Mostrando entradas con la etiqueta Proba-1. Mostrar todas las entradas
Mostrando entradas con la etiqueta Proba-1. Mostrar todas las entradas

sábado, 29 de octubre de 2016

ESA : 15 years of Proba-1 .- Proba-1 view of Lena River Delta .- 15 años del Satélite Proba-1, vista del Río Lena

http://www.esa.int/spaceinimages/Images/2016/10/Proba-1_view_of_Lena_River_Delta

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  • Title Proba-1 view of Lena River Delta
  • Released 27/10/2016 9:52 am
  • Copyright ESA
  • Description
    An icy close-up view of part of Russia’s Lena River Delta acquired by ESA’s veteran Proba-1 microsatellite, celebrating 15 years in orbit.
    The Lena River is the 11th longest river in the world. It empties into the Laptev Sea through a 32 000 sq km delta, the largest such delta in the Arctic.
    Protected as a wilderness reserve and nominated as a UNESCO World Heritage Site, the Lena River Delta spends much of the year frozen, but blossoms into a verdant wetland during the brief polar summer.
    The cubic-metre Proba-1 is the first in ESA’s series of satellites aimed at flight-testing new space technologies. It was launched on 22 October 2001 but is still going strong, having since been reassigned to ESA’s Earth observation duties.
    Proba-1’s main hyperspectral CHRIS imager records 15 m-resolution scenes across a programmable selection of up to 62 spectral bands, from a variety of viewing angles. CHRIS is supplemented by a 5 m-resolution black-and-white microcamera.
    Other innovations included what were then novel gallium-arsenide solar cells, the use of startrackers for gyroless attitude control, one of the first lithium-ion batteries – now the longest such item operating in orbit – and one of ESA’s first ERC32 microprocessors to run Proba-1’s agile computer.
    For more background on Proba-1, read this celebration in the ESA Bulletin.
    Proba-1 led the way for the Sun-monitoring Proba-2 in 2009, the vegetation-tracking Proba-V in 2013 and the Proba-3 precise formation-flying mission planned for 2019.
  • Id 367734

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lunes, 13 de agosto de 2012

Olympic Games 2012: Proba-1 microsat snaps Olympic neighbourhood

Hi My Friends: A VUELO DE UN QUINDE EL BLOG., This Olympics has been watched from all over the world – and beyond. Benefiting from a cloudless sky, this view of London’s Olympic Park was captured by the smallest imager aboard ESA’s smallest mission: the High Resolution Camera on the Proba-1 microsatellite.
 Great Britain's gold medalists stand on the roof of Team GB House to celebrate on the last day of the Olympics. Photograph: Georgie Gillard/NOPP
 Proba-1 HRC image of London Olympic Park neighbourhood
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 The London Olympic Park including Olympic Stadium is visible towards the base of this Proba-1 High Resolution Camera image of East London, acquired on 11 August 2012. The 5-m resolution black and white image covers 25 sq km. 
Credits: ESA
 This Olympics has been watched from all over the world – and beyond. Benefiting from a cloudless sky, this view of London’s Olympic Park was captured by the smallest imager aboard ESA’s smallest mission: the High Resolution Camera on the Proba-1 microsatellite.

The Olympic Park, dominated by the circular Olympic Stadium, is visible towards the base of this 5 m-resolution image, with Victoria Park to its west and Hackney Marsh to the northwest.
This image was acquired by the High Resolution Camera (HRC). This black and white digital camera incorporates a Cassegrain telescope miniaturised to fit aboard Proba-1. Orbiting at 720 km altitude, the entire satellite’s volume is less than a cubic metre.
HRC operates alongside Proba-1’s larger CHRIS (Compact High Resolution Imaging Spectrometer) hyperspectral imager, which returns 15 m-resolution scenes across a programmable selection of up to 62 spectral bands, from a variety of viewing angles. This HRC image was acquired on 11 August. 

 Marking 10 years in orbit in October 2011, Proba-1, ESA's first Project for On Board Autonomy micro-satellite, demonstrates the potential and feasibility of small satellites for advanced scientific and Earth observation missions 
Credits: ESA

 About Proba-1

Operational for more than a decade, Proba-1 was the first in ESA’s series of satellites aimed at providing in-orbit testing of new space technologies. Smaller than a cubic metre, Proba-1’s many experiments include the compact HRC, acquiring monochromatic images with an area of 25 sq km.
Proba stands for ‘Project for Onboard Autonomy’ – both cameras are largely autonomous. Controllers at ESA’s Redu station in Belgium send up the location to be imaged – latitude, longitude and altitude – then the satellite itself does the rest, lining up its instruments with its target on the ground.
 

Proba-1 was launched back in October 2001 as an experimental mission but is still going strong, having since been reassigned to ESA’s Earth observation team. This year a software fix returned its radiation-damaged star trackers to full operations.
In November 2009 Proba-1 was joined in orbit by Proba-2, focused on solar monitoring. Proba-V, to monitor global vegetation, is due to launch next year.
 ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
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ayabaca@yahoo.com
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martes, 5 de junio de 2012

Astronoomía: Las misiones de la ESA se preparan para observar el tránsito de Venus

Hola Amigos: A VUELO DE UN QUINDE EL BLOG., Los satélites de la ESA Venus Express y Proba-2, y las misiones internacionales SOHO, Hinode y Hubble se preparan para observar tanto a Venus como al Sol durante el tránsito del planeta hermano de la Tierra en la noche del 5 al 6 de junio.
Actualmente, Venus Express es el único satélite en órbita a Venus. Esta misión europea utilizará la luz del Sol para estudiar la atmósfera del planeta, mientras los científicos estudian el tránsito desde la Tierra.
La luz del Sol, al filtrarse a través de la atmósfera del planeta, permite estudiar cómo varía la concentración de distintas especies químicas con la altura sobre la superficie de Venus.
Esta técnica también se utiliza para estudiar las atmósferas de los planetas que se encuentran fuera de nuestro Sistema Solar – también conocidos como ‘exoplanetas’ – y permite determinar si reúnen las condiciones necesarias para albergar vida.
Durante este tránsito, el último del siglo, se compararán los resultados de Venus Express con los datos recogidos de forma simultánea en observatorios de todo el mundo. 

 The path that Venus will take as it approaches the Sun in SOHO’s field of view. The image is from the transit of Venus in 2004, but a similar path will be taken during the transit of 2012. 
Credits: SOHO/ESA/NASA

Los científicos dedicados al estudio de los exoplanetas podrán así poner a prueba las técnicas que utilizan para determinar las características de los planetas rocosos de tamaño similar al de la Tierra.
Como Venus Express se encuentra en órbita al planeta, no notará nada inusual durante el tránsito. Para él, el Sol simplemente se pondrá a través de la atmósfera de Venus. Sin embargo, los datos que recoja durante esta puesta de sol serán de gran utilidad al compararlos con los obtenidos de forma simultánea desde la Tierra.
El microsatélite Proba-2 de la ESA y el satélite japonés para el estudio del Sol, Hinode, contarán con asientos de primera fila para el evento, observando desde la órbita terrestre cómo Venus pasa por delante del disco solar.
“Proba-2 detectará un descenso en la intensidad de la radiación solar tan pronto como la atmósfera de Venus comience a cruzar la silueta del Sol. Este fenómeno es muy importante para el estudio de los exoplanetas”, explica Joe Zender, responsable de la misión Proba-2 para la ESA.
Si Venus pasase exactamente por delante de una región activa del Sol, sería posible obtener información sobre la energía emitida por esta región en concreto.
“Estos resultados serían muy importantes para el estudio de la meteorología espacial, del Sol y de su influencia sobre la Tierra”.
Hinode observará el tránsito en las bandas del visible, rayos X y ultravioleta, estudiando fenómenos como el ‘efecto de la gota negra’ – tanto al comienzo como al fin del tránsito, la silueta de Venus parece estar conectada con el limbo del Sol, deformándose hasta tomar la apariencia de una gota de agua.
Esta misión también estudiará la aureola, un arco de luz que se puede observar alrededor del disco planetario durante los primeros y los últimos minutos del tránsito.
“Las imágenes más espectaculares serán las tomadas por el Telescopio Óptico de Hinode, actualmente el instrumento para el estudio del Sol con mayor resolución de todos los que se encuentran en órbita”, comenta Bernhard Fleck, científico de los proyectos Hinode y SOHO para la ESA.
“Desafortunadamente, SOHO no se encontrará en una buena posición para observar el tránsito. Sin embargo, este satélite será capaz de seguir a Venus a medida que se acerca al Sol, días antes del tránsito, y cuando se aleje después de éste, algo fuera del alcance de los otros satélites.”
Mientras tanto, el Telescopio Espacial NASA/ESA Hubble utilizará la Luna como un espejo gigante para estudiar el reflejo difuso de la luz solar: una pequeña fracción de esa luz habrá pasado a través de la atmósfera de Venus de camino a la Luna.
Esta campaña de observaciones permitirá probar nuevas técnicas diseñadas para caracterizar las atmósferas de exoplanetas rocosos de tamaño similar al de la Tierra, que podrían albergar vida fuera de nuestro Sistema Solar.
 Para más información
 Guillermo Gonzalo Sánchez Achutegui
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martes, 25 de octubre de 2011

The Earth: Small but agile Proba-1 reaches 10 years in orbit

Hi My Friends: A VUELO DE UN QUINDE EL BLOG., A good photographer needs agility. So it is with ESA microsatellite Proba-1, which turns in space to capture terrestrial targets. Celebrating its tenth birthday this week, Proba-1’s unique images are used by hundreds of scientific teams worldwide.

For most Earth-observing satellites, image acquisition is only a matter of opening a viewing aperture but Proba-1 is different. The satellite’s platform and payload work as one: spinning reaction wheels guided by a startracker roll it up to 25º side to side and 55º along its path. This helps Proba-1 compensate for its 7.5 km/s speed, like a photographer panning to snap a moving target. In addition, Proba-1 can record up to five differently angled views of the same target, important for researchers investigating how vegetation changes appearance with shifts in view. Understanding 'Bi-Reflectance Distribution Function' has proved beneficial for mapping and classifying land cover, from forest monitoring in Canada to crop yield predictions in Europe, Australia and China.

Credits: ESA.

A good photographer needs agility. So it is with ESA microsatellite Proba-1, which turns in space to capture terrestrial targets. Celebrating its tenth birthday this week, Proba-1’s unique images are used by hundreds of scientific teams worldwide.

A technology demonstrator turned into an Earth observation mission, the microsatellite – just a cubic metre in volume – has acquired nearly 20 000 environmental science images with its main Compact High Resolution Imaging Spectrometer (CHRIS), used by a total of 446 research groups in 60 countries.




CHRIS is used to measure directional spectral reflectance of land areas, thus providing new biophysical and biochemical data, and information on land surfaces.

Credits: SIRA.

ESA has a family of experimental ‘Project for Onboard Autonomy’ microsatellites: the Sun-watching Proba-2 went into orbit in 2009 and the vegetation-imaging Proba-V will be launched next year.
But it was Proba-1, launched from India on 22 October 2001, that started it all


CHRIS's multi-angled view of Golden Gate Bridge in San Francisco, USA. For most Earth-observing satellites, image acquisition is only a matter of opening a viewing aperture but Proba-1 is different. The satellite’s platform and payload work as one: spinning reaction wheels guided by a startracker roll it up to 25º side to side and 55º along its path. This helps Proba-1 compensate for its 7.5 km/s speed, like a photographer panning to snap a moving target. In addition, Proba-1 can record up to five differently angled views of the same target, important for researchers investigating how vegetation changes appearance with shifts in view. Understanding this has proved beneficial for mapping and classifying land cover, from forest monitoring in Canada to crop yield predictions in Europe, Australia and China.

Credits: ESA

“Proba-1 remains the most agile and stable satellite platform in its range,” explains Frank Preud’homme of QinetiQ Space Belgium, the company that built Proba-1 for ESA.
“These attributes are a prerequisite for high performance remote sensing.”
For most Earth-observing satellites, image acquisition is only a matter of opening a viewing aperture but Proba-1 is different.

Proba-1 CHRIS image of Mount Kilimanjaro in Tanzania, the highest peak in Africa, acquired on 27 April 2011

Credits: ESA

The satellite’s platform and payload work as one: spinning reaction wheels guided by a startracker roll it up to 25º side to side and 55º along its path.
This helps Proba-1 compensate for its 7.5 km/s speed, like a photographer panning to snap a moving target.

This Proba image shows numerous small lakes in the otherwise arid environment of the Gobi Desert in the Chinese Autonomous Region of Inner Mongolia, surrounded by some of the highest and largest sand dunes in the world. This image was acquired on 29 September 2005 by the Compact High Resolution Imaging Spectrometer (CHRIS).

Credits: ESA
In addition, Proba-1 can record up to five differently angled views of the same target, important for researchers investigating how vegetation changes appearance with shifts in view.
“Look at a sunflower on the ground – you’ll see a different mix of colours depending on where you stand, as well as the growing season and time of day,” explains Mike Cutter of Surrey Satellite Technology Ltd, which designed CHRIS. “The same is true in orbit.”

Proba-1 CHRIS image of the southern tip of Portsmouth Harbour, the Isle of Wight and the heavily-trafficked waters of the Solent in between, acquired 26 November 2010

Credits: ESA

Understanding this has proved beneficial for mapping and classifying land cover, from forest monitoring in Canada to crop yield predictions in Europe, Australia and China.
Other researchers favour the fact that CHRIS’s spectral response can be programmed as desired, to home in on diverse factors such as inland or coastal water quality –identifying oil spills, for example – atmospheric pollution or even desert lichens – significant for conserving topsoil in marginal environments.


A cloudy day on North Sentinel Island in the Indian Ocean as seen from ESA's Proba satellite on 23 April 2005.

Credits: ESA, Sira Technology Ltd

CHRIS’s 17 m resolution is useful in its own right, adds Mr Cutter: “It can give extra detail of a local section of a larger satellite image acquired at lower resolution.”
For instance, more than 500 CHRIS images have been delivered for the International Charter ‘Space and Major Disasters’, a space agency agreement to prioritise damage mapping of disaster-struck regions.

Proba's CHRIS image of the French town of Arles, acquired on 7 December 2003 during flooding that swamped the northern part of the settlement under one metre of water. The image was acquired following activation of the Charter on Space and Major Disasters.

Credits: ESA

“This mission came down to an experiment – Proba’s name derived is from the Latin word Probare: ‘let’s try’,” comments Frederic Teston, head of ESA’s In-Orbit Demonstration Programme, giving Europe’s space industry the opportunity to flight-test new technologies.
“We were demonstrating as many new technologies as possible on a single platform, the resulting satellite being able

This black and white image shows Uluru, also known as Ayers Rock, in Australia. It was acquired 24 April 2004 by the High-Resolution Camera (HRC) aboard Proba. Uluru is the world's largest monolith, and a sacred site to Australia's Aborigines. It is 3.6 km long and two km wide. The walk around it covers 9.4 km.

Credits: ESA

CHRIS users simply submit the latitude, longitude and altitude of their chosen target and Proba-1’s computer navigates to the correct location, tilts, shoots and delivers the scene.
Other innovations included then-novel gallium arsenide solar cells and one of the first laptop-style lithium ion batteries – now the longest operating example in Earth orbit.

Proba-1, Project for On Board Autonomy, demonstrates the potential and feasibility of small satellites for advanced scientific and Earth Observation missions.

Credits: ESA
CHRIS is only the largest of Proba-1’s payloads. A smaller imager, the High Resolution Camera developed by Belgian company OIP Sensor Systems, provides black-and-white 5–10 m-resolution images.
The microsatellite is overseen from ESA’s Redu ground station in Belgium and the use of Proba-1's instruments is managed from ESA's ESRIN Earth observation centre in Italy.
Guillermo Gonzalo Sánchez Achutegui



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