Mostrando entradas con la etiqueta Russia. Mostrar todas las entradas
Mostrando entradas con la etiqueta Russia. Mostrar todas las entradas

domingo, 12 de marzo de 2017

ESA : Kamchatka, Russia .- Kamchatka, Rusia

http://www.esa.int/spaceinimages/Images/2017/03/Kamchatka_Russia

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  • Title Kamchatka, Russia
  • Released 10/03/2017 10:00 am
  • Copyright contains modified Copernicus Sentinel data (2017), processed by ESA
  • Description
    The Sentinel-3A satellite takes us over the Sea of Okhotsk in the Russian Far East on 15 February, where clouds blend with the ice and snow beneath from our bird’s-eye view.
    One of the fascinating features is the pattern of floating sea ice, appearing light blue. Along the left we can see cracks in the ice covering the water. In the middle/right, small pieces of fragmented ice driven by wind and currents create the swirls of blue along the coast of the Kamchatka Peninsula.
    Located in the Russian Far East, this peninsula has a landscape covered with volcanoes due to its location along the highly active Pacific ‘Ring of Fire’. There are about 160 volcanoes on the peninsula, 29 of which are still active.
    We can see part of the central mountain range running down the spine of the peninsula, while the eastern range is mostly covered by clouds. Between them lies the central valley, appearing somewhat brown from the lack of snow cover.
    It is no surprise that the area is often referred to as the ‘land of fire and ice’.
    Owing to minimal development, the peninsula is known for its abundance of large brown bears. Other common animals include foxes, wolves, reindeer and wolverines.
    Sentinel-3 is a two-satellite mission for Europe’s Copernicus programme. While Sentinel-3A has been in orbit since February 2016, the second is set for launch later this year.
    This image is featured on the Earth from Space video programme.
  • Id 374357

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Guillermo Gonzalo Sánchez Achutegui
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domingo, 30 de octubre de 2016

ESA : Putorana Plateau, Siberia .-

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

Putorana Plateau, Siberia

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  • Title Putorana Plateau, Siberia
  • Released 28/10/2016 10:00 am
  • Copyright Contains modified Copernicus Sentinel data (2016), processed by ESA
  • Description
    Sentinel-2A brings us over the snowy landscape of the Putorana Plateau in northern Central Siberia.
    The area pictured shows part of the Putoransky State Nature Reserve, which is listed as a UNESCO World Heritage Site. Situated about 100 km north of the Arctic Circle, the site serves as a major reindeer migration route – an increasingly rare natural phenomenon – and is one of the very few centres of plant species richness in the Arctic.
    Virtually untouched by human influence, this isolated mountain range includes pristine forests and cold-water lake and river systems. The lakes are characterised by elongated, fjord-like shapes, such as Lake Ayan in the upper-central part of the image. 
    Zooming in on the lake we can see that it is mostly ice-covered, with small patches of water peeking through around its lower reaches.
    Another feature of this area are the flat-topped mountains, formed by a geological process called ‘plume volcanism’: a large body of magma seeped through Earth’s surface and formed a blanket of basalt kilometres thick. Over time, cracks in the rock filled with water and eroded into the rivers and lakes we see today.
    This image, also featured on the Earth from Space video programme, was captured on 2 March 2016 by the Copernicus Sentinel-2A satellite.
  • Id 367705

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martes, 3 de febrero de 2015

NASA : Cloud Streets in the Bering Sea .- Calles de la nube en el mar de Bering

Hola amigos. A VUELO DE UN QUINDE EL BLOG., . hemos recibido de la Fundación Nacional de Ciencias de Los Estados Unidos, sobre una espectacular fotografía del Mar de Bering, que precisamente la toma da una idea como si fuesen calles de hielo, captada por  NASA's Aqua satellite: Aguas de hielo, viento, temperaturas frías y mar se combinaron para creadas formaciones de nubes dramáticas sobre el mar de Bering a finales de enero de 2015....
La tundra congelada de Rusia se encuentra en el noroeste de la imagen, y Alaska nevado se encuentra en el noreste. El hielo marino se extiende desde la tierra hasta bien entrado el Mar de Bering. Durante la brillante línea de nubes blancas agua oscura en de cerca, filas paralelas. Estas formaciones son conocidas como "calles de nubes".

Más información. lea usted abajo....

Cloud Streets in the Bering Sea
Ice, wind, cold temperatures and ocean waters combined to created dramatic cloud formations over the Bering Sea in late January, 2015. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA's Aqua satellite passed over the region and captured this true-color image on Jan. 23.
The frozen tundra of Russia lies in the northwest of the image, and snow-covered Alaska lies in the northeast. Sea ice extends from the land well into the Bering Sea. Over the dark water bright white clouds line in up close, parallel rows. These formations are known as “cloud streets”.
Air blowing over the cold, snowy land and then over ice becomes both cold and dry. When the air then moves over relatively warmer and much moister water and lead to the development of parallel cylinders of spinning air. On the upper edge of these cylinders of air, where the air is rising, small clouds form. Where air is descending, the skies are clear. This clear/cloudy pattern, formed in parallel rows, gives the impression of streets.
The clouds begin over the sea ice, but they primarily hang over open ocean. The streets are neat and in tight rows closest to land, while further over the Bering Sea the pattern widens and begins to become more random. The rows of clouds are also not perfectly straight, but tend to curve. The strength and direction of the wind helps create these features: where the wind is strongest, nearest to shore, the clouds line up most neatly. The clouds align with the wind direction, so the direction of the streets gives strong clues to prevailing wind direction.
Image Credit: NASA/Jeff Schmaltz, MODIS Land Rapid Response Team, NASA GSFC
NASA
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viernes, 7 de febrero de 2014

NASA : Sochi, Russia Winter Olympic Sites (Mountain Cluster)


Sochi, Russia Winter Olympic Sites (Mountain Cluster)
The 2014 Winter Olympic ski runs may be rated double black diamond, but they're not quite as steep as they appear in this image of the skiing and snowboarding sites for the Sochi Winter Olympic Games, acquired on Jan. 4, 2014, by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra spacecraft. Rosa Khutar ski resort near Sochi, Russia, is in the valley at center, and the runs are visible on the shadowed slopes on the left-hand side of the valley. Height has been exaggerated 1.5 times to bring out topographic details. The games, which begin on Feb. 7 and continue for 17 days, feature six new skiing and boarding events plus the return of the legendary Jamaican bobsled team to the winter games for the first time since 2002.
In this southwest-looking image, red indicates vegetation, white is snow, and the resort site appears in gray. The area imaged is about 11 miles (18 kilometers) across in the foreground and 20 miles (32 kilometers) from front to back. The image was created from the ASTER visible and near-infrared bands, draped over ASTER-derived digital elevation data.
With its 14 spectral bands from the visible to the thermal infrared wavelength region and its high spatial resolution of 15 to 90 meters (about 50 to 300 feet), ASTER images Earth to map and monitor the changing surface of our planet. ASTER is one of five Earth-observing instruments launched Dec. 18, 1999, on Terra. The instrument was built by Japan's Ministry of Economy, Trade and Industry. A joint U.S./Japan science team is responsible for validation and calibration of the instrument and data products.
The broad spectral coverage and high spectral resolution of ASTER provides scientists in numerous disciplines with critical information for surface mapping and monitoring of dynamic conditions and temporal change. Example applications are: monitoring glacial advances and retreats; monitoring potentially active volcanoes; identifying crop stress; determining cloud morphology and physical properties; wetlands evaluation; thermal pollution monitoring; coral reef degradation; surface temperature mapping of soils and geology; and measuring surface heat balance.
The U.S. science team is located at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The Terra mission is part of NASA's Science Mission Directorate, Washington, D.C. ;More information about ASTER is available at asterweb.jpl.nasa.gov/.
Image Credit: NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team

NASA
Guillermo Gonzalo Sánchez Achutegui

martes, 8 de octubre de 2013

ESA : European ground stations enable Galileo search and rescue testing


Maspalomas station

European ground stations enable Galileo search and rescue testing

8 October 2013
ESA’s completion of a pair of dedicated ground stations at opposite ends of Europe has enabled Galileo satellites in orbit to participate in global testing of the Cospas–Sarsat search and rescue system.
The Maspalomas station, at the southern end of the largest island of the Canary Islands, at the southern fringe of European waters, was activated in June. And this last month has seen the Svalbard site on Spitsbergen in the Norwegian Arctic come on line – the two sites can already communicate and will soon be performing joint tests.
This speedy progress has enabled the participation of the latest two Galileo satellites in an international demonstration and evaluation programme – a worldwide test campaign for a new expansion of the world’s oldest and largest satellite-based rescue system, Cospas–Sarsat.
Founded by Canada, France, Russia and the US, Cospas–Sarsat has assisted in the rescue of tens of thousands of souls in its three decades of service. Distress signals from across the globe are detected by satellites, then swiftly relayed to the nearest search and rescue (SAR) authorities.
Svalbard station
Now the programme is introducing a new medium-orbit SAR system to improve coverage and response times, with the Galileo satellites in the vanguard of this major expansion.
Supporting search and rescue is a separate function to Galileo’s main task of providing global navigation and timing services, but no less important.
The second pair of Europe’s Galileo satellites – launched together on 12 October last year – are the first of the constellation to host SAR payloads. These can pick up UHF signals from emergency beacons aboard ships, aircraft or carried by individuals, which are then relayed to ground stations. There, the source is pinpointed and automatically passed on to a control centre, which then routes it to local authorities for rescue.
Test localisation from Maspalomas
“The Galileo satellites, tested in combination with the same SAR payloads on Russian Glonass satellites as well as compatible repeaters on a pair of US GPS satellites, showed an ability to pinpoint simulated emergency beacons down to an accuracy of 2–5 km in a matter of minutes,” explained ESA’s Galileo SAR engineer, Igor Stojkovic.
“Our in-orbit validation tests so far have been in line with expectation and beyond, giving us a lot of confidence in the performance of the final system, once completed.
“And using a combination of satellites is just how the upgraded system will operate in practice, in order to localise distress signals.”
 
 
Cospas–Sarsat system
Currently, Cospsas–Sarsat relies on satellites in both low and geostationary orbits. Galileo’s SAR payloads support the introduction of a new system based instead on satellites in medium orbits, combining the ability to perform rapid localisation with the very wide field of view afforded by the satellites’ high altitude – 23 222 km in the case of Galileo.
This increases the probability that the alert will be detected by multiple satellites at once, especially important if the beacon is partially obscured in a rugged landscape.
This high vantage point also means much fewer ground stations are required: “Just a trio of these stations has been deemed enough to serve all of European territory,” explained Erik van der Wenden, who oversaw their procurement for ESA.
“Maspalomas and Spitsbergen will combine with a third station at Larnaca in Cyprus, currently approaching completion. These three sites are monitored and controlled from the SAR Ground Segment Data Service Provider site, based at Toulouse in France.
Extending Europe's search and rescue cover
“Each site is equipped with four antennas to track four satellites. The stations are networked to share raw data, effectively acting as a single huge 12-antenna station, achieving unprecedented detection time and localisation accuracy.”
All future Galileo satellites will carry SAR payloads, as will Glonass and the new generation of US GPS satellites, debuting later this decade.
In 2015–16, as the number of available satellites in medium orbits increases, the service will enter ‘Initial Operational Capability’, although an initial ‘SAR/Galileo Early Service’ is expected to start sooner.
 
 
ESA
Guillermo Gonzalo Sánchez Achutegui

lunes, 29 de julio de 2013

NASA - Cloud Streets over the Bering Sea


The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this natural-color image of clouds stretched in parallel rows over the Bering Sea on April 7, 2013. Image Credit: NASA GSFC
 
Cloud Streets over the Bering Sea
In early April 2013, clouds stretched in parallel rows for hundreds of kilometers over the Bering Sea. The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this natural-color image of the phenomenon on April 7, 2013.
The parallel clouds, known as cloud streets, originated along the edge of the sea ice, which extended southward from the snow-covered expanses of Russia and Alaska. The location of the cloud formation was not a coincidence. When cold air blows over ice and snow and encounters moist air over open water, the meeting of the air masses can cause the formation of parallel cylinders of spinning air. Clouds form along the upward cycle in the cylinders, where air is rising, and skies remain clear along the downward cycle, where air is falling.
In the north, light cloud cover partially obscured the sea ice, but its characteristic tendril shapes could still be seen through the clouds.
Image Credit: Jeff Schmaltz, LANCE/EOSDIS MODIS Rapid Response Team at NASA GSFC
Caption: Michon Scott
NASA
Guillermo Gonzalo Sánchez Achutegui
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miércoles, 8 de mayo de 2013

ESA - Expertos europeos se reúnen en Madrid para evaluar las opciones ante un asteroide como el de Chelyabinsk






Asteroid trace over Chelyabinsk, Russia, on 15 February 2013
8 May 2013
In February, a speeding asteroid slammed into our atmosphere and exploded high over Russia’s Ural region, injuring hundreds and causing millions of euros of damage. What should we do if we have a similar – or even bigger – strike in the future?
Of the more than 600 000 known asteroids in our Solar System, almost 10 000 are classified as near-Earth objects, or NEOs, because their orbits bring them relatively close to Earth’s path. 
Dramatic proof that any of these can strike Earth came on 15 February, when an unknown object thought to be 17–20 m in diameter arrived at 66 000 km/h and exploded high above Chelyabinsk, Russia, with 20–30 times the energy of the Hiroshima atomic bomb.
The resulting shock wave caused widespread damage and injuries, making it the largest known natural object to have entered the atmosphere since the 1908 Tunguska event, which destroyed a remote forest area of Siberia.
“It’s important that we become aware of the current and future position of NEOs, develop estimates on the likelihood of impacts and assess the possible consequences,” says Detlef Koschny, Head of NEO activities in the Agency’s Space Situational Awareness (SSA) Programme Office.
Artist's impression of NEO asteroids passing Earth ESA SSA
Artist's impression of asteroids passing Earth
“More importantly, we must consider whether and how warning, mitigation and possible deflection actions can be taken. It’s important not only for Europe, but for the rest of the planet, too.”
One aspect of ESA’s four-year-old effort requires the development of an integrated system to scan the sky nightly for as-yet-undiscovered NEOs.
Another important element is studying how mitigation measures can be applied in the case of smaller NEOs, and how to deflect any larger ones that may seriously threaten our home planet.
This week, Deimos Space, an industrial partner working for ESA on SSA, has invited top researchers from universities, research institutes, national space agencies and industry in Europe and the USA to discuss the state of the art in NEO impact effects and threat mitigation.
The meeting is taking place in Tres Cantos, Spain, near Madrid.
“A great deal of work remains to be done, for example, in computer modelling of impact effects, how airbursts differ from ground strikes, kinetic versus explosive deflection strategies and much more,” says Gerhard Drolshagen, of the SSA Programme Office.
“The aim is to develop plans that will guide us in current and future NEO research and development.”
Ultimately, ESA aims to develop the capability to integrate European current and new assets such as automated telescopes into a coordinated and more efficient NEO system that can provide nightly sky surveys and advanced warning.
“With this, we can work with our partner agencies, scientists, industry and international bodies like the UN to offer firm options to national governments and political decision-makers,” says Nicolas Bobrinsky, Head of ESA’s SSA Programme.
“Events like the Chelyabinsk strike show that the NEO hazard is not just theoretical, and we need to invest in practical measures today to address tomorrow’s threats.”
Editor’s note: A summary of the workshop findings will be available as a downloadable PDF after 8 May.
ESA
Guillermo Gonzalo Sánchez Achutegui
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miércoles, 6 de marzo de 2013

nsf.gov - News - Incoming! Then Outgoing! Waves Generated by Russian Meteor Recorded Crossing the U.S.

Network of stations with seismometers and air pressure sensors detected the blast waves.-
 
 Sky showing a meteor trail over eastern Russia

Meteor trail over eastern Russia is seen in this image from the Russian Emergency Ministry.
Credit: Russian Emergency Ministry
Download the high-resolution JPG version of the image. (78 KB) 
 Map showing the trajectory of the meteor as it neared impact in Russia.

Trajectory of the meteor as it neared impact in Russia.
Credit: Wikimedia Commons
Download the high-resolution JPG version of the image. (84 KB)
 Sky showing a meteor as it streaked by buildings in Russia.

Is it a bird, a plane, a...meteor? A view of the meteor as it streaked by buildings in Russia.
Credit: Russian Emergency Ministry
Download the high-resolution JPG version of the image. (101 KB)
 People standing next to hole in the ice at Russia's Lake Chebarkul, said to be caused by the meteor.

Hole in the ice at Russia's Lake Chebarkul, said to be caused by the meteor.
Credit: Wikimedia Commons
Download the high-resolution JPG version of the image. (33 KB) Stores with shattered windows from the meteor that crashed in eastern Russia.

As the meteor streaked by then crashed, window glass in eastern Russia shattered.
Credit: Russian Emergency Ministry
Download the high-resolution JPG version of the image. (142 KB)



Infrasound pressure waves are detected by a sensor installed in an EarthScope TA station. 
 Infrasound pressure waves are detected by a sensor installed in an EarthScope TA station.
Credit: IRIS
Download the high-resolution JPG version of the image. (509 KB)
A network of seismographic stations recorded spectacular signals from the blast waves of the meteor that landed near Chelyabinsk, Russia, as the waves crossed the United States.
The National ScieMeteornce Foundation- (NSF) supported stations are used to study earthquakes and the Earth's deep interior.
While thousands of earthquakes around the globe are recorded by seismometers in these stations--part of the permanent Global Seismographic Network (GSN) and EarthScope's temporary Transportable Array (TA)--signals from large meteor impacts are far less common.
The meteor explosion near Chelyabinsk on Feb. 15, 2013, generated ground motions and air pressure waves in the atmosphere. The stations picked up the signals with seismometers and air pressure sensors.
The ground motions were recorded by the GSN and the TA. The pressure waves were detected by special sensors that are part of the TA.
"The NSF-supported Global Seismic Network and EarthScope Transportable Array made spectacular recordings of the Chelyabinsk meteor's impact," says Greg Anderson, program director in NSF's Division of Earth Sciences.
"These recordings of seismic waves through the Earth, and sound waves through the atmosphere, are good examples of how these facilities can help global organizations better monitor earthquakes, clandestine nuclear tests and other threats."
Incoming! Then outgoing!
The Chelyabinsk meteor exploded in the atmosphere at approximately 9.20 a.m. local time.
The blast caused significant damage in the city, breaking thousands of windows and injuring more than 1,000 people.
Energy from the blast created pressure waves in the atmosphere that moved rapidly outward and around the globe. The blast also spread within the Earth as a seismic wave.
The two wave types--seismic wave and pressure wave--travel at very different speeds.
Waves in the ground travel quickly, at about 3.4 kilometers per second. Waves in the atmosphere are much slower, moving at about 0.3 kilometers per second, and can travel great distances.
GSN stations in Russia and Kazakhstan show the ground-traveling wave as a strong, abrupt pulse with a duration of about 30 seconds.
The atmospheric waves--referred to as infrasound--were detected across a range of inaudible frequencies and were observed at great distances on infrasound microphones.
When the infrasound waves reached the eastern United States--after traveling 8.5 hours through the atmosphere across the Arctic from the impact site in Russia--they were recorded at TA stations at the Canadian border.
The infrasound waves reached Florida three hours later, nearly 12 hours after the blast.
Infrasound sensors at TA stations along the Pacific coast and in Alaska also recorded the blast, but with signatures that were shorter and simpler than those recorded by stations in the mid-continent and along the southeastern seaboard.
The duration of the signals, and the differences between the waveforms in the east and west, scientists believe, are related to the way in which energy travels and bounces on its long path through the atmosphere.
EarthScope Transportable Array
The Transportable Array is operated by the IRIS (Incorporated Research Institutions for Seismology) Consortium as part of NSF's EarthScope Project. It consists of 400 stations traversing the United States, recording at each site along the way for two years.
Each of the TA stations was originally equipped with sensitive broadband seismometers for measuring ground motions, but in 2010, NSF awarded the University of California, San Diego, in cooperation with IRIS, funding to add pressure and infrasound sensors.
These special sensors help scientists understand how changes in pressure affect ground motions recorded by the TA's seismometers and provide a view of regional pressure changes related to weather patterns.
The sensors also record events such as tornadoes, derechos, rocket launches, chemical explosions--and meteor impacts.
The Chelyabinsk meteor is the largest signal recorded to date.
In 2013, the Transportable Array will reach states in the Northeast, completing its traverse of the contiguous United States and southern Canada.
Global Seismographic Network
The GSN's primary mission is collecting data to monitor worldwide earthquakes and to study the Earth's deep interior.
It's funded jointly by NSF and the U.S. Geological Survey and is managed and operated by IRIS in collaboration with the U.S. Geological Survey's Albuquerque Seismological Laboratory and the University of California, San Diego.
As part of a worldwide network of seismic stations, data from the GSN have contributed over the past three decades to the monitoring of nuclear explosions at test sites in the United States, the former Soviet Union, India, Pakistan and Korea. For example, GSN stations provided observations of the Korean nuclear test on Feb. 12, 2013.
-NSF-
Media Contacts Cheryl Dybas, NSF (703) 292-7734 cdybas@nsf.gov
Related WebsitesNSF EarthScope Project: http://www.earthscope.org
Incorporated Research Institutions for Seismology: http://www.iris.edu
Global Seismographic Network: http://www.iris.edu/hq/programs/gsn
IRIS 'special event' page for the Chelyabinsk meteor: http://www.iris.edu/dms/nodes/dmc/specialevents/2013/02/19/chelyabinsk-russia-bolide-meteor/
The National Science Foundation (NSF) is an independent federal agency that supports fundamental research and education across all fields of science and engineering. In fiscal year (FY) 2012, its budget is $7.0 billion. NSF funds reach all 50 states through grants to nearly 2,000 colleges, universities and other institutions. Each year, NSF receives over 50,000 competitive requests for funding, and makes about 11,000 new funding awards. NSF also awards nearly $420 million in professional and service contracts yearly.
Useful NSF Web Sites:
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/

 The National Science Foundation (NSF).-
 Guillermo Gonzalo Sánchez Achutegui
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