z-logo
Premium
Solar Rotation Period Driven Modulations of Plasmaspheric Density and Convective Electric Field in the Inner Magnetosphere
Author(s) -
Thaller S. A.,
Wygant J. R.,
Cattell C. A.,
Breneman A. W.,
Tyler E.,
Tian S.,
Engel A.,
De Pascuale S.,
Kurth W. S.,
Kletzing C. A.,
Tears J.,
Malaspina David M.
Publication year - 2019
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2018ja026365
Subject(s) - plasmasphere , magnetosphere , physics , electric field , rotation period , solar wind , extreme ultraviolet , solar maximum , atmospheric sciences , solar irradiance , plasma , solar cycle , astronomy , optics , stars , quantum mechanics , laser
This paper presents the first analysis of Van Allen Probes measurements of the cold plasma density and electric field in the inner magnetosphere to show that intervals of strong modulation at the solar rotation period occur in the locations of the outer plasmasphere and plasmapause (~0.7 R E peak‐to‐peak), in the large‐scale electric field (~0.24 mV/m peak‐to‐peak), and in the cold plasma density (~250 to ~70 cm −3 peak‐to‐peak). Solar rotation modulation of the inner magnetosphere is more apparent in the declining phase of the solar cycle than near solar maximum. The periodicities in these parameters are compared to solar extreme ultraviolet irradiance, solar wind dawn‐dusk electric field, and Kp . The variations in the plasmapause location at the solar rotation period anticorrelate with solar wind electric field, magnetospheric electric field, and Kp , but not with extreme ultraviolet irradiance, indicating that convective erosion is the dominant physical process controlling the plasmapause at these timescales.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here