Magnetic field is in a permanent state of flux. Magnetic north wanders, andevery few hundred thousand years the polarity flips so that a compass would point south instead of north. Moreover, the strength of the magnetic field constantly changes - and it is currently showing signs of significant weakening. (ESA)
Measurements made by Swarm over the past six months confirm the general trend of the field's weakening, with the most dramatic declines over the Western Hemisphere. But in other areas, such as the southern Indian Ocean, the magnetic field has strengthened since January.
The field is particularly weak over the South Atlantic Ocean - known as the South Atlantic Anomaly and the latest measurements confirm the movement of magnetic North towards Siberia.
The weak field has indirectly caused many temporary satellite 'hiccups' (called Single Event Upsets) as the satellites are exposed to strong radiation over this area. (ESA)
This animation shows changes in Earth's magnetic field from January to June 2014 as measured by ESA's Swarm trio of satellites:
© ESA/DTU Space‘Snapshot’ of the main magnetic field at Earth’s surface as of June 2014 based on Swarm data. The measurements are dominated by the magnetic contribution from Earth’s core (about 95%) while the contributions from other sources (the mantle, crust, oceans, ionosphere and magnetosphere) make up the rest. Red represents areas where the magnetic field is stronger, while blues show areas where it is weaker.
© ESA/AOES MedialabSwarm is ESA's first Earth observation constellation of satellites. The three identical satellites are launched together on one rocket. Two satellites orbit almost side-by-side at the same altitude – initially at about 460 km, descending to around 300 km over the lifetime of the mission. The third satellite is in a higher orbit of 530 km and at a slightly different inclination. The satellites’ orbits drift, resulting in the upper satellite crossing the path of the lower two at an angle of 90° in the third year of operations.
The different orbits along with satellites’ various instruments optimise the sampling in space and time, distinguishing between the effects of different sources and strengths of magnetism.
The different orbits along with satellites’ various instruments optimise the sampling in space and time, distinguishing between the effects of different sources and strengths of magnetism.
Its first results were presented today, June 19th, at the 'Third Swarm Science Meeting' in Copenhagen, Denmark.
"These initial results demonstrate the excellent performance of Swarm," said Rune Floberghagen, ESA's Swarm Mission Manager. "With unprecedented resolution, the data also exhibit Swarm's capability to map fine-scale features of the magnetic field."
Over the coming months, scientists will analyse the data to unravel the magnetic contributions from other sources, namely the mantle, crust, oceans, ionosphere and magnetosphere.
This will provide new insight into many natural processes, from those occurring deep inside our planet to space weather triggered by solar activity. In turn, this information will yield a better understanding of why the magnetic field is weakening.
Magnetic field:
#1 An introduction
#2 Why it matters
#3 Learning more with Swarm
Comment: Actual measurements of the intensity of the total geomagnetic field began in Gauss's observatories in 1840. Since then, its intensity has been continually decreasing at a rate of 6.3% per century. At this rate the intensity of the field will reach 0 in 1,600 years. This trend has been confirmed by studies of the magnetization in ancient clay pots, showing that the Earth's magnetic field was approximately twice as strong in Roman times.
To understand why this is happening, read the recently published Red Pill Press book, 'Earth Changes and the Human Cosmic Connection'.