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Below is a table of INTERBALL-2 experiments summary to remind you about specific features of each instrument. Click on the name of an appropriate instrument to see some samples of data processing.
See bottom of the page for additional information.
Experiment | Measured Parameters | PI And Key Scientists |
---|---|---|
AURORAL PLASMA | ||
S K A - 3![]() |
Spectra of electrons and ions 0.03 < E < 15 keV; anisotropy of electrons and ions (M = 1, 4, 16), 30 < E < 500 keV/Q | F. Shuiskaya
A. Kuzmin Yu. Galperin R. Kovrazhkin V. Stepanov IKI, Moscow, Russia |
I O N | Electron and ion spectra and anisotropy (M = 1, 2, 4, 16), 0.005 < E < 20 keV/Q | J. A.
Sauvaud
CESR, Toulouse, France R. Kovrazhkin K. Afanasiev IKI, Moscow, Russia |
PROMICS-3 | Ion composition (M = 1-32) and 3-D energy distribution, 10 eV < E < 30 keV/Q | I. Sandahl
IRF, Kiruna, Sweden E. Budnik N. Pissarenko E. Dubinin IKI, Moscow, Russia H. Koskinen T. Pulkkinen FMI, Helsinki, Finland |
THERMAL PLASMA | ||
HYPERBOLOID | Ion composition and 3-D distribution functions, M = 1-32 (with H+, He+, O++, O+ routinely), 0.1 < E < 80 eV | N. Dubouloz
J. -J. Berthelier CETP, Saint-Maur, France Yu. Galperin T. Muliarchik D. Chugunin IKI, Moscow, Russia |
K M - 7 | Temperature of cold electrons, T < 10 eV | J. Smilauer
Inst. of Atm. Physics CAS, Prague, Czech. Republic V. Afonin IKI, Moscow, Russia |
ALPHA-3![]() |
Thermal plasma ion flux, E < 25 eV/Q | V. Bezrukikh
IKI, Moscow, Russia |
WAVES AND FIELDS | ||
I M A P - 3![]() |
Magnetic field (three components). Range 1-±70000 nT, band 0-10 Hz. | I. Arshinkov
SDS, Sofia, Bulgaria L. Zhuzgov V. Styazhkin IZMIRAN, Troitsk, Russia |
I E S P - 2M | DC electric field and ULF waves (0.1-30 Hz) | S. Perraut
CETP, Saint-Maur, France M. Mogilevsky IKI, Moscow, Russia |
POLRAD | Auroral kilometric radiation (20 kHz - 2 MHz) | J. Hanasz
Space Research Centre PAS, Torun, Poland M. Mogilevsky T. Romantsova IKI, Moscow, Russia |
M E M O | Electromagnetic waves in wide band (quantitative analysis) < 240 kHz | F. Lefeuvre
LPCE, Orleans, France M. Mogilevsky IKI, Moscow, Russia |
NVK-ONCH | VLF electromagnetic waves 20 Hz - 20 kHz | A. Goljavin
IZMIRAN, Troitsk, Russia M. Mogilevsky IKI, Moscow, Russia |
ENERGETIC PARTICLES | ||
D O K - 2 | Energy spectra, angular distributions and time variations of electrons (E = 15-400 keV) andions (E = 20-1000 keV) | K. Kudela
Inst. of Experim. Physics SAS, Kosice, Slovakia V. Lutsenko IKI, Moscow, Russia E. Sarris University of Thrace, Xanthi, Greece |
S/C POTENTIAL CONTROL | ||
R O N | Space electric potential control by two ion beams (N2+, In+). Ion beam currents Ibeam=0-15mkA. | W. Riedler
K. Torkar Space Res. Inst., Austrian Acad. Sci., Graz, Austria R. Schmidt ESA/ESTEC, Nordwijk, The Netherlands Yu. Galperin M. Veselov IKI, Moscow, Russia |
OPTICAL OBSERVATIONS | ||
U V A I | UV auroral imager (140 - 160 nm) | L. Cogger
Univ. of Calgary, Canada Yu. Galperin M. Veselov IKI, Moscow, Russia |
UFSIPS![]() |
UV auroral oxygen emissions 130.4, 135.6, 149.3 nm in the footprint regionof the Earth's atmosphere | A. Kuzmin
IKI, Moscow, Russia K. Palazov Observ. Yuri Gagarin, Stara Zagora, Bulgaria |
TECHNOLOGICAL EXPERIMENTS | ||
R D - 1M | Dosimetric measurements | V. Bengin
V. Petrov IMBP, Moscow, Russia S. Kuznetsov Moscow University, Moscow, Russia |
A N O D | Comparison of different models of solar panels | A. Kozlov
State Scientific-industrial corporation QUANT, Moscow, Russia T. Muliarchik IKI, Moscow, Russia |
SERVICE SYSTEMS | ||
BNK, BNTR,
BNTS |
Communication blocks | J. Dikareva
IKI, Moscow, Russia |
S S N I | Telemetry system | L. Chesalin
IKI, Moscow, Russia |
S T O | Telemetry system | L. Bodnar
Politechn. Inst. Budapest, Hungary J. Vojta Inst. of Atm. Phys. CAS, Prague, Czech. Republik S. Roishik Aviation Inst., Warsaw, Poland G. Terekhin IKI, Moscow, Russia |
B N S | Attitude processor | J. Klas
Inst. of Atm. Phys. CAS, Prague, Czech. Republik N. Eismont Yu. Lisakov IKI, Moscow, Russia |
This page is designed at Space Plasma Physics Department, IKI . Please send your comments and suggestions about this page and subsequent pages to Vladimir Stepanov (see SKA-3 experiment also), or contact appropriate instrument group directly.
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