PARAMETERIZED IONOSPHERIC MODEL - A GLOBAL IONOSPHERIC PARAMETERIZATION BASED ON FIRST PRINCIPLES MODELS

被引:213
作者
DANIELL, RE
BROWN, LD
ANDERSON, DN
FOX, MW
DOHERTY, PH
DECKER, DT
SOJKA, JJ
SCHUNK, RW
机构
[1] PHILLIPS LAB,GEOPHYS DIRECTORATE,BEDFORD,MA 01731
[2] BOSTON COLL,INST SPACE RES,CHESTNUT HILL,MA 02159
[3] BOSTON UNIV,CTR SPACE PHYS,BOSTON,MA 02215
[4] UTAH STATE UNIV,CTR ATMOSPHER & SPACE SCI,LOGAN,UT 84322
关键词
D O I
10.1029/95RS01826
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe a parameterized ionospheric model (PIM), a global model of theoretical ionospheric climatology based on diurnally reproducible runs of four physics based numerical models of the ionosphere. The four numerical models, taken together, cover the E and F layers for all latitudes, longitudes, and local times. PIM consists of a semianalytic representation of diurnally reproducible runs of these models for low, moderate, and high levels of both solar and geomagnetic activity and for June and December solstice and March equinox conditions. PIM produces output in several user selectable formats including global or regional latitude/longitude grids (in either geographic or geomagnetic coordinates), a set of user-specified points (which could lie along a satellite orbital path), or an altitude/azimuth/elevation grid for a user-specified location. The user selectable output variables include profile parameters (f(0)F(2), h(m)F(2), total electron content, etc.), electron density profiles, and ion composition (O+, NO+, and O-2(+)).
引用
收藏
页码:1499 / 1510
页数:12
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