Sukcesem zakończyły się testy polskiej aparatury badawczej, zainstalowanej na pokładzie chińskich sond kosmicznych misji Chang’E-4. Instrumenty zaprojektowali i wykonali naukowcy z Centrum Badań Kosmicznych Polskiej Akademii Nauk (CBK PAN). W ciągu najbliższego miesiąca próbniki zostaną wystrzelone w stronę Księżyca.

Cassini is a joint mission of NASA and ESA established to study the Saturn System and its largest moon, Titan. The mission was launched on October 5, 1997 and arrived at Saturn on July 1, 2004. On January 14,

The RELEC satellite was launched on July 8, 2014 into the Sun’s synchronous orbit with apogee: 830km, perigee: 640km and inclination: 98,4deg. The aim of the RELEC mission is to study the precipitation of the magnetosphere’s relativistic electrons and

CHOMIK – powstał w Centrum Badań Kosmicznych PAN w Warszawie. Urządzenie to wzięło udział w rosyjskiej misji kosmicznej Fobos-Grunt. Do najważniejszych celów misji należało dostarczenie na Ziemię próbki materiału z powierzchni Fobosa, satelity Marsa. Materiał ten miał zostać pobrany

Spektrometr podczerwony SIR-2 jest jednym z trzech przyrządów naukowych dostarczonych przez ESA dla misji Chandrayaan-1 przygotowywanej przez Indyjską Agencję Badań Kosmicznych ISRO na Księżyc. Spektrometr został opracowany i wykonany w Max Planck Institute for Solar System Research w Katlenburg-Lindau

COMPASS-2 was the first micro-satellite of the Russian Space Agency’s low orbiting system. Its aim was to investigate the geodynamics-related effects in the ionospheric plasma. The project was coordinated by IZMIRAN RAS, and Polish CBK PAN in Warsaw was

Celem projektu jest realizacja polskiego udziału w międzynarodowym eksperymencie PFS (Planetary Fourier Spectrometer) dla misji Venus-Express przygotowywanej przez ESA. W CBK PAN prowadzone były następujące prace związane z PFS: konstrukcja modułu skanera – systemu do pozycjonowania przestrzennego osi optycznej

DEMETER (Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions) jest francuskim mikrosatelitą o niskiej orbicie (715 km), którego głównym zadaniem jest badanie sygnałów elektromagnetycznych pochodzących od zjawisk sejsmicznych i wulkanicznych. Misja wystartowała 29 czerwca 2004 z Bajkonuru na rosyjskiej

Cele misji Misja Rosetta ma na celu wyjaśnić zjawiska związane z powstaniem komet, związków zachodzących w materii międzygwiezdnej oraz ich wpływie na powstanie Układu Słonecznego. Będzie to możliwe m.in. dzięki następującym badaniom: ogólna charakterystyka jądra, określenie właściwości dynamicznych, zawartości

COMPAS was a small satellite created for investigation of ionospheric plasma effects related to geodynamics. Poland provided the plasma wave radiospectrometer. The spacecraft lost contact with its ground telemetric station after launch.

German/Indian DEOS (Dynamics of the Equatorial Ionosphere Over Shriharikota Range) Rocket Campaign was aimed at studying the structure and dynamics of the equatorial ionosphere under the equinox conditions. Three sounding rockets were launched in 1998 from SHAR (South India).

The MARS 96 mission was designed to send an orbiter, two small autonomous stations, and two surface penetrators to Mars in order to investigate the evolution of the planet by studying its physical and chemical processes. The Mars 96

The INTERBALL project was a new approach to the investigation of physical processes in the Earth’s magnetosphere and interplanetary medium with two satellites as well as two deployed sub-satellites delivered by the Czech Republic. The AURORAL PROBE (Interball-2) satellite

Projekt był częścią międzynarodowego eksperymentu ISTOK-1 należącego do satelitarnego projektu PRIRODA. Eksperyment polegał na badaniu atmosfery i powierzchni Ziemi przy pomocy aparatury spektrometrycznej wykonującej analizę widmową z pokładu stacji orbitalnej MIR. WIZJER jest uniwersalną kamerą telewizyjną, zamontowaną razem ze

Magion 4 was a subsatellite to INTERBALL 1 (Tail probe) and was launched together with it. The INTERBALL project’s main goal were the multi point simultaneous measurements at different altitudes in the Earth’s magnetosphere.On board of Magion 4 was

The INTERBALL project was a new approach to the investigation of the physical processes in the Earth’s magnetosphere and interplanetary medium by means of two satellites, as well as two deployed Czech sub-satellites. The TAIL PROBE (Interball-1) satellite along

The satellite CORONAS-I was launched on March 2, 1994. Its task was to study physical processes on the Sun and their influence on the Earth. Poland provided two instruments located on board the spacecraft. The first one, the X-ray

The payload-electric field detector was launched on June 6, 1992 on a Terrier-boosted Black Brant VC rocket (NASA 36.064 CE, El Coqui AA-3B) from the Puerto Rico’s North Coast. Peak altitude: 370km. Trajectory plane: within 10° of the magnetic

The Intercosmos-25 satellite with a Czech made sub-satellite was launched on the Earth’s orbit on December 18, 1991. Aboard the spacecraft were: an electron gun (6.2keV), a plasma gun (400eV), and a plasma diagnostics system. Another plasma diagnostics package

GAMMA mission launched on July 12, 1990, was a research in the field of high-energy (gamma/x-ray) astrophysics prepared jointly by Russia, France and Poland. The satellite was based on the Soyuz manned spacecraft. Poland provided the Telezvezda star tracker

The Intercosmos-24 satellite was launched on the Earth’s orbit on September 28, 1989. The IK-24 satellite consisted of the 10kW power transmitter at 9.6kHz, a full plasma diagnostics system located on the spacecraft as well as Czech made sub-satellite

The PHOBOS mission to Mars, consisting of 2 nearly identical spacecrafts Phobos-1 and Phobos-2, was launched on 7 and 12 July, 1988 respectively. The mission was performed as a cooperation between 14 nations including Sweden, Switzerland, Austria, France, West

COSMOS-1809 – was launched on December 18, 1986 to an almost circular orbit to investigate the physical processes in the Earth’s ionosphere. On board the satellite were instruments, among others the ionospheric topside sounder, designed and manufactured by several

As a part of Plasma experiment the MR-12 rocket was launched from the North Atlantic (18N 30W), on March 18, 1985. It was a mother-daughter type experiment. The impulse Li+ ion gun of 300A and 8.3eV was located on

Probe designed for investigations of the planet Venus and Halley’s Comet. VEGA-1 and VEGA-2 were launched on December 15, 1984 and December 21, 1984, respectively. The Vega spacecrafts were fitted with scientific apparatus and equipment built in eight countries

MR-12 rocket launched on May 20, 1983 to investigate the processes in the lower ionosphere. Poland provided the equipment measuring the low frequency spectra of plasma waves as well as electron density. The telemetric link with the scientific instruments

Rocket launched on December 21, 1981. Peak altitude: 1510km. Atmospheric and ionospheric studies, with devices from the Soviet Union and cooperating countries, were carried out. Poland provided the spectrum analyser to measure the ionospheric plasma irregularities.

The rocket experiment Gruzya-60 Spurt (G-60-S) was aimed at studying the processes in the vicinity of the vehicle caused by the injection of an electron beam. The payload was launched on September 18, 1981 with VERTICAL rocket going up

Spacecraft was launched on December 25, 1980 on Earth’s elongated orbit to investigate the interaction of solar wind with the magnetosphere. Measurements performed by scientific instruments obtained by international teams were related to the effects of solar activity on

Spacecraft launched on February 27, 1979 was designed to investigate the topside ionospheric structure and electromagnetic phenomena. The ionospheric topside sounder on board of the spacecraft was supported by a set of diagnostics plasma instruments provided by five countries.

INTERCOSMOS-15 tested new systems and satellite components in the spaceflight conditions. Poland provided the sub-carrier frequency generator for the unified telemetric system ETMS  located on IK-15’s board. Good performance of the device made it possible to use it also

INTERCOSMOS-COPERNICUS 500 spacecraft aimed at observations of solar radio bursts at r.f. frequencies and plasma resonances in the upper ionosphere. Poland provided the r.f. radiospectrometer. The spacecraft was launched on April 19, 1973 to commemorate the 500th anniversary of