The AURORAL PROBE with its subsatellite was launched on 29 August 1996, also to the 65 degrees inclination orbit, but with the apogee of 20 000 km above the northern auroral zone and polar cap.
Two different auroral imagers are installed on the Auroral probe main satellite. These imagers are aimed to provide the two-dimensional global patterns of auroral phenomena and their time development. This allows to place in situ measurements from the two probes in the global geophysical perspective of large-scale magnetospheric processes.
Interball Auroral Probe : On-board Experiments
PLASMA
SKA-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
Yu.GALPERIN, R.KOVRAZHKIN, A.KUZMIN, F.SHUISKAYA IKI, Moscow, Russia
ION
Electron and ion spectra and anisotropy (M = 1, 2, 4, 16), 0.005 < E < 20 keV/Q
J.A.SAUVAUD CESR, Toulouse, France - R.A.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 - 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
J.J.BERTHELIER CETP Saint Maur, France - Yu.GALPERIN, T.MULIARCHIK IKI, Moscow, Russia
KM-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 FIELS
IMAP-3
Magnetic field (three components) Range 1 ÷ ± 70 000 nT, band 0-10 Hz
I.ARSHINKOV SDS, Sofia, Bulgaria - L.ZHUZGOV, V.STYAZHKIN IZMIRAN, Troitsk, Russia
IESP-2M
DC electric field and ULF waves (0.1-30 Hz)
S.PERRAUT CETP Velizy, France - M.MOGILEVSKY IKI, Moscow, Russia
POLRAD
Auroral Kilometric radiation (4 kHz - 2 MHz)
J. HANASZ, (Space Res. Centre PAS - Torun, Poland) - R. SCHREIBER (Copernicus Astr. Centre PAS - Torun, Poland) - H. DE FERAUDY (CETP/CNRS - Velizy, France)
MEMO
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
DOK-2
Energy spectra, angular distributions and time variations of electrons (E = 20-1000 keV)
K.KUDELA Inst. of Experim. Phys. SAS, Kosice, Slovakia - V.LUTSENKO IKI, Moscow, Russia - E.SARRIS University of Thrace, Xanthi, Greece
S/C POTENTIAL CONTROL
RON
Space electric potential control by two ion beams (N2+, In+). Ion beam currents Ibeam = 0-15 µA
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
UVAI
UV auroral imager (140 - 160 nm)
L.COGGER Univ. of Calgary, Canada - Yu.GALPERIN, M.VESELOV IKI, Moscow, Russia
UVSIPS
UV auroral oxygen emissions 130.4, 135.6, 149.3 nm in the footprint region of the Earth's atmosphere
A.KUZMIN IKI, Moscow, Russia - K.PALAZOV Observ. Yuri Gagarin, Stara Zagora, Bulgaria
TECHNOLOGICAL EXPERIMENTS
RD-1M
Dosimetric measurements
V.BENGIN, V.PETROV IMBP, Moscow, Russia - S.KUZNETSOV Moscow University, Moscow, Russia
ANOD
Comparison of different models of solar panels
A.KOZLOV State Scientific-industrial corporation QVANT, Moscow, Russia - T.MULIARCHIK IKI, Moscow, Russia
SERVICE SYSTEMS
BNK, BNTR, BNTS
Commutation blocks
J.DIKAREVA IKI, Moscow, Russia
SSNI
Telemetry system
L.CHESALIN IKI, Moscow, Russia
STO
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
BNS
Attitude processor
J.KLAS Inst. of Atm. Phys. CAS, Prague, Czech. Republic - N.EISMONT, Yu.LISSAKOV IKI, Moscow, Russia
Version:2.4.0
The AURORAL PROBE with its subsatellite was launched on 29 August 1996, also to the 65 degrees inclination orbit, but with the apogee of 20 000 km above the northern auroral zone and polar cap.
Two different auroral imagers are installed on the Auroral probe main satellite. These imagers are aimed to provide the two-dimensional global patterns of auroral phenomena and their time development. This allows to place in situ measurements from the two probes in the global geophysical perspective of large-scale magnetospheric processes.
Interball Auroral Probe : On-board Experiments
PLASMA
SKA-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
Yu.GALPERIN, R.KOVRAZHKIN, A.KUZMIN, F.SHUISKAYA IKI, Moscow, Russia
ION
Electron and ion spectra and anisotropy (M = 1, 2, 4, 16), 0.005 < E < 20 keV/Q
J.A.SAUVAUD CESR, Toulouse, France - R.A.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 - 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
J.J.BERTHELIER CETP Saint Maur, France - Yu.GALPERIN, T.MULIARCHIK IKI, Moscow, Russia
KM-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 FIELS
IMAP-3
Magnetic field (three components) Range 1 ÷ ± 70 000 nT, band 0-10 Hz
I.ARSHINKOV SDS, Sofia, Bulgaria - L.ZHUZGOV, V.STYAZHKIN IZMIRAN, Troitsk, Russia
IESP-2M
DC electric field and ULF waves (0.1-30 Hz)
S.PERRAUT CETP Velizy, France - M.MOGILEVSKY IKI, Moscow, Russia
POLRAD
Auroral Kilometric radiation (4 kHz - 2 MHz)
J. HANASZ, (Space Res. Centre PAS - Torun, Poland) - R. SCHREIBER (Copernicus Astr. Centre PAS - Torun, Poland) - H. DE FERAUDY (CETP/CNRS - Velizy, France)
MEMO
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
DOK-2
Energy spectra, angular distributions and time variations of electrons (E = 20-1000 keV)
K.KUDELA Inst. of Experim. Phys. SAS, Kosice, Slovakia - V.LUTSENKO IKI, Moscow, Russia - E.SARRIS University of Thrace, Xanthi, Greece
S/C POTENTIAL CONTROL
RON
Space electric potential control by two ion beams (N2+, In+). Ion beam currents Ibeam = 0-15 µA
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
UVAI
UV auroral imager (140 - 160 nm)
L.COGGER Univ. of Calgary, Canada - Yu.GALPERIN, M.VESELOV IKI, Moscow, Russia
UVSIPS
UV auroral oxygen emissions 130.4, 135.6, 149.3 nm in the footprint region of the Earth's atmosphere
A.KUZMIN IKI, Moscow, Russia - K.PALAZOV Observ. Yuri Gagarin, Stara Zagora, Bulgaria
TECHNOLOGICAL EXPERIMENTS
RD-1M
Dosimetric measurements
V.BENGIN, V.PETROV IMBP, Moscow, Russia - S.KUZNETSOV Moscow University, Moscow, Russia
ANOD
Comparison of different models of solar panels
A.KOZLOV State Scientific-industrial corporation QVANT, Moscow, Russia - T.MULIARCHIK IKI, Moscow, Russia
SERVICE SYSTEMS
BNK, BNTR, BNTS
Commutation blocks
J.DIKAREVA IKI, Moscow, Russia
SSNI
Telemetry system
L.CHESALIN IKI, Moscow, Russia
STO
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
BNS
Attitude processor
J.KLAS Inst. of Atm. Phys. CAS, Prague, Czech. Republic - N.EISMONT, Yu.LISSAKOV IKI, Moscow, Russia
Role | Person | StartDate | StopDate | Note | |
---|---|---|---|---|---|
1. | ProjectScientist | spase://CNES/Person/CDPP-Archive/Lev.Zelenyi |