OMNIDIRECTIONAL PLASMA SENSOR VDP
Welcome to VDP home page.
J. Safrankova, Z. Nemechek, M. Simerski, L. Prech
Faculty of Mathematics and Phisics of Charles University, Prague,
Czech Republic
G. Zastenker, A.Fedorov, O. Vaisberg, A.Leybov
Space Research Institute, Academy of Sciences of Russia, Moscow, Russia
Yu. Sharko, T. Romasenko
Design bureau AALAM, Bishkek, Kirgizstan
Description
The VDP instrument was designed for determination of integral flux vector
or integral energetic spectrum at the range 0.2 - 2.4 keV of ions or
electrons of magnetospheric plasma. The instrument includes 6 identical
Faraday caps, located by following ways:
Cap #1 is directed toward the Sun. It's main axis lies along axis of
spacecraft rotation (+X).
Cap #6 has antisunward direction (-X).
Caps #2 - #5 are directed along +Y, +Z, -Y, -Z axes respectively. These axes
rotate with spacecraft.
The figure shows cross-section of one Faraday cup.
Positive grid (C2) and negative grid (C3) is used to select ions or elecrons
measurement. In case of constant voltage, sensor supplies the total flux
of ions plus flux of electrons above 2400 eV energy, or total flux of
electrons plus flux of ions above 2400 eV energy. To get ion or electron
spectra the voltage of C2 or C3 is changed step by step over 16 steps in
range 0 - 2400 V. Cup #1 does not have negative grid and supplies
the ion flux plus electron flux with energy more then 170eV.
The maximum of data rate is 16 sample per second. In case of spectra
measuring one step is held during one second and full spectrum takes
16s.
The output range of direct current amplifier is -6.0 - + 6.0 V. The
flux can be calculated by :
P = 0.43E+9 1/cm*cm*s/V
The minimal digitased flux is 6.0E+5 1/cm*cm*s
and the maximum flux is
2.6E+9 1/cm*cm*s.
Operation and Measurements
VDP instrument works since August 14, 1995. Two Faraday caps #4 and #6
have problems and are not developed now.
Following pictures demonstrates instrument perfomance:
The example of magnetopause crossing on October 9.
Click picture to get big one.
Please, send your comments to
- Jana Safrankova (SAFRANK@CSPUNI12.BITNET)
- Georgy Zastenker (gzastenk@esoc1.iki.rssi.ru)
- Andrey Fedorov (af@afed.iki.rssi.ru)