THE TOROIDAL IMAGING MASS-ANGLE SPECTROGRAPH (TIMAS) FOR THE POLAR MISSION

被引:103
作者
SHELLEY, EG
GHIELMETTI, AG
BALSIGER, H
BLACK, RK
BOWLES, JA
BOWMAN, RP
BRATSCHI, O
BURCH, JL
CARLSON, CW
COKER, AJ
DRAKE, JF
FISCHER, J
GEISS, J
JOHNSTONE, A
KLOZA, DL
LENNARTSSON, OW
MAGONCELLI, AL
PASCHMANN, G
PETERSON, WK
ROSENBAUER, H
SANDERS, TC
STEINACHER, M
WALTON, DM
WHALEN, BA
YOUNG, DT
机构
[1] UNIV BERN, INST PHYS, CH-3012 BERN, SWITZERLAND
[2] SW RES INST, DEPT SPACE SCI, SAN ANTONIO, TX 78228 USA
[3] UNIV CALIF BERKELEY, SPACE SCI LAB, BERKELEY, CA 94720 USA
[4] UCL, MULLARD SPACE SCI LAB, DORKING RH5 6NT, SURREY, ENGLAND
[5] MAX PLANCK INST EXTRATERR PHYS, W-8046 GARCHING, GERMANY
[6] MAX PLANCK INST AERON, W-3411 KATLENBURG DUHM 3, GERMANY
[7] NATL RES COUNCIL CANADA, HERZBERG INST ASTROPHYS, OTTAWA, ON K1A 0R6, CANADA
关键词
D O I
10.1007/BF00751339
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The science objectives of the Toroidal Imaging Mass-Angle Spectrograph (TIMAS) are to investigate the transfer of solar wind energy and momentum to the magnetosphere, the interaction between the magnetosphere and the ionosphere, the transport processes that distribute plasma and energy throughout the magnetosphere, and the interactions that occur as plasmas of different origins and histories mix and interact. In order to meet these objectives the TIMAS instrument measures virtually the full three-dimensional velocity distribution functions of all major magnetospheric ion species with one-half spin period time resolution. The TIMAS is a first-order double focusing (angle and energy), imaging spectrograph that simultaneously measures all mass per charge components from 1 AMU e(-1) to greater than 32 AMU e(-1) over a nearly 360 degrees by 10 degrees instantaneous field-of-view. Mass per charge is dispersed radially on an annular microchannel plate detector and the azimuthal position on the detector is a map of the instantaneous 360 degrees field of view. With the rotation of the spacecraft, the TIMAS sweeps out very nearly a 4 pi solid angle image in a half spin period. The energy per charge range from 15 eV e(-1) to 32 keV e(-1) is covered in 28 non-contiguous steps spaced approximately logarithmically with adjacent steps separated by about 30%. Each energy step is sampled for approximately 20 ms; 14 step (odd or even) energy sweeps are completed 16 times per spin. In order to handle the large volume of data within the telemetry limitations the distributions are compressed to varying degrees in angle and energy, log-count compressed and then further compressed by a lossless technique. This data processing task is supported by two SA3300 microprocessors. The voltages (up to 5 kV) for the tandem toroidal electrostatic analyzers and preacceleration sections are supplied from fixed high voltage supplies using optically controlled series-shunt regulators.
引用
收藏
页码:497 / 530
页数:34
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