Mostrando entradas con la etiqueta Centre National d'Études Spatiales (CNES). Mostrar todas las entradas
Mostrando entradas con la etiqueta Centre National d'Études Spatiales (CNES). Mostrar todas las entradas

domingo, 13 de noviembre de 2016

ESA : Flying the fantastic four .- Volando los cuatro fantásticos...............El vuelo de los Cuatro Fantásticos.......

http://www.esa.int/Our_Activities/Operations/Flying_the_fantastic_four
http://www.esa.int/Our_Activities/Navigation/Galileo/Launching_Galileo/Four_Galileo_satellites_on_one_Ariane_5

Separation will mark the start of a set of critical activities and manoeuvres to ensure the four Galileo sats are ready for handover by the 'CNESOC' team to the Galileo Control Centre the rest of their mission
Quad satellites see space
 
8 November 2016
This month, a single Ariane 5 rocket is set to propel four Galileo satellites into orbit for the navigation constellation’s first-ever quadruple launch. Mission controllers are training intensively for the complex space delivery.
On 17 November, an Ariane 5 will use a new payload dispenser to release four identical satellites into orbit in one go.
This will be the eighth Galileo launch, and will bring the number of satellites in space to 18. Once complete, the system will sport 24 operational satellites and a ground network to provide positioning, navigation and timing services.
To date, Soyuz rockets have carried two satellites at a time. This quadruple launch presents several technical challenges, including the new dispenser and the need to establish control over four independent satellites almost simultaneously.

Four times complex mission control

The ascent into the medium-altitude orbit will take three and a half hours. Then, after the satellites separate, a combined team from ESA and France’s CNES space agency will take over, establishing control and shepherding them through their early orbits, lasting nine days for one pair and 13 days for the other.
 
The joint ESA/CNES mission control team works, alternately, from here and from ESOC, in Darmstadt, Germany, to oversee the critical launch and early orbit phase flight control of Galileo satellites.
Galileo control room
 
“At the time that the four satellites separate two by two, we’ll have two shifts of the mission team working in the control room at the CNES centre in Toulouse, France, each shift managing two satellites – so it will be an intense period,” says Liviu Stefanov, co-flight director from ESA.
“This is the same team who conducted the previous Galileo early orbit phases, so we’re familiar with the satellites themselves,” says Hélène Cottet, lead flight director from CNES.
“What’s different this time is managing four satellites, sometimes in sequence and sometimes in parallel. We have concentrated a lot of effort on planning and training for the first few hours in space.”
Since 2011, the joint team have conducted the Galileo initial flight operations alternately from ESA’s centre in Darmstadt, Germany, and the CNES centre in Toulouse.

Target orbit: 23 200 km

Cutaway view shows the four Galileo satellites mounted on top of a specially adapted Ariane 5 rocket underneath the aerodynamic fairing.
Cut-away foursome
 
Separation will mark the start of a set of critical activities and manoeuvres to ensure the four are ready for handover to the Galileo Control Centre in Oberpfaffenhofen, Germany for the rest of their mission.
This includes ensuring that each have opened their solar wings and are ‘power positive’, establishing a data link via a set of ground stations, conducting extensive health checks and then switching the craft into a stable Earth-pointing mode, ready for subsequent manoeuvres.
Each must make three engine firings at roughly one-day intervals to get onto their ‘drift’ orbits, after which control will be passed from the joint team to the Galileo Control Centre.
“After a few days, we expect things to settle down, and we’ll be able to concentrate on manoeuvring two satellites while babysitting the other two,” says ESA’s Tom Cowell, one of four spacecraft operations managers.

The joint ESA/CNES ‘CNESOC’ mission control team seen at ESOC in 2015 just prior to Galileo 9/10 launch
Teamwork
 
“After handover of the first pair to Oberpfaffenhofen, we can manoeuvre the other two just as we’ve done for previous dual launches.”
Even after handover, specialists will continue determining the orbits and computing manoeuvres to position the satellites in their final orbits at around 23 200 km, expected early in 2017.

Training, simulating, preparing

Since summer, everyone involved in this Galileo launch has worked through multiple simulations, mostly focused on preparing for if things go wrong.
This week, the training will end with an intensive three-day live simulation in Toulouse.
After a network countdown practice on 14 November, the live network countdown for the actual launch will start a couple of hours after midnight on 17 November, with lift off from the European Spaceport in Kourou, French Guiana, set for the same day at 13:06 GMT (14:06 CET).
“It will be a challenge, but having already taken 14 Galileo satellites into orbit, our joint teams are confident of our abilities and skills,” says Hervé Côme, co-flight director from ESA.
“We know we can rely on teamwork and expertise, and we’re looking forward to a smooth lift off for Galileo’s first quad launch.”
 
VERSIÓN EN ESPAÑOL :

El vuelo de los Cuatro Fantásticos

Cutaway view shows the four Galileo satellites mounted on top of a specially adapted Ariane 5 rocket underneath the aerodynamic fairing.
Sección del cohete con los cuatro satélites
 
9 noviembre 2016
Este mes, cuatro satélites del sistema de navegación Galileo serán puestos en órbita a bordo de un cohete Ariane 5, en lo que constituirá el primer envío cuádruple de esta constelación. Los controladores de la misión están preparándose a fondo para este complejo lanzamiento al espacio. 
El 17 de noviembre, el Ariane 5 empleará un nuevo dispensador capaz de situar en órbita cuatro satélites idénticos de una sola vez.
Se trata del octavo lanzamiento de Galileo y, con él, serán 18 los satélites en el espacio. Una vez completado, el sistema contará con 24 satélites operativos y una red terrestre para la provisión de servicios de posicionamiento, navegación y determinación de la hora.
Hasta el momento, los satélites se enviaban de dos en dos a bordo de cohetes Soyuz. Este lanzamiento cuádruple presenta varios retos técnicos, incluyendo el nuevo dispensador de la carga útil y la necesidad de establecer el control sobre cuatro satélites independientes casi al mismo tiempo. 

Una sala de control cuatro veces más compleja

El ascenso hasta la órbita circular intermedia durará tres horas y media. A continuación, una vez separados los satélites, un equipo formado por personal de la ESA y de la agencia espacial francesa CNES asumirá su control y los guiará por sus órbitas tempranas. Esta fase se prolongará durante nueve días en el caso de la primera pareja de satélites, mientras que su duración para los otros dos será de 13 días. 
 
The joint ESA/CNES mission control team works, alternately, from here and from ESOC, in Darmstadt, Germany, to oversee the critical launch and early orbit phase flight control of Galileo satellites.
Sala de control de Galileo
 
“En el momento en que los cuatro satélites se separen por parejas, el equipo de la misión se dividirá en dos turnos para trabajar desde la sala de control del CNES en Toulouse, Francia. Cada uno de estos turnos se encargará de dos satélites, por lo que el trabajo será intenso”, explica Liviu Stefanov, codirector de vuelos de la ESA.
Como reconoce Hélène Cottet, directora principal de vuelos del CNES: “Se trata del mismo equipo que llevó a cabo las anteriores fases de órbita temprana de Galileo, por lo que conocemos bien los satélites”.
“La diferencia esta vez está en que hay que gestionar cuatro satélites, a veces en secuencia y a veces en paralelo. Así, hemos invertido mucho esfuerzo en planificación y entrenamiento de cara a las primeras horas en el espacio”.
Desde 2011, este equipo conjunto ha dirigido las operaciones de vuelo iniciales de Galileo alternando el trabajo desde el centro de la ESA en Darmstadt, Alemania, y el del CNES de Toulouse. 

Órbita objetivo: 23.200 km

Separation will mark the start of a set of critical activities and manoeuvres to ensure the four Galileo sats are ready for handover by the 'CNESOC' team to the Galileo Control Centre the rest of their mission
Llegada de los cuatro satélites al espacio
 
La separación marcará el comienzo de una serie de actividades y maniobras críticas para garantizar que los cuatro satélites estén listos para su traspaso al Centro de Control de Galileo en Oberpfaffenhofen, Alemania, por el resto de la misión.
Entre otras cuestiones, se comprobará que cada uno de ellos ha desplegado sus paneles solares y recibe energía; además, habrá que establecer un enlace de datos mediante una serie de estaciones terrestres, llevar a cabo amplias comprobaciones de funcionamiento y, a continuación, poner los módulos en un modo estable orientados hacia la Tierra, quedando así listos para posteriores maniobras.
 
ENGLISH VERSION:
 
Four Galileo satellites on one Ariane 5
 
Fairing lowered onto Galileo satellites
 
11 November 2016
Europe’s next four Galileo navigation satellites are together on their dispenser atop the Ariane 5 launcher due to launch them next Thursday from Europe’s Spaceport in French Guiana.
Having been attached to their dispenser as a combined ‘upper composite’, the four 715 kg satellites were transported to the final assembly building on 31 October.
The next step saw them put on top of the upper stage of their customised launcher. Finally, on 3 November, the quartet was enclosed within a protective fairing – the last time they were seen by human eyes – to protect them from the onrushing atmosphere during ascent.
In the following week, the rocket was prepared for takeoff, including filling its cryogenic upper stage, in preparation for the move to the launch pad on Tuesday, 15 November.
 
Galileos atop Ariane 5

In development since 2012, this new Ariane variant has evolved from the version used to place ESA’s 20 t Automated Transfer Vehicle vehicle into low orbit. The new launcher has to carry a lighter payload but needs to take it up to the much higher altitude of 22 900 km.
The target orbit is actually 300 km under the Galileo constellation’s final working altitude. This leaves Ariane’s upper stage in a stable ‘graveyard orbit’, while the four Galileos manoeuvre themselves up to their final set height.
The decision to proceed with this launch was taken after in-depth analysis of two recent anomalies occurring in rubidium atomic clocks aboard Galileo satellites in orbit.
 
Galileos meet Ariane 5

Highly accurate timing is core to satellite navigation. Each Galileo carries four atomic clocks to ensure quadruple redundancy of the timing subsystem: two Passive Hydrogen Maser clocks plus two Rubidium Atomic Frequency Standard (RAFS) clock.
Investigations jointly conducted by ESA and industry point to a short circuit in these two RAFS units. The ultimate objective of the fourfold redundancy on each satellite is to ensure operations over their planned lifetime.
Taking into account the redundancy and considering that the upcoming launch will increase the constellation’s overall robustness,it has been decided to maintain the mid-November launch date. 
 
Separation will mark the start of a set of critical activities and manoeuvres to ensure the four Galileo sats are ready for handover by the 'CNESOC' team to the Galileo Control Centre the rest of their mission
Quad satellites see space

Once this latest flight is complete, there will be 18 Galileo satellites in orbit – the single largest increase of any navigation satellite constellation from a single launch.
This will mark the first time that ESA deploys four satellites simultaneously. Usually, simply shepherding a spacecraft through the first critical days in orbit is a demanding enough task. A combined team from ESA and France’s CNES space agency based in Toulouse, France, will make contact, establish control and then see the quartet through its initial, critical, activities.
Two further Ariane 5 flights are planned for Galileo during the next two years, one each for the constellation’s remaining orbital planes.
Guillermo Gonzalo Sánchez Achutegui
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viernes, 14 de octubre de 2016

ESA : Sloshing fluids .- El salpicar de los fuidos

http://www.esa.int/spaceinimages/Images/2016/10/Sloshing_fluids

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  • Title Sloshing fluids
  • Released 11/10/2016 3:39 pm
  • Copyright CNES–E. Grimault, 2016
  • Description
    Have you ever tried walking while carrying a full cup of water? Your steps invariably cause the water to slosh about, making spills hard to avoid. Now imagine a satellite turning – the fuel inside will slosh, affecting the satellite’s stability.  
    France’s CNES space agency Fluidics experiment will run during ESA astronaut Thomas Pesquet’s Proxima mission on the International Space Station to probe how fluids behave in weightlessness. Co-funded by Airbus DS, the experiment will help to improve the performance of satellite propellant systems, extending their working lives by using every last drop in their tanks.
    A second part of Fluids will look at surface turbulence in liquids. On Earth, gravity and surface tension influence how energy dissipates in waves or ripples. In space, scientists can observe how surface forces behave without gravity – removing one factor simplifies our understanding.
    The experiment consists of three small transparent spheres in a centrifuge. One sphere holds water for the wave-turbulence research; the other two carry a special liquid with low viscosity and little surface tension for sloshing. 
  • Id 366727

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Guillermo Gonzalo Sánchez Achutegui
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sábado, 3 de mayo de 2014

NASA : NASA-CNES Move Forward with Global Water and Ocean Surface Mission


SWOT Agreement signed at NASA
NASA Administrator Charles Bolden, left, and Centre National d'Études Spatiales (CNES) President Jean-Yves Le Gall sign an agreement to move from feasibility studies to implementation of the Surface Water and Ocean Topography (SWOT) mission, Friday, May 2, 2014 at NASA Headquarters in Washington.
Image Credit:
NASA/Bill Ingalls
 
NASA and the French space agency Centre National d'Études Spatiales (CNES) have agreed to jointly build, launch, and operate a spacecraft to conduct the first-ever global survey of Earth's surface water and to map ocean surface height with unprecedented detail.
NASA Administrator Charles Bolden and CNES President Jean-Yves Le Gall signed an agreement Friday at NASA Headquarters in Washington to move from feasibility studies to implementation of the Surface Water and Ocean Topography (SWOT) mission. The two agencies began initial joint studies on the mission in 2009 and plan to complete preliminary design activities in 2016, with launch planned in 2020.
"With this mission, NASA builds on a legacy of Earth science research and our strong relationship with CNES to develop new ways to observe and understand our changing climate and water resources," said NASA Administrator Charles Bolden. "The knowledge we'll gain from SWOT will help decision makers better analyze, anticipate, and act to influence events that will affect us and future generations."
SWOT is one of the NASA missions recommended in the National Research Council's 2007 decadal survey of Earth science priorities. The satellite will survey 90 percent of the globe, studying Earth's lakes, rivers, reservoirs and ocean to aid in freshwater management around the world and improve ocean circulation models and weather and climate predictions.
This new agreement covers the entire life cycle of the mission, from spacecraft design and construction through launch, science operations, and eventual decommissioning. NASA will provide the SWOT payload module, the Ka-band Radar Interferometer (KaRIn) instrument, the Microwave Radiometer (MR) with its antenna, a laser retroreflector array, a GPS receiver payload, ground support, and launch services.
CNES will provide the SWOT spacecraft bus, the KaRIn instrument’s Radio Frequency Unit (RFU), the dual frequency Ku/C-band Nadir Altimeter, the Doppler Orbitography and Radiopositioning Integrated by Satellite (DORIS) receiver package, satellite command and control, and data processing infrastructure.
NASA and CNES began collaborating on missions to monitor ocean surface changes in the 1980s. From the TOPEX/Poseidon mission launched in 1992 to the Jason-1 mission launched in 2001 to the Jason-2/Ocean Surface Topography Mission launched in 2008, the collaboration has produced critical information on sea-level rise as well as El Niño causing world-wide impact.
The SWOT mission will use wide swath altimetry technology to produce high-resolution elevation measurements of the ocean surface and the surface of lakes, reservoirs, and wetlands. A more complete inventory of Earth's lakes and the changing amount of water they hold will yield improved assessments of how climate-induced changes can impact freshwater resources worldwide. Only 15 percent of lakes around the world are currently measured from space. SWOT will inventory a majority of medium to large lakes as well as the discharge volumes of rivers.
SWOT will be able to measure the ocean's surface with 10 times the resolution of current technologies. This will allow scientists to study small-scale features that are key components of how heat and carbon are exchanged between the ocean and atmosphere. The higher resolution of SWOT observations also will enable researchers to compute the velocity and energy of ocean circulation. A better understanding of small-scale ocean currents and eddies is also important to impacts on coastal regions such as navigation, erosion and dispersing pollutants.
For more information on the SWOT mission, visit:
NASA and its partners monitor Earth's vital signs from land, air and space with a fleet of satellites and ambitious airborne and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.
For more information about NASA's Earth science activities in 2014, visit:
 

What
is El Nino?
El Nino Globe
by David Herring
April 27, 1999
Fishermen who ply the waters of the Pacific off the coast of Peru and Ecuador have known for centuries about the El Niño. Every three to seven years during the months of December and January, fish in the coastal waters off of these countries virtually vanish, causing the fishing business to come to a standstill. South American fishermen have given this phenomenon the name El Niño, which is Spanish for "the Boy Child," because it comes about the time of the celebration of the birth of the Christ Child. During an El Niño, the physical relationships between wind, ocean currents, oceanic and atmospheric temperature, and biosphere break down into destructive patterns that are second only to the march of the seasons in their impacts to weather conditions around the world.

El Niño: A temperature anomalyThe vast tropical Pacific Ocean receives more sunlight than any other region on Earth. Much of this sunlight is stored in the ocean in the form of heat. Typically, the Pacific trade winds blow from east to west, dragging the warm surface waters westward, where they accumulate into a large, deep pool just east of Indonesia, and northeast of Australia. Meanwhile, the deeper, colder waters in the eastern Pacific are allowed to rise to the surface, creating an east-west temperature gradient along the equator known as the thermocline tilt.
The trade winds tend to lose strength with the onset of springtime in the northern hemisphere. Less water is pushed westward and, consequently, waters in the central and eastern Pacific begin to heat up (usually several degrees Fahrenheit) and the thermocline tilt diminishes. But the trade winds are usually replenished by the Asian summer monsoon, and the delicate balance of the thermocline tilt is again maintained.
Sometimes, and for reasons not fully understood, the trade winds do not replenish, or even reverse direction to blow from west to east. When this happens, the ocean responds in a several ways. Warm surface waters from the large, warm pool east of Indonesia begin to move eastward. Moreover, the natural spring warming in the central Pacific is allowed to continue and also spread eastward through the summer and fall. Beneath the surface, the thermocline along the equator flattens as the warm waters at the surface effectively act as a 300-foot-deep cap preventing the colder, deeper waters from upwelling. As a result, the large central and eastern Pacific regions warm up (over a period of about 6 months) into an El Niño. On average, these waters warm by 3° to 5°F, but in some places the waters can peak at more than 10°F higher than normal (up from temperatures in the low 70s Fahrenheit, to the high 80s).


Thermocline tilt January 1997Thermocline tilt April 1997Thermocline tilt July 1997
In the east, as temperatures increase, the water expands, causing sea levels to rise anywhere from inches to as much as a foot. But in the western Pacific, sea level drops as much of the warm surface water flows eastward. During the 1982-83 El Niño, this drop in sea level exposed and destroyed upper layers of coral reefs surrounding many western Pacific islands.
 
NASA
Guillermo Gonzalo Sánchez Achutegui

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