we find that the sums of...
Significant error has been observed in the long term prediction of the Mean Local Time of the Ascend...
This will be presented at the International Earth Science Constellation Mission Operations Working G...
Context. Solar active longitudes and their rotation have been studied for a long time usin...
We investigate the relationship between interdiurnal variation geomagnetic activity indices, IDV and...
Each Inclination Adjust Maneuver (IAM) series requires a post-series analysis along with a long term...
Earth’s orbit and rotation produces systematic variations in geomagnetic activity, most notably via ...
Information on the rotation rate of the corona, and its variation over latitude and solar cycle, is ...
International audienceVarious manifestations of solar activity are not uniformly distributed with he...
We analyse the widely-used international/ Zürich sunspot number record, R, with a view to quantifyin...
International audienceThe tendency of the atmospheric angular momentum (AAM) is investigated using a...
Aims. We seek the long-term variations close to the length of a solar cycle in the mean meridiona...
Continuous observations of solar oscillations over the last twenty years have provided an opportuni...
The purpose of this resource is to understand what causes the Earth's seasons with a focus on the Ea...
The Earth’s revolution is modified by changes in inclination of its rotation axis. Its trajectory is...