Magnetic and Ionospheric Disturbances
Author | : |
Publisher | : |
Total Pages | : 104 |
Release | : 1961 |
Genre | : Sudden ionospheric disturbances |
ISBN | : |
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Author | : |
Publisher | : |
Total Pages | : 104 |
Release | : 1961 |
Genre | : Sudden ionospheric disturbances |
ISBN | : |
Author | : A. P. Nikolʹskiĭ |
Publisher | : |
Total Pages | : 54 |
Release | : 1962 |
Genre | : Geomagnetism |
ISBN | : |
Author | : Paul M. Kintner, Jr. |
Publisher | : John Wiley & Sons |
Total Pages | : 762 |
Release | : 2013-05-03 |
Genre | : Science |
ISBN | : 1118671716 |
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 181. Filling the need for a 20-year lag in substantial consideration of the midlatitude ionosphere, this volume focuses on work that takes advantage of GPS and UV imaging from satellites over the past decade, two methods that have profoundly transformed our understanding of this stratum of the atmosphere. Its interdisciplinary content brings together researchers of the solar wind, magnetosphere, ionosphere, thermosphere, polar and equatorial ionospheres, and space weather. Modeling and assimilative imaging of the ionosphere and thermosphere show for the first time the complex and global impact of midlatitude ionospheric storms. The editors invited the leading experts in the following areas to contribute the chapters herein: Characterization of Midlatitude Storms Electric Field Coupling From the Heliosphere and Inner Magnetosphere Thermospheric Control of the Midlatitude Ionosphere Ionospheric Irregularities Experimental Methods and New Techniques These themes were chosen to create a path for understanding the midlatitude ionosphere. They continue to be largely valid and represent a coherent division of the subject matter. They will be critical for understanding space weather during the upcoming solar maximum. This book was inspired by the Chapman Conference of the same name held January 2007.
Author | : I︠U︡riĭ Dmitrievich Kalinin |
Publisher | : |
Total Pages | : 96 |
Release | : 1961 |
Genre | : Magnetic storms |
ISBN | : |
Author | : |
Publisher | : |
Total Pages | : 96 |
Release | : 1961 |
Genre | : Sudden ionospheric disturbances |
ISBN | : |
Author | : A. P. NIKOL'SKIY |
Publisher | : |
Total Pages | : 1 |
Release | : 1962 |
Genre | : |
ISBN | : |
A comparison is made of the theory that the cause of irregular disturbances of the earth's magnetic field is solar corpuscles penetrating the ionosphere, and observations and experimental data. The movement of electrically charged particles in the field of a magnetic dipole substantiates the observations and theory.
Author | : Kenneth Davies |
Publisher | : |
Total Pages | : 60 |
Release | : 1972 |
Genre | : Ionosphere |
ISBN | : |
Author | : R. A. Zevakina |
Publisher | : |
Total Pages | : 98 |
Release | : 1968 |
Genre | : Ionospheric radio wave propagation |
ISBN | : |
The main features of ionospheric-geomagnetic storms and their probable causes are reviewed. Disturbances in short-wave radio propagation during such storms are discussed. The principles of short-term prediction of ionospheric-geomagnetic storms are summarized and all kinds of Izmiran's forecasts are described. The application of these forecasts and current ionospheric data to calculation of usable radio propagation frequencies is explained. This Manualiis of interest to radio-communication operators as well as to geophysicists dealing with this field of science.
Author | : B. N.. Bhargava |
Publisher | : |
Total Pages | : 4 |
Release | : 1968 |
Genre | : |
ISBN | : |
Author | : John Emory Jones |
Publisher | : |
Total Pages | : 478 |
Release | : 1969 |
Genre | : Doppler radar |
ISBN | : |
This report describes a radio investigation of traveling ionospheric disturbances carried out near Boulder, Colorado, over a 1-year period from June 1967 to June 1968. The three-dimensional motions of F2 layer disturbances were measured by the high frequency Doppler technique with spaced transmitters and at several probing frequencies. Horizontal motions were determined by cross-correlating three signals on frequencies near 5 MHz, whose reflection points were approximately at the corners of a horizontal equilateral triangle with 40-km sides. Vertical motions were determined from cross-correlation of signals on frequencies of 3.3, 4.0, and 5.1 MHz, whose reflection points were aligned vertically.