TY - JOUR
T1 - The dayside Venus ionosphere. I. Pioneer-Venus retarding potential analyzer experimental observations
AU - Miller, Kent L.
AU - Knudsen, William C.
AU - Spenner, Karl
N1 - Funding Information:
We thank Dr. Arvydas J. Kliore for supplying the radio occultation profiles required to make the median Ne,RO profile in Fig. 13. We also thank H. A. Taylor, Jr., and L. H. Brace for use of their UADS data in constructing the median N¢,Lp and 5~ni,eMs profiles in the same figure. We are grateful to Tom Canty for his assistance in organizing and plotting the data. Support for K. L. Miller and W. C. Knudsen was provided by NASA Contract NAS2-9481 and Lockheed Independent Research Funds.
PY - 1984/3
Y1 - 1984/3
N2 - The median values of the principal ionospheric quantities of the Venus dayside ionosphere are presented. The values are derived from the quantities measured by the Pioneer-Venus orbiter retarding potential analyzer over a period of two Earth yaers at solar cycle maximum. Quantities reported are total ion density, O+ density, O2+ density, sum density (NO+ + N2+ + CO+), CO2+ density, ion temperature, electron temperature, and plasma particle pressure. The data are organized to reveal altitude, solar zenith angle, solar longitude, and latitude dependences. The O+ density exhibits both a solar longitude and a latitude dependence which we suggest is caused by superrotation of the thermosphere and/or ionosphere. Asymmetry between the dawn and dusk terminator regions in the behavior of other quantities is also descibed.
AB - The median values of the principal ionospheric quantities of the Venus dayside ionosphere are presented. The values are derived from the quantities measured by the Pioneer-Venus orbiter retarding potential analyzer over a period of two Earth yaers at solar cycle maximum. Quantities reported are total ion density, O+ density, O2+ density, sum density (NO+ + N2+ + CO+), CO2+ density, ion temperature, electron temperature, and plasma particle pressure. The data are organized to reveal altitude, solar zenith angle, solar longitude, and latitude dependences. The O+ density exhibits both a solar longitude and a latitude dependence which we suggest is caused by superrotation of the thermosphere and/or ionosphere. Asymmetry between the dawn and dusk terminator regions in the behavior of other quantities is also descibed.
UR - http://www.scopus.com/inward/record.url?scp=20344397269&partnerID=8YFLogxK
U2 - 10.1016/0019-1035(84)90125-8
DO - 10.1016/0019-1035(84)90125-8
M3 - Article
AN - SCOPUS:20344397269
SN - 0019-1035
VL - 57
SP - 386
EP - 409
JO - Icarus
JF - Icarus
IS - 3
ER -