scholarly journals Drivers of Upper Atmosphere Climate Change

Eos ◽  
2020 ◽  
Vol 101 ◽  
Author(s):  
Sarah Stanley
Keyword(s):  
Climate Change ◽  
Magnetic Field ◽  
Carbon Dioxide ◽  
Upper Atmosphere ◽  
Earth’S Magnetic Field ◽  
Temperature Trends ◽  
Earth's Magnetic Field ◽  
New Research

New research confirms the influence of carbon dioxide on long-term temperature trends in the upper atmosphere, but changes in Earth’s magnetic field also play a key role.

scholarly journals Slow variations of the Earth’s magnetic field: technical, methodological and organizational features of measurements

2019 ◽  
Vol 127 ◽  
pp. 02026
Author(s):  
Sergey Y. Khomutov
Keyword(s):  
Magnetic Field ◽  
Global Network ◽  
Earth’S Magnetic Field ◽  
Measurement Systems ◽  
Long Term Stability ◽  
Earth's Magnetic Field ◽  
Methodological Problems ◽  
Organizational Features ◽  
Magnetic Observatories

Variations of the Earth’s magnetic field with times of several years or more reflect the processes within the planet and cause great scientific interest. Over the past 100 years the regular observations at magnetic observatories (MOs) and repeat stations are the only experimental basis for studying such variations. In recent decades, satellite measurements have complemented ground-based measurements, thus partially solving the problems of spatially highly heterogeneous global network of magnetic observatories. Absolute observations are made at MOs to get the total field intensity vector. Until now, these measurements are performed manually, they are labor intensity and subject to many factors, that are often poorly controlled and reduce the reliability of the results, especially over long periods of time (years and decades), including (1) systematic errors of used magnetometers; (2) magnetic pollution of the absolute pavilion and its surroundings (at a distance of the first hundred meters); (3) instability of the pillars and remote target required to determine magnetic declination; (4) changes of observers and their weak qualification. Significant methodological problems arise if MO is moved to new location without special activity or infrastructure of MO (pavilions or pillars) is changed without careful control. For long-term stability and reliability of measurements, magnetic observatories were joined in IAGA network and then INTERMAGNET. Within these networks, requirements and standards have been defined, absolute magnetometers are compared every two years and observers are being trained. Modern hardware technologies allow to solve partially problems the automation of absolute observations, the self-calibration of the magnetometers, the checking of the MO’s magnetic environment, etc. Fully automated measurement systems help to expand the MO network.

Long-term variations of the external and internal components of the Earth's magnetic field

1986 ◽  
Vol 91 (B5) ◽  
pp. 4787 ◽  
Author(s):  
J. Gavoret ◽  
D. Gibert ◽  
M. Menvielle ◽  
J. L. Le Mouël
Keyword(s):  
Magnetic Field ◽  
Earth’S Magnetic Field ◽  
Earth's Magnetic Field ◽  
Long Term Variations

scholarly journals Long-term changes in solar quiet (Sq) geomagnetic variations related to Earth's magnetic field secular variation

2013 ◽  
Vol 118 (6) ◽  
pp. 3712-3718 ◽  
Author(s):  
Blas F. de Haro Barbas ◽  
Ana G. Elias ◽  
Ingrid Cnossen ◽  
Marta Zossi de Artigas
Keyword(s):  
Magnetic Field ◽  
Secular Variation ◽  
Earth’S Magnetic Field ◽  
Geomagnetic Variations ◽  
Long Term Changes ◽  
Earth's Magnetic Field

scholarly journals II. The lunar diurnal magnetic variation at Greenwich and other observatories

1926 ◽  
Vol 225 (626-635) ◽  
pp. 49-91 ◽  
Keyword(s):  
Magnetic Field ◽  
Electrical Conductivity ◽  
Diurnal Variation ◽  
Solid Earth ◽  
Upper Atmosphere ◽  
Earth’S Magnetic Field ◽  
Terrestrial Magnetism ◽  
Magnetic Variation ◽  
Earth's Magnetic Field ◽  
The Subject

§ 1. The present research forms part of a wider investigation of terrestrial magnetism, the main object of which is the study of certain electrical phenomena that are associated with solar emissions absorbed in the upper atmosphere, and with the systematic motions of the upper atmosphere. The subject also bears on the electrical conductivity of the solid earth and oceans. The results are briefly discussed from this standpoint in Part IV. The immediate subject of the paper is the lunar diurnal variation of the earth’s magnetic field, and particularly that of the declination at Greenwich, although the results of extensive reductions for other elements, at Batavia, Zikawei, and Pavlovsk, are also included.

Does Earth's magnetic field secular variation control centennial climate change?

2005 ◽  
Vol 236 (1-2) ◽  
pp. 339-347 ◽  
Author(s):  
Yves Gallet ◽  
Agnès Genevey ◽  
Frédéric Fluteau
Keyword(s):  
Climate Change ◽  
Magnetic Field ◽  
Secular Variation ◽  
Earth’S Magnetic Field ◽  
Earth's Magnetic Field
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