Carla Suárez applauds the reverse to a hand of Bouchard

first_imgEugenie Bouchard continues her coaching for the return of the season in tennis. The Canadian tennis participant, who has not had a good begin to the season, desires to redeem herself and for this she has began to enhance some photographs that assist her enhance her outcomes. One of these blows is the reverse to one hand, as Bouchard herself confirmed by means of social networks with a video of a coaching session and the remark. “Hello guys, a fast announcement: As we’ve a lengthy break forward, I’ve determined to make a change to my recreation. I’m changing into a one-handed participant! It has all the time been my dream to play backhand with one hand. I’m very enthusiastic about this journey forward! “ hey guys, fast announcement: since we’ve such a lengthy break forward of us i’ve determined to make a change in my recreation. I’m switching to a one hander! it’s all the time been a dream of mine to play with a one handed backhand. I’m so excited for this journey forward! pic.twitter.com/gnsWJwN1NG– Genie Bouchard (@geniebouchard) April 1, 2020center_img 🙊🙊😅😅 Just isn’t simple!– Carla Suárez Navarro (@CarlaSuarezNava) April 1, 2020After the video, the group of the Coupe Rogers, the most essential event in Canada, requested Carla Suárez, specialist on this sort of blows, due to the Canadian’s skill, to which the Canarian replied: “It’s not simple!”. Phrase from a specialist that Bouchard will attempt to take be aware of to get better his greatest tennis.last_img read more

This global telescope may finally see the event horizon of our galaxys

first_imgThe EHT takes aim just once a year, when good weather is likely, when both black holes are visible in the sky, and when it’s possible to get time at all the observatories around the globe. This year, the team will observe for 5 nights during a 10-night window from 5 to 14 April. Then, an intensive data processing effort begins, and it may be a year before they know whether they’ve succeeded. “It’s an exercise in delayed gratification. Delayed gratification squared,” says EHT director Shep Doeleman at the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts.Imaging black holes is a formidable challenge, and not just because their intense gravity prevents even light from escaping. They are also surprisingly small. Sgr A* is calculated to contain the mass of 4 million suns, based on the nervy, high-speed orbits of stars in its gravitational grip. But its event horizon, the point of no return for anything approaching a black hole, is 24 million kilometers across, just 17 times wider than the sun. To see something so small from 26,000 light-years away requires a telescope dish of global dimensions.At optical wavelengths, Sgr A* is hidden by the shroud of dust and gas obscuring the galaxy’s heart. Radio waves can pass through more easily, but ordinary radio dishes are still hampered by ionized gas clouds and low resolution. Best are telescopes sensitive to the shortest radio waves—millimeter waves—but the dishes, detectors, and data processing technology for this part of the spectrum were developed only in the past few decades. “There is only a tiny window where we can see the event horizon,” says Heino Falcke, an astrophysicist at Radboud University in Nijmegen, the Netherlands, and chair of the EHT science council. “The Milky Way is like a milky glass.” A shot in the dark The Event Horizon Telescope now combines eight millimeter-wave radio observatories into a global telescope. The farther apart they are, the better the resolution. By Daniel CleryMar. 2, 2017 , 9:00 AM Click to view the privacy policy. Required fields are indicated by an asterisk (*) This global telescope may finally see the event horizon of our galaxy’s giant black hole Early this decade, Doeleman and other EHT researchers began testing the idea with millimeter-sensitive dishes in Hawaii, California, and Arizona. Later, they extended the array to include the Large Millimeter Telescope in Mexico. Along the way, they got a good enough image of the black hole in M87 to see the base of its matter-spewing jets—data that are helping them understand how the jets are created. In 2015, they glimpsed the magnetic field around Sgr A*, which may help explain how black holes heat up the material around them.But to see the event horizon itself, the EHT had to grow even larger. Over the years, it has evolved from a loose, poorly funded group to a worldwide collaboration involving 30 institutions in 12 countries. Next month it will include farflung additions, including the IRAM dish in Spain, the South Pole Telescope, and the Atacama Large Millimeter/submillimeter Array (ALMA), a large international observatory comprising 66 dishes in northern Chile. With its huge dish area, ALMA is the big catch because it will boost the EHT’s sensitivity by an order of magnitude. “That’s the key for us,” Doeleman says.Adding new instruments isn’t simple. The technique for combining signals from distant dishes is known as very long baseline interferometry, and most millimeter-wave telescopes are not equipped to take part. EHT researchers had to visit each facility to tinker with its hardware and install new digital signal processors and data recorders. In the case of ALMA, that took some persuading. “We had to go into the bowels of ALMA and rewire it,” Doeleman says. “It required political buy-in at all levels.”The campaign next month will be a nervous time for the EHT team. All eight observatories need clear skies and no technical glitches to get the best possible observations. “The first time, things can go wrong,” Falcke says. Data volumes will be so large that they have to be recorded on hard drives and shipped back to the Haystack Observatory in Westford, Massachusetts, and the Max Planck Institute for Radio Astronomy in Bonn, Germany, for processing. There, devices known as correlators, made from clusters of PCs but with the power of supercomputers, will spend months crunching through the data, combining the signals from separate dishes as if they came from a single dish as wide as Earth. Adding further delay, data from the South Pole Telescope won’t arrive until September or October, when planes can retrieve the hard drives after the Antarctic winter.When the data finally all come together sometime next year, the team hopes to see a bright ring of light from photons orbiting close to the event horizon, with a dark disk in its center. The ring should be brighter on one side, where the rotation of the black hole gives photons a boost, although the images on this first attempt may not be as crisp as the team’s simulations. “It’ll probably be a crappy image, but scientifically it will be very interesting,” Falcke says.Doeleman hopes to see structure in the matter swirling around the event horizon and watch, movielike, as gas falls into it and vanishes. Such observations might help explain why some black holes gorge on matter and shine brightly, whereas others—like Sgr A*—seem to be on a starvation diet. Falcke has a simpler wish. “The event horizon is the defining thing about a black hole,” he says. “I hope to see it; to literally see it.” Email Country * Afghanistan Aland Islands Albania Algeria Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas Bahrain Bangladesh Barbados Belarus Belgium Belize Benin Bermuda Bhutan Bolivia, Plurinational State of Bonaire, Sint Eustatius and Saba Bosnia and Herzegovina Botswana Bouvet Island Brazil British Indian Ocean Territory Brunei Darussalam Bulgaria Burkina Faso Burundi Cambodia Cameroon Canada Cape Verde Cayman Islands Central African Republic Chad Chile China Christmas Island Cocos (Keeling) Islands Colombia Comoros Congo Congo, the Democratic Republic of the Cook Islands Costa Rica Cote d’Ivoire Croatia Cuba Curaçao Cyprus Czech Republic Denmark Djibouti Dominica Dominican Republic Ecuador Egypt El Salvador Equatorial Guinea Eritrea Estonia Ethiopia Falkland Islands (Malvinas) Faroe Islands Fiji Finland France French Guiana French Polynesia French Southern Territories Gabon Gambia Georgia Germany Ghana Gibraltar Greece Greenland Grenada Guadeloupe Guatemala Guernsey Guinea Guinea-Bissau Guyana Haiti Heard Island and McDonald Islands Holy See (Vatican City State) Honduras Hungary Iceland India Indonesia Iran, Islamic Republic of Iraq Ireland Isle of Man Israel Italy Jamaica Japan Jersey Jordan Kazakhstan Kenya Kiribati Korea, Democratic People’s Republic of Korea, Republic of Kuwait Kyrgyzstan Lao People’s Democratic Republic Latvia Lebanon Lesotho Liberia Libyan Arab Jamahiriya Liechtenstein Lithuania Luxembourg Macao Macedonia, the former Yugoslav Republic of Madagascar Malawi Malaysia Maldives Mali Malta Martinique Mauritania Mauritius Mayotte Mexico Moldova, Republic of Monaco Mongolia Montenegro Montserrat Morocco Mozambique Myanmar Namibia Nauru Nepal Netherlands New Caledonia New Zealand Nicaragua Niger Nigeria Niue Norfolk Island Norway Oman Pakistan Palestine Panama Papua New Guinea Paraguay Peru Philippines Pitcairn Poland Portugal Qatar Reunion Romania Russian Federation Rwanda Saint Barthélemy Saint Helena, Ascension and Tristan da Cunha Saint Kitts and Nevis Saint Lucia Saint Martin (French part) Saint Pierre and Miquelon Saint Vincent and the Grenadines Samoa San Marino Sao Tome and Principe Saudi Arabia Senegal Serbia Seychelles Sierra Leone Singapore Sint Maarten (Dutch part) Slovakia Slovenia Solomon Islands Somalia South Africa South Georgia and the South Sandwich Islands South Sudan Spain Sri Lanka Sudan Suriname Svalbard and Jan Mayen Swaziland Sweden Switzerland Syrian Arab Republic Taiwan Tajikistan Tanzania, United Republic of Thailand Timor-Leste Togo Tokelau Tonga Trinidad and Tobago Tunisia Turkey Turkmenistan Turks and Caicos Islands Tuvalu Uganda Ukraine United Arab Emirates United Kingdom United States Uruguay Uzbekistan Vanuatu Venezuela, Bolivarian Republic of Vietnam Virgin Islands, British Wallis and Futuna Western Sahara Yemen Zambia Zimbabwe CREDITS: (GRAPHIC) ADAPTED BY A. CUADRA/SCIENCE; (DATA) EVENT HORIZON TELESCOPE Sign up for our daily newsletter Get more great content like this delivered right to you! Country Last year researchers “heard” black holes for the first time, when they detected the gravitational waves unleashed as two of them crashed together and merged. Now, they want to see a black hole, or at least its silhouette. Next month, astronomers will harness radio telescopes across the globe to create the equivalent of a single Earth-spanning dish—an instrument powerful enough, they hope, to image black holes backlit by the incandescent gas swirling around them. Their targets are the supermassive black hole at the heart of our Milky Way galaxy, known as Sagittarius A* (Sgr A*), and an even bigger one in the neighboring galaxy M87.Earlier observations using this Event Horizon Telescope (EHT) without its full roster of dishes yielded tantalizing results, but in images the two black holes remained featureless blobs. This year, for the first time, the EHT will add dishes in Chile and Antarctica, sharpening its resolution and raising expectations. Astronomers now hope to see how the black holes whip the hot gas around them into accretion disks and spawn matter-spewing jets. They also hope to chart the size and shape of the event horizon—the boundary of the black hole—to test whether Albert Einstein’s theory of gravity, general relativity, still works under such extreme conditions.”It’s a very bold and gutsy experiment,” says theoretical astrophysicist Roger Blandford of Stanford University in Palo Alto, California, who is not involved in the project. Blandford believes the EHT may not only show how black holes work, but also deliver a more fundamental message. “It will validate this remarkable proposition: that black holes are common in the universe. Seeing is believing.”last_img read more