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Author : Richard Frank Donnelly
Publisher : Unknown
Page : 448 pages
File Size : 45,8 Mb
Release : 1979
Category : Geophysics
ISBN : UOM:39015017172324
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 448 pages
File Size : 42,8 Mb
Release : 1979
Category : Cosmic physics
ISBN : STANFORD:36105133453709
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 752 pages
File Size : 51,9 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112101570262
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 528 pages
File Size : 41,6 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112005438368
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 744 pages
File Size : 43,8 Mb
Release : 1979
Category : Geophysics
ISBN : UOM:39015017172258
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 752 pages
File Size : 41,8 Mb
Release : 1979
Category : Cosmic physics
ISBN : MINN:30000010400806
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 528 pages
File Size : 48,8 Mb
Release : 1979
Category : Cosmic physics
ISBN : MINN:30000010400798
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 0 pages
File Size : 52,8 Mb
Release : 1979
Category : Cosmic physics
ISBN : LCCN:80016181
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 736 pages
File Size : 42,7 Mb
Release : 1979
Category : Cosmic physics
ISBN : MINN:30000010400780
Author : Richard Frank Donnelly
Publisher : Unknown
Page : 736 pages
File Size : 55,7 Mb
Release : 1979
Category : Ionospheric forecasting
ISBN : UIUC:30112005438350
Author : C.S. Deehr,J.A. Holtet
Publisher : Springer Science & Business Media
Page : 507 pages
File Size : 55,5 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400984172
This book is an ordered collection of tutorial lectures on the physical processes in the polar upper atmosphere given at the NATO Advanced Study Institute (ASI) on "The Exploration of the Polar Upper Atmosphere" held at Lillehammer, Norway, May 5-16, 1980. The polar cap is an important part of the high latitude atmosphere not only because of circulation and horizontal trans port in the neutral atmosphere and convection in the ionosphere, but also because of its unique energy sources and sinks. In addition, solar wind plasma is led into-the upper atmosphere by the geomagnetic field at the poles, and the polar cap is, as stated by Tutorial Leader Roederer in this volume, "the place where outer space meets earth". The atmosphere at lower latitudes is well-known to the ground-based observer, and the advent of satellite observations was simply the beginning of a new perspective. The exploration of the atmosphere at polar latitudes, however, proceeded in quite the opposite manner, and satellite maps of the polar caps may be compared with a relatively meagre set of ground-based data. Recent efforts to extend the polar observations from the ground have resulted in the need for a review of the physical principles and processes occurring in the polar upper atmosphere. The interdisciplinary nature of these efforts led to the emphasis here on a tutorial program.
Author : Anonim
Publisher : Unknown
Page : 564 pages
File Size : 51,7 Mb
Release : 1994
Category : Aeronautics
ISBN : UIUC:30112067190071
Author : William R. Barron
Publisher : Unknown
Page : 36 pages
File Size : 44,5 Mb
Release : 1982
Category : Protons
ISBN : UOM:39015095143056
Time-integrated solar ratio fluxes and their association with satellite observed solar energetic proton flux increases have been studied. The time-integration was only of the U-portion of the radio burst flux increase. The best correlations between the integrated radio fluxes and the proton peak fluxes were realized when the radio fluxes were multiplied by the factor exp (-3B), where B is the angular distance, in radians, between the site of the flare and the solar footpoint of the magnetic field connection between the sun and the earth. The solar footpoint positions were determined from the solar wind speed. Two-variate linear regressions were computed using the time-integrated radio fluxes at five discrete radio frequencies in the 606 to 8800 MHz frequency interval and peak proton fluxes at > 10 MeV and > 30 MeV. The higher frequencies of 2695, 4995 and 8800 MHz all correlated better with the > 10 -MeV protons than the lower frequencies. The > 30-MeV protons were even better correlated with the higher frequencies, but correlation with the lower frequencies were poorer. The Total Energy Density, E sub T, of the radio burst, an integration across the frequency interval of the time-integrated radio fluxes at each frequency, was found to be better correlated with the proton fluxes than any of the individual frequencies.
Author : United States. Air Force. Directorate of Chemical and Atmospheric Sciences
Publisher : Unknown
Page : 236 pages
File Size : 52,6 Mb
Release : 1981
Category : Atmospheric chemistry
ISBN : UOM:39015016077367
Author : Environmental Research Laboratories (U.S.)
Publisher : Unknown
Page : 234 pages
File Size : 41,6 Mb
Release : 1993
Category : Environmental policy
ISBN : UIUC:30112104152092