Cluster Post-Launch Support 2008-2010
Lead Research Organisation:
University College London
Department Name: Mullard Space Science Laboratory
Abstract
The Cluster Mission, for the first time, is exploring the magnetosphere with a fleet of four spacecraft orbiting in a group. The magnetosphere is the region of space around the Earth in which the Earth's magnetic field can be detected. It is the operating environment for many spacecraft that affect our quality of life, such as weather, television and communications satellites, as well as scientific spacecraft used to study the Earth, the Sun and solar system, and the cosmos. The magnetosphere is occasionally a dangerous environment for spacecraft, and understanding why this is so is one of the motivations for the Cluster project. The original 2 year mission was extended to allow Cluster to investigate a range of phenomena with different scale sizes, by varying the size of the Cluster tetrahedron from year to year. More recently, the Cluster Multi-Scale Mission has been under way, in which 3 of the spacecraft are separated by ~10,000 km. The distance between one of these and the fourth spacecraft has been varied from a tiny 40 km (in space plasma terms) up to 10,000 km. This work is laying the foundations for the proposed Cross-Scale mission (see www.cross-scale.org). Another exciting aspect of the Cluster Multi-scale Mission is that it will visit regions of the magnetosphere which were previously unexplored by Cluster, including the places where the solar wind first meets the magnetosphere, where aurorae are generated and where some magnetospheric substorms originate. In all of these places, Cluster's 4 well instrumented spacecraft, will provide new data to reveal the plasma physical processes at work, which in turn will help us understand how the magnetosphere works. A Plasma Electron And Current Experiment (PEACE) instrument can measure the three dimensional velocity distribution of electrons in a space plasma, for an energy range from a few electronvolts to about 30 kiloelectronvolts, every 4 seconds. A PEACE instrument is flying on each of the four Cluster II spacecraft, and consists of two sensor units and a data processing unit. All 8 sensors and 4 DPUs are still working well, after 8 years in space, despite regular passages through the earth's radiation belts. PEACE can tell us about the density and temperature of the electron plasma near the spacecraft, whether it is flowing and how fast, and whether electron beams from energetic sources elsewhere are passing the spacecraft, guided by the local magnetic field - giving PEACE a remote sensing capability. PEACE can tell us about the electrical currents being carried by the electrons, which is important as such currents transmit forces throughout the magnetosphere. The four PEACE instruments working together can tell us whether there are local flow shears (as in a river where the water flows faster nearer the middle) or even eddies and vortices in the electron plasma; whether there are waves in the plasma or on plasma boundaries, and can determine pressure gradients. This is a unique measurement capability for Cluster, as the counterpart plasma ion instruments do not work on all four spacecraft. It is providing glimpses of the way that explosive energy release processes such a magnetic reconnection work, which is very important as such processes are very active on the Sun and throughout the cosmos. Similarly, PEACE is helping to reveal how collisionless shocks work. Shocks are also phenomena that likely occur throughout the cosmos, and which are capable of energising electrons and ions to very large energies. This grant will allow us to continue operating the PEACE instruments until late 2009 and to do essential work on data handling, processing and curation, and maintaining up-to-date instrument calibrations. All this is needed to enable us to make scientifically useful data available to the research community. It will also help us to play our part in constructing and populating the Cluster Active Archive being created by the European Space Agency.
People |
ORCID iD |
Andrew Fazakerley (Principal Investigator) |
Publications
Alexandrova O
(2009)
Universality of solar-wind turbulent spectrum from MHD to electron scales.
in Physical review letters
Allen R
(2016)
A statistical study of EMIC waves observed by Cluster: 2. Associated plasma conditions
in Journal of Geophysical Research: Space Physics
Alm L
(2015)
Statistical altitude distribution of the auroral density cavity
in Journal of Geophysical Research: Space Physics
Alm L
(2014)
In situ observations of density cavities extending above the auroral acceleration region
in Journal of Geophysical Research: Space Physics
Alm L
(2013)
Pseudo altitude: A new perspective on the auroral density cavity
in Journal of Geophysical Research: Space Physics
Alm L
(2015)
Electron density and parallel electric field distribution of the auroral density cavity
in Journal of Geophysical Research: Space Physics
Amata E
(2011)
High kinetic energy density jets in the Earth's magnetosheath: A case study
in Planetary and Space Science
Andriopoulou M
(2015)
Deriving plasma densities in tenuous plasma regions, with the spacecraft potential under active control
in Journal of Geophysical Research: Space Physics
André M
(2012)
Low-energy ions: A previously hidden solar system particle population
in Geophysical Research Letters
Apatenkov S
(2009)
Radial propagation velocity of energetic particle injections according to measurements onboard the Cluster satellites
in Cosmic Research
Description | The scientific data from the PEACE instruments on the 4 co-orbiting Cluster spacecraft is used, together with data from other Cluster instruments, to investigate the Earth's magnetosphere and how it responds to the ever changing solar wind. Areas of progress include the nature of magnetic reconnection, the processes that produce the aurorae (northern lights), where and how solar wind material enters the magnetosphere, how plasma waves are generated within the magnetosphere and their roles in energising charged particles including those in the radiation belts. |
Exploitation Route | We continue to operate the PEACE instruments and the Cluster misison continues to explore new magnetospheric regions and make measurements on new scales, thus although the narrowly defined original mission objectives have been met, the mission continues to provide important new scientific measurements. The research community, including our own research group, continue to exploit the power of the Cluster dataset to shed new light on basic plasma physical processes, and on how the magnetosphere works. An improved understanding of the magnetosphere will be of interest to commercial and defence satellite operators, since this is the environment where their spacecraft operate, and "space weather" can at times adversely affect operations or even damage the spacecraft. |
Sectors | Aerospace Defence and Marine Other |
URL | http://www.ucl.ac.uk/mssl/space-plasma-physics/missions/cluster-peace/peace-publications |
Description | The Cluster PEACE scientific data that has been made available to the research community as a result of this funding has been used to produce more than 350 referreed scientific papers (as of summer 2014) as part of a total of 2060 referreed scientific papers from the Cluster mission as a whole. |
First Year Of Impact | 2001 |
Sector | Other |
Title | Cluster PEACE data in the Cluster Science Archive |
Description | Part of the funded work is the provision of the full set of data collected by the 4 Cluster PEACE instruments, after ground and in-flight calibrations have been applied, in scientific units, to the Cluster Science Archive. As the mission proceeds, more data is added. The data is publically available - to all researchers. |
Type Of Material | Database/Collection of data |
Year Produced | 2006 |
Provided To Others? | Yes |
Impact | The availability of the data from the Archive has enabled a high annual publication rate for the mission to be achieved and maintained, reflecting the strong interest of the research community in the Cluster mission. |
URL | http://www.cosmos.esa.int/web/csa/access |
Description | ESA Cluster Active Archive |
Organisation | European Space Agency |
Department | Science and Operations Department |
Country | France |
Sector | Academic/University |
PI Contribution | We provide multiple data products from our instruments to the ESA Cluster Active Archive, in a special format, with the best possible calibration knowledge based on detailed inflight calibration knowledge. The ESA funding contributes part of the salary of an additional (UK) person who is an integral part of our team, and not regarded as an external partner with limited data access etc. Thus the work of the ESA funded person benefits from the intellectual stimulation, training (UCL-based) and team support that we provide, and in return helps us meet the contract goals which might otherwise be impossible for the STFC funded team alone (who also do other tasks such as science planning and commanding of the instruments). |
Collaborator Contribution | ESA provides funding which helps us to employ an additional team member. ESA also provides the central archive and its web interface, and facilitates regular cross-calibration workshops that bring all the Cluster instrument teams together |
Impact | The outcome is that our entire dataset, with very high quality calibrations,together with that of all the other Cluster instruments, is gradually becoming available to the global science community. This is an unprecedented facility in space plasma physics. The main impact (we believe) is that the annual publication rate for Cluster remains high even though it has been in operation since 2001, and is likely to remain so for many years after the mission ends and the instrument teams disband. Thus we are working to ensure very high scientific return from our instruments now and in the future. |
Start Year | 2006 |