Lower Thermosphere Density Variations in the Southern Hemisphere

Lower Thermosphere Density Variations in the Southern Hemisphere
Author: F. A. Marcos
Publisher:
Total Pages: 23
Release: 1972
Genre:
ISBN:

Profiles of the neutral atmospheric density have been obtained at high and middle latitudes in the southern hemisphere from OV1-15 (SPACES) satellite accelerometer measurements. The data were obtained during a geomagnetically quiet period near the equinox, 24-28 September 1968, when the satellite was in a nearly down-dusk orbit. Perigee moved from 50 degrees S to 65 degrees S during this period. Measurements were made in the altitude range 170-250 km. Density values at dusk at high latitudes (before perigee) are less than those at midlatitudes (after perigee). The average difference between the high latitude and midlatitude data is 15 percent. A longitudinal variation is superimposed on the latitudinal gradients. Enhanced densities at high southern latitudes are found at longitudes near the south geomagnetic pole. (Author).

Atlas of Northern Hemisphere Density Between 30 and 60 Km

Atlas of Northern Hemisphere Density Between 30 and 60 Km
Author: Arthur J. Kantor
Publisher:
Total Pages: 56
Release: 1982
Genre: Atmosphere, Upper
ISBN:

Mean seasonal density charts for the Northern hemisphere for 5-km increments of altitude between 30 and 60 km are presented in this report, along with estimates of the day-to-day variations around the mean seasonal values. This meets the need for a climatology of atmospheric density at constant altitudes above radiosonde levels. These charts are based on compilations of data by workers at the National Meteorological Center, NOAA, who combined data from TIROS operational vertical sounders with meteorological rocketsonde observations to produce once-weekly analyses of height and temperature fields for the Northern hemisphere at the 5, 2, 1, and .4 mb levels for the period July 1976 through April 1980.

A Global Thermospheric Density Model Based on Satellite Accelerometer Data

A Global Thermospheric Density Model Based on Satellite Accelerometer Data
Author: Frank A. Marcos
Publisher:
Total Pages: 48
Release: 1982
Genre: Accelerometers
ISBN:

Measurements from the accelerometer experiments on four low-altitude satellites (S3-1 and Atmosphere Explorer-C, -D, and -E) have been combined to produce an empirical model of the neutral mass density from 140 to 240 km. Data from over a 8000 orbits are analyzed using the least-squares method of multiple linear regression. The resulting model gives density as a function of solar flux (for flux values 60 to 130 units), geomagnetic activity, day of year, local time, latitude and altitude. It provides a more accurate fit to the measured data than other available atmospheric models. Three commonly used models are evaluated by comparison of their predicted density variations with those of this empirical model.

Ionospheric Space Weather

Ionospheric Space Weather
Author: Timothy Fuller-Rowell
Publisher: John Wiley & Sons
Total Pages: 311
Release: 2016-12-05
Genre: Science
ISBN: 1118929209

This monograph is the outcome of an American Geophysical Union Chapman Conference on longitude and hemispheric dependence of ionospheric space weather, including the impact of waves propagating from the lower atmosphere. The Chapman Conference was held in Africa as a means of focusing attention on an extensive geographic region where observations are critically needed to address some of the fundamental questions of the physical processes driving the ionosphere locally and globally. The compilation of papers from the conference describes the physics of this system and the mechanisms that control ionospheric space weather in a combination of tutorial-like and focused articles that will be of value to the upper atmosphere scientific community in general and to ongoing global magnetosphere-ionosphere-thermosphere (MIT) modeling efforts in particular. A number of articles from each science theme describe details of the physics behind each phenomenon that help to solve the complexity of the MIT system. Because this volume is an outcome of the research presented at this first space science Chapman Conference held in Africa, it has further provided an opportunity for African scientists to communicate their research results with the international community. In addition, the meeting and this conference volume will greatly enhance the space science education and research interest in the African continent and around the world. Ionospheric Space Weather includes articles from six science themes that were discussed at the Chapman Conference in 2012. These include: Hemispherical dependence of magnetospheric energy injection and the thermosphere-ionosphere response Longitude and hemispheric dependence of storm-enhanced densities (SED) Response of the thermosphere and ionosphere to variability in solar radiation Longitude spatial structure in total electron content and electrodynamics Temporal response to lower-atmosphere disturbances Ionospheric irregularities and scintillation Ionospheric Space Weather: Longitude Dependence and Lower Atmosphere Forcing will be useful to both active researchers and advanced graduate students in the field of physics, geophysics, and engineering, especially those who are keen to acquire a global understanding of ionospheric phenomena, including observational information from all longitude sectors across the globe.

Southern Hemisphere Seasonal Correlations (Classic Reprint)

Southern Hemisphere Seasonal Correlations (Classic Reprint)
Author: Robert Cockburn Mossman
Publisher: Forgotten Books
Total Pages: 42
Release: 2018-02-03
Genre: Science
ISBN: 9780267699315

Excerpt from Southern Hemisphere Seasonal Correlations The subject of synchronous compensation between the types of seasons at places situated in different parts of the Earth, and of the relation that exists between the sequence of weather at one place with the weather following at another place, even when the two localities are situated at a great distance from one another, is one that has of late years received increasing attention at the hands of meteorologists. Hildebrandsson, among a score of workers at this fascinating class of research, stands pre-eminent for his numerous contributions. In four papers on the Centres of Action of the Atmosphere, he has given a large number of examples of this species of weather correlation, most of which refer to places in the northern hemisphere, where we possess many of the long and homogeneous series of observations so necessary for this form of research. In his fourth and last memoir* Hildebrandsson has carried his investigations into the southern hemisphere, being hampered con siderably by the absence of data from regions where the southern centres of action are located. Having of late begun to collect data for South America with the object of preparing a general memoir on the climatology of that Continent, a considerable mass of material is already available for testing whether the South American weather sequences show as pronounced resemblances or contrasts when compared with data from other regions, as do those in the northern hemisphere. Cordoba in the Argentine Republic, it would appear, is the only station in South America with a long record situated in what may prove to be an action centre, most other places referring'to regions located in a transitional zone. While for the purposes of the present inquiry there is a lack of data from pronounced action centres, still many of the stations are so placed that they serve as an index of the pulsations taking place in the neighbouring foci of cyclonic and anti-cyclonic activity. As will be apparent later, some of the correlations obtained lend considerable support to the opinion expressed by other workers that the action centres of the globe are mutually associated, and that abnormal conditions in one hemisphere are inter-twined, not only with simul taneous but in many cases subsequent exceptional features in the other half of the earth. About the Publisher Forgotten Books publishes hundreds of thousands of rare and classic books. Find more at www.forgottenbooks.com This book is a reproduction of an important historical work. Forgotten Books uses state-of-the-art technology to digitally reconstruct the work, preserving the original format whilst repairing imperfections present in the aged copy. In rare cases, an imperfection in the original, such as a blemish or missing page, may be replicated in our edition. We do, however, repair the vast majority of imperfections successfully; any imperfections that remain are intentionally left to preserve the state of such historical works.