mioara mandea - research observatory

Why all the effort?

Direct measurements of the Earth’s magnetic field are continuously made at magnetic observatories around the world, and are also obtained from a variety of sources, including oceanographic surveys, land-based surveys, aircraft, and even satellites. All of this data collection has led some to ask, "Why all the effort?" For me, there are two main reasons that stand out. First, very few physical quantities can provide a historical record that can be measured today. While studies of seismology and the Earth's gravity field have revealed many secrets about our planet’s interior, they do not offer a timeline through which we can observe how these measurements have changed over time. Measurements that can be examined retroactively are extremely valuable for making inferences about the Earth's past conditions. The second reason relates to the fact that the magnetic field we measure is not a single entity, but a combination of fields produced by different sources. The Earth's primary magnetic field is generated in the fluid outer core through a self-exciting dynamo process. In addition to the core field, the magnetic field observable at the Earth's surface is also influenced by sources in the crust, the ionosphere, and the magnetosphere. The geomagnetic field varies on a wide range of spatial and temporal scales, and these variations can now be described in both the space and time domains, from low-frequency to high-frequency changes. Earth’s magnetic field is highly dynamic, and its variations—particularly those linked to solar activity—can have significant effects on modern technology. For instance, geomagnetic disturbances can impact power grids, cause blackouts, and interfere with communication systems, such as radios and telephones.

Understanding and mapping these variations has been a central focus of my research, contributing to a large international effort aimed at improving our knowledge of Earth's magnetic field. In the following sections, I will provide a more detailed account of my work and explain why the study of planetary magnetic fields—such as those of Mars, Mercury, and Venus—is also of great interest to me. For more detailed information, my publications list provides further insights into this field of research.

Ancient magnetic data

Before the establishment of modern geomagnetic observatories and the development of absolute methods for measuring magnetic intensity (such as those introduced by Gauss in the 1830s), magnetic observations were made primarily by mariners engaged in merchant and naval shipping. These early observations, mostly focused on declination, extend the global dataset of magnetic field variations back to the early 16th century. As part of my research, I have discovered new sources of historical magnetic data and reviewed early attempts to describe the Earth's magnetic field, including the work of Nautonier (1602). This work led me to examine old books and maps, including measurements taken by the French Navy and some of the first geomagnetic maps. I have also conducted a study on magnetic field variations in Western Europe over the last few centuries, focusing on data from cities like Paris, London, Munich, and Bucharest.

Observatories

Magnetic observatories play a crucial role in measuring and monitoring the Earth's magnetic field. These observatories record absolute vector observations of the geomagnetic field with high precision and continuous time resolution—often with intervals as short as one minute. There are two main categories of instruments used in these observatories: variometers, which measure the geomagnetic field in relative units, and absolute instruments, which measure the field in terms of absolute physical units or universal constants. In addition to my efforts in France to maintain a network of global magnetic observatories, I have also been involved in the development of a geomagnetic observatory network run by Germany.

Other ground direct observations

In addition to observatories, the Earth's magnetic field is studied through repeat stations and surveys conducted on land, from aircraft, and aboard ships. Repeat stations are designated sites where high-quality magnetic observations are made at regular intervals—ranging from a few hours to a few days—over a period of years. These stations are primarily used to track changes in the core-generated magnetic field. I have been involved in field campaigns across various regions, from Romania to France and Germany, as well as in Southern Africa, contributing valuable magnetic data to improve our understanding of Earth's magnetic variations.

In 2001, I participated in an expedition to locate the North Magnetic Pole, a challenging but exciting mission that provided the opportunity to take absolute magnetic measurements in extreme conditions.

Satellites

Since the 1960s, the Earth's magnetic field has been intermittently observed by satellites. The first dedicated magnetic field mission, MAGSAT (1979-1980), provided valuable data, though its short mission duration and sun-synchronous orbit limited its ability to capture long-term trends.

A major improvement came with the launch of the Ørsted satellite, which, 20 years after MAGSAT, provided continuous measurements of the geomagnetic field. While Ørsted’s higher orbit led to some resolution limitations, it represented a significant leap forward in our understanding of the Earth's magnetic field.

The CHAMP mission (2000–2010) further advanced our capabilities. With its high-inclination orbit (87°) and low altitude (starting at 454 km), CHAMP provided highly accurate data, greatly improving our understanding of secular variations in the magnetic field. This satellite’s five-year mission, along with its advanced instrumentation, significantly enhanced the precision of geomagnetic measurements, offering new perspectives on the role of magnetic field data in studying the solid Earth.

The Swarm mission, launched in 2013, consists of a constellation of three identical satellites designed to measure the Earth’s magnetic field with unprecedented accuracy. Swarm is part of the European Space Agency’s Earth Explorer program, and its primary scientific objective is to provide the most comprehensive survey of the geomagnetic field and its temporal evolution. This mission aims to improve our understanding of the Earth’s interior and the connections between the Earth and the Sun. I have been involved in this mission since its inception, and it continues to be one of the key missions I oversee within the Solid Earth program. The French contribution to the Swarm mission includes the supply of absolute magnetometers by CNES.

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