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"content": "\u003cp>Diversity of thought has always been a cornerstone of science; however, diversity amongst scientists has often gone unnoticed. Martin Luther King’s \u003ca href=\"http://www.mlkday.gov/\">birthday\u003c/a> was just celebrated in remembrance of his leadership in the African American community. However, he is not the only pioneer who has brought about great and lasting change. Below are just two examples of the great scientists and innovators in the African American community who have graced the history of science for the betterment of mankind.\u003c/p>\n\u003cp>\u003cstrong>George Washington Carver: (1864-1943)\u003c/strong>\u003cbr>\n\u003cem>\u003cstrong> Agricultural Chemist and Innovator\u003c/strong>\u003c/em>\u003c/p>\n\u003cp>On the epitaph on the grave of George Washington Carver it reads, \"He could have added fortune to fame, but caring for neither, he found happiness and honor in being helpful to the world.”\u003c/p>\n\u003cp>Through his work as an agricultural chemist, Dr. George Washington Carver changed the agriculture of the South by discovering three hundred uses for peanuts and hundreds more uses for soybeans, pecans and sweet potatoes. From the peanut Dr. Carver created meal, instant and dry coffee, bleach, tar remover, wood filler, metal polish, paper, ink, shaving cream, rubbing oil, linoleum, synthetic rubber, and plastics. 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This was the first U.S. federal monument dedicated to an African-American.\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2008/01/matthew-henson.bmp\">\u003cem>Matthew Henson\u003c/em>\u003c/span>\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>\u003cstrong>Matthew Alexander Henson (1866-1955)\u003c/strong>\u003cbr>\n\u003cem>\u003cstrong> Arctic Explorer\u003c/strong>\u003c/em>\u003c/p>\n\u003cp>\u003cem>\"As I stood at the top of the world and thought of the hundreds of men who had lost their lives in the effort to reach it, I felt profoundly grateful that I, as the personal attendant of the commander, had the honor of representing my race in the historic achievement.\"\u003c/em>\u003c/p>\n\u003cp>Matthew Henson was the first man to reach the geographic North Pole with long time colleague and explorer Robert Peary. Henson was born of poor parents in Charles County, Maryland. 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The Academy is a wonderful fit for her because of her curiosity about the natural world and her experience in working with native California wildlife.\u003c/em>\u003c/p>\n\u003cp>\u003cbr clear=\"all\">\u003c/p>\n\u003cp>\u003c/p>\n\u003cp class=\"geo\"> latitude: 37.769\u003cspan class=\"latitude\">\u003c/span>, longitude:-122.467\u003cspan class=\"longitude\">\u003c/span>\u003c/p>\n\n",
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"content": "\u003cp>\u003cstrong>In the North Bay, a new nursery is lending Mother Nature a hand.\u003c/strong>\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2007/12/blog_nursery.jpg\">\u003c/span>On a recent foggy morning, I drove up to the \u003ca href=\"http://www.fws.gov/refuges/profiles/index.cfm?id=11644\">San Pablo Bay National Wildlife Refuge\u003c/a> to tour their native plant nursery with biologist Giselle Block and nursery manager Leia Giambastiani. The Refuge hugs the northern reaches of the Bay (If you've driven across Highway 37, you've seen some of it). Historically this was part of one of the most extensive wetland systems on the West Coast. Here at the Bay's ecologically rich fringes, habitats shaded one to the next, from open water, to mudflat, to tidal marsh, to upland. During extreme high tides, marsh inhabitants like salt marsh harvest mouse and California clapper rail--both now endangered--sought refuge in the marsh-upland transition zone, where native plants provided cover from predation.\u003c/p>\n\u003cp>Over the past 150 years, the marsh-upland transition zone has, so to speak, gone the way of the wetlands. Now, with plans to restore 100,000 acres of the Bay's lost wetlands in the coming decades, scientists also are turning their attention to the critical habitat just above tide line. These days, as a result of our radical re-engineering of the Bay landscape, the transition zone is often on man made levees.\u003c/p>\n\u003cp>Once reconnected to the Bay, tidal marshes can do a lot of the work of restoring themselves, as seeds and nutrients travel in on the tides. But the transition zone is not so lucky. Without sources nearby, many seeds don't have a way to get there. Even if they manage the journey, native plants face stiff competition on levees from weedy invaders. Here's where the Refuge's nursery comes in, raising from seed native plants such as yarrow (\u003cem>Achillea millefolium\u003c/em>), blue wildrye (\u003cem>Elymus glaucus\u003c/em>), seaside woolly sunflower (\u003cem>Eriophyllum staechadifolium\u003c/em>), and western goldenrod (\u003cem>Euthamia occidentalis\u003c/em>), then marshaling volunteers to help remove invasives and plant the natives. In 2007--just its second year--the nursery propagated over 4,000 plants.\u003c/p>\n\u003cp>What makes this restoration work particularly exciting is that it is truly science in action, an ongoing experiment still working to answer a variety of questions: what's the best way to get rid of invasives? (Different projects around the Bay have experimented with using a plastic sheeting to \"cook\" the weed seeds--\u003cem>solarization\u003c/em>--and using concentrated salt water from salt ponds to poison them--\u003cem>salinization\u003c/em>). Which native plants fare best on the levees, a relatively harsh environment with soils that may differ from natural transition zones? Should the new plantings be left to do their thing, or do survival rates significantly improve with mulching or fertilizer?\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>And what happens when, as a result of climate change and sea level rise, you run out of levee? Giselle Block points out that no doubt there will be new levees in new places. By working now to create habitat, there will be local sources for seeding new transitions zones, and--hopefully--there will still be clapper rails and salt marsh harvest mice to seek refuge there.\u003c/p>\n\u003cp>\u003cem>The Refuge and The Bay Institute are partnering to develop more opportunities for volunteers to assist with propagation of native plants at the nursery, invasive removal, and restoration plantings. For more information, contact Leia Giambastiani (707-769-4200, \u003ca href=\"mailto:giambastiani@bay.org\">giambastiani@bay.org\u003c/a>).\u003c/em>\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/icon_annd.jpg\">\u003c/span>\u003cem>\u003cstrong>Ann Dickinson\u003c/strong> is Communications Manager for The Bay Institute (\u003ca href=\"http://www.bay.org\">www.bay.org\u003c/a>), a nonprofit research, education, and advocacy organization dedicated to protecting and restoring San Francisco Bay and its watershed, \"from the Sierra to the sea.\"\u003c/em>\u003cbr>\n\u003cbr clear=\"all\">\u003c/p>\n\u003cp>\u003c/p>\n\u003cp class=\"geo\"> latitude: \u003cspan class=\"latitude\">38.1528\u003c/span>, longitude: \u003cspan class=\"longitude\">-122.492\u003c/span>\u003c/p>\n\n",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>\u003cstrong>In the North Bay, a new nursery is lending Mother Nature a hand.\u003c/strong>\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2007/12/blog_nursery.jpg\">\u003c/span>On a recent foggy morning, I drove up to the \u003ca href=\"http://www.fws.gov/refuges/profiles/index.cfm?id=11644\">San Pablo Bay National Wildlife Refuge\u003c/a> to tour their native plant nursery with biologist Giselle Block and nursery manager Leia Giambastiani. The Refuge hugs the northern reaches of the Bay (If you've driven across Highway 37, you've seen some of it). Historically this was part of one of the most extensive wetland systems on the West Coast. Here at the Bay's ecologically rich fringes, habitats shaded one to the next, from open water, to mudflat, to tidal marsh, to upland. During extreme high tides, marsh inhabitants like salt marsh harvest mouse and California clapper rail--both now endangered--sought refuge in the marsh-upland transition zone, where native plants provided cover from predation.\u003c/p>\n\u003cp>Over the past 150 years, the marsh-upland transition zone has, so to speak, gone the way of the wetlands. Now, with plans to restore 100,000 acres of the Bay's lost wetlands in the coming decades, scientists also are turning their attention to the critical habitat just above tide line. These days, as a result of our radical re-engineering of the Bay landscape, the transition zone is often on man made levees.\u003c/p>\n\u003cp>Once reconnected to the Bay, tidal marshes can do a lot of the work of restoring themselves, as seeds and nutrients travel in on the tides. But the transition zone is not so lucky. Without sources nearby, many seeds don't have a way to get there. Even if they manage the journey, native plants face stiff competition on levees from weedy invaders. Here's where the Refuge's nursery comes in, raising from seed native plants such as yarrow (\u003cem>Achillea millefolium\u003c/em>), blue wildrye (\u003cem>Elymus glaucus\u003c/em>), seaside woolly sunflower (\u003cem>Eriophyllum staechadifolium\u003c/em>), and western goldenrod (\u003cem>Euthamia occidentalis\u003c/em>), then marshaling volunteers to help remove invasives and plant the natives. In 2007--just its second year--the nursery propagated over 4,000 plants.\u003c/p>\n\u003cp>What makes this restoration work particularly exciting is that it is truly science in action, an ongoing experiment still working to answer a variety of questions: what's the best way to get rid of invasives? (Different projects around the Bay have experimented with using a plastic sheeting to \"cook\" the weed seeds--\u003cem>solarization\u003c/em>--and using concentrated salt water from salt ponds to poison them--\u003cem>salinization\u003c/em>). Which native plants fare best on the levees, a relatively harsh environment with soils that may differ from natural transition zones? Should the new plantings be left to do their thing, or do survival rates significantly improve with mulching or fertilizer?\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>And what happens when, as a result of climate change and sea level rise, you run out of levee? Giselle Block points out that no doubt there will be new levees in new places. By working now to create habitat, there will be local sources for seeding new transitions zones, and--hopefully--there will still be clapper rails and salt marsh harvest mice to seek refuge there.\u003c/p>\n\u003cp>\u003cem>The Refuge and The Bay Institute are partnering to develop more opportunities for volunteers to assist with propagation of native plants at the nursery, invasive removal, and restoration plantings. For more information, contact Leia Giambastiani (707-769-4200, \u003ca href=\"mailto:giambastiani@bay.org\">giambastiani@bay.org\u003c/a>).\u003c/em>\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/icon_annd.jpg\">\u003c/span>\u003cem>\u003cstrong>Ann Dickinson\u003c/strong> is Communications Manager for The Bay Institute (\u003ca href=\"http://www.bay.org\">www.bay.org\u003c/a>), a nonprofit research, education, and advocacy organization dedicated to protecting and restoring San Francisco Bay and its watershed, \"from the Sierra to the sea.\"\u003c/em>\u003cbr>\n\u003cbr clear=\"all\">\u003c/p>\n\u003cp>\u003c/p>\n\u003cp class=\"geo\"> latitude: \u003cspan class=\"latitude\">38.1528\u003c/span>, longitude: \u003cspan class=\"longitude\">-122.492\u003c/span>\u003c/p>\n\n\u003c/div>\u003c/p>",
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"content": "\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2007/12/starsflash_blog.jpg\">\u003cem>Credit: T. Credner & S. Kohle, AlltheSky.com\u003c/em>\u003c/span>You may be surprised to hear that \u003ca href=\"http://www.nasa.gov/worldbook/venus_worldbook.html\" target=\"_blank\">Venus\u003c/a> is the warmest planet in the solar system. Venus has an average temperature of 850 degrees Fahrenheit. This is much warmer than the \u003ca href=\"http://www.nasa.gov/worldbook/earth_worldbook.html\" target=\"_blank\">Earth\u003c/a>, at 60 degrees, and even warmer than \u003ca href=\"http://www.nasa.gov/worldbook/mercury_worldbook.html\" target=\"_blank\">Mercury\u003c/a>, which sits much closer to the sun, at 350 degrees. A reader asked if the high temperature on Venus was related to the composition of the atmosphere.\u003c/p>\n\u003cp>It turns out that the atmosphere of Venus is actually made almost entirely of carbon dioxide, and a lot of it. Because of this thick atmosphere and clouds of reflective sulfuric acid, not much was known about the planet's surface until recently. Before 1960, astronomers couldn't even estimate the length of one day on Venus! Now \u003ca href=\"http://en.wikipedia.org/wiki/Satellite\" target=\"_blank\">satellites\u003c/a>, like the \u003ca href=\"http://sci.esa.int/science-e/www/area/index.cfm?fareaid=64\" target=\"_blank\">Venus Express\u003c/a>, orbit around the planet and \u003ca href=\"http://en.wikipedia.org/wiki/Lander_%28spacecraft%29\" target=\"_blank\">landers\u003c/a>, like the \u003ca href=\"http://nssdc.gsfc.nasa.gov/planetary/venera.html\" target=\"_blank\">Soviet Venera\u003c/a>, have reached the surface.\u003c/p>\n\u003cp>We now know that the surface of Venus is scarred with impact craters, lava flows and more volcanoes than any other planet in the solar system. We know that the atmosphere is almost entirely carbon dioxide and that this atmosphere is responsible for severe global warming on the planet. However, we don't know if any of these volcanoes are still active, how much water was originally present, or if conditions were ever conducive to life.\u003c/p>\n\u003cp>Reading the stats on Venus got me thinking about the conditions on the other planets. Looking for the details, I came across a nice website dedicated to the solar system, \u003ca href=\"http://www.nineplanets.org/\" target=\"_blank\">www.nineplanets.org\u003c/a>. Although each planet has a very complex composition, I list here only the one or two most common gases in each planet's atmosphere. \u003ca href=\"http://www.nineplanets.org/mercury.html\" target=\"_blank\">Mercury\u003c/a>: essentially no atmosphere;\u003ca href=\"http://www.nineplanets.org/venus.html\" target=\"_blank\"> Venus\u003c/a>: almost 100 times pressure at Earth's surface, mostly carbon dioxide, very hot; \u003ca href=\"http://en.wikipedia.org/wiki/Earth's_atmosphere\" target=\"_blank\">Earth\u003c/a>: roughly 78% nitrogen and 21% oxygen, very little carbon dioxide; \u003ca href=\"http://www.nineplanets.org/mars.html\" target=\"_blank\">Mars\u003c/a>: Very thin, atmospheric pressure 100 times less than Earth, mostly carbon dioxide; \u003ca href=\"http://www.nineplanets.org/jupiter.html\" target=\"_blank\">Jupiter\u003c/a>: atmosphere indistinguishable from surface, 90% hydrogen and 10% helium; \u003ca href=\"http://www.nineplanets.org/saturn.html\" target=\"_blank\">Saturn\u003c/a>: 75% hydrogen, 25% helium; \u003ca href=\"http://www.nineplanets.org/uranus.html\" target=\"_blank\">Uranus\u003c/a>: 83% hydrogen, 15% helium; \u003ca href=\"http://www.nineplanets.org/neptune.html\" target=\"_blank\">Neptune\u003c/a>: mostly hydrogen and helium.\u003c/p>\n\u003cp>In reading over the description of the planetary atmospheres, you may notice some interesting trends. For one thing, the Earth definitely stands out with its atmosphere of nitrogen and oxygen. Maybe all of the life on Earth's surface is responsible? Maybe the water??\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\n\u003cp>You may also notice that the planets which are furthest from the sun are made up almost entirely of hydrogen and helium. In composition, the gaseous outer planets actually resemble the original nebula that gave birth to the solar system, a feature not shared with the inner rocky planets. Why did all of the hydrogen and helium disappear from the inner planets? For that matter, where is the atmosphere of Mercury?\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/icon_kdawson.jpg\">\u003c/span>\u003cem>\u003cstrong>Kyle S. Dawson\u003c/strong> is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at \u003ca href=\"http://www.lbl.gov/\" target=\"_blank\">Lawrence Berkeley National Laboratory\u003c/a>\u003c/em>.\u003cbr>\n\u003cbr clear=\"all\">\u003c/p>\n\u003cp>\u003c/p>\n\u003cp class=\"geo\"> latitude: \u003cspan class=\"latitude\">37.6797\u003c/span>, longitude: \u003cspan class=\"longitude\">-121.698\u003c/span>\u003c/p>\n\n",
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"description": "Credit: T. Credner & S. Kohle, AlltheSky.comYou may be surprised to hear that Venus is the warmest planet in the solar system. Venus has an average temperature of 850 degrees Fahrenheit. This is much warmer than the Earth, at 60 degrees, and even warmer than Mercury, which sits much closer to the sun, at 350",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/2007/12/starsflash_blog.jpg\">\u003cem>Credit: T. Credner & S. Kohle, AlltheSky.com\u003c/em>\u003c/span>You may be surprised to hear that \u003ca href=\"http://www.nasa.gov/worldbook/venus_worldbook.html\" target=\"_blank\">Venus\u003c/a> is the warmest planet in the solar system. Venus has an average temperature of 850 degrees Fahrenheit. This is much warmer than the \u003ca href=\"http://www.nasa.gov/worldbook/earth_worldbook.html\" target=\"_blank\">Earth\u003c/a>, at 60 degrees, and even warmer than \u003ca href=\"http://www.nasa.gov/worldbook/mercury_worldbook.html\" target=\"_blank\">Mercury\u003c/a>, which sits much closer to the sun, at 350 degrees. A reader asked if the high temperature on Venus was related to the composition of the atmosphere.\u003c/p>\n\u003cp>It turns out that the atmosphere of Venus is actually made almost entirely of carbon dioxide, and a lot of it. Because of this thick atmosphere and clouds of reflective sulfuric acid, not much was known about the planet's surface until recently. Before 1960, astronomers couldn't even estimate the length of one day on Venus! Now \u003ca href=\"http://en.wikipedia.org/wiki/Satellite\" target=\"_blank\">satellites\u003c/a>, like the \u003ca href=\"http://sci.esa.int/science-e/www/area/index.cfm?fareaid=64\" target=\"_blank\">Venus Express\u003c/a>, orbit around the planet and \u003ca href=\"http://en.wikipedia.org/wiki/Lander_%28spacecraft%29\" target=\"_blank\">landers\u003c/a>, like the \u003ca href=\"http://nssdc.gsfc.nasa.gov/planetary/venera.html\" target=\"_blank\">Soviet Venera\u003c/a>, have reached the surface.\u003c/p>\n\u003cp>We now know that the surface of Venus is scarred with impact craters, lava flows and more volcanoes than any other planet in the solar system. We know that the atmosphere is almost entirely carbon dioxide and that this atmosphere is responsible for severe global warming on the planet. However, we don't know if any of these volcanoes are still active, how much water was originally present, or if conditions were ever conducive to life.\u003c/p>\n\u003cp>Reading the stats on Venus got me thinking about the conditions on the other planets. Looking for the details, I came across a nice website dedicated to the solar system, \u003ca href=\"http://www.nineplanets.org/\" target=\"_blank\">www.nineplanets.org\u003c/a>. Although each planet has a very complex composition, I list here only the one or two most common gases in each planet's atmosphere. \u003ca href=\"http://www.nineplanets.org/mercury.html\" target=\"_blank\">Mercury\u003c/a>: essentially no atmosphere;\u003ca href=\"http://www.nineplanets.org/venus.html\" target=\"_blank\"> Venus\u003c/a>: almost 100 times pressure at Earth's surface, mostly carbon dioxide, very hot; \u003ca href=\"http://en.wikipedia.org/wiki/Earth's_atmosphere\" target=\"_blank\">Earth\u003c/a>: roughly 78% nitrogen and 21% oxygen, very little carbon dioxide; \u003ca href=\"http://www.nineplanets.org/mars.html\" target=\"_blank\">Mars\u003c/a>: Very thin, atmospheric pressure 100 times less than Earth, mostly carbon dioxide; \u003ca href=\"http://www.nineplanets.org/jupiter.html\" target=\"_blank\">Jupiter\u003c/a>: atmosphere indistinguishable from surface, 90% hydrogen and 10% helium; \u003ca href=\"http://www.nineplanets.org/saturn.html\" target=\"_blank\">Saturn\u003c/a>: 75% hydrogen, 25% helium; \u003ca href=\"http://www.nineplanets.org/uranus.html\" target=\"_blank\">Uranus\u003c/a>: 83% hydrogen, 15% helium; \u003ca href=\"http://www.nineplanets.org/neptune.html\" target=\"_blank\">Neptune\u003c/a>: mostly hydrogen and helium.\u003c/p>\n\u003cp>In reading over the description of the planetary atmospheres, you may notice some interesting trends. For one thing, the Earth definitely stands out with its atmosphere of nitrogen and oxygen. Maybe all of the life on Earth's surface is responsible? Maybe the water??\u003c/p>\n\u003cp>\u003c/p>\u003c/div>",
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"content": "\u003cdiv class=\"post-body\">\u003cp>\u003c/p>\n\u003cp>You may also notice that the planets which are furthest from the sun are made up almost entirely of hydrogen and helium. In composition, the gaseous outer planets actually resemble the original nebula that gave birth to the solar system, a feature not shared with the inner rocky planets. Why did all of the hydrogen and helium disappear from the inner planets? For that matter, where is the atmosphere of Mercury?\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/icon_kdawson.jpg\">\u003c/span>\u003cem>\u003cstrong>Kyle S. Dawson\u003c/strong> is engaged in post-doctorate studies of distant supernovae and development of a proposed space-based telescope at \u003ca href=\"http://www.lbl.gov/\" target=\"_blank\">Lawrence Berkeley National Laboratory\u003c/a>\u003c/em>.\u003cbr>\n\u003cbr clear=\"all\">\u003c/p>\n\u003cp>\u003c/p>\n\u003cp class=\"geo\"> latitude: \u003cspan class=\"latitude\">37.6797\u003c/span>, longitude: \u003cspan class=\"longitude\">-121.698\u003c/span>\u003c/p>\n\n\u003c/div>\u003c/p>",
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"content": "\u003cp>\u003cspan class=\"left\">\u003ca href=\"http://ww2.kqed.org/quest/audio/view/675\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/radio2-7_spill300.jpg\" alt=\"\">\u003c/a>\u003c/span>It has been nine days since a Chinese freighter hit the Bay Bridge spilling 58-thousand gallons of bunker fuel into the Bay. After a massive effort only 25 percent of the oil has been cleaned up. And experts say they may not be able to recover much more. As clean-up crews in hazmat suits scour the beaches, scientists say they'll be dealing with the aftermath of last week's oil spill for months, maybe even years. Why is it so hard to clean up oil? And what will happen to the thousands of gallons of spilled oil that can't be recovered?\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003ca href=\"http://ww2.kqed.org/quest/audio/view/675\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/images/radio_icon_light.gif\" alt=\"\">\u003c/a>You may \u003ca href=\"http://ww2.kqed.org/quest/audio/view/675\"> listen to the \"Cleaning Up Oil in the Bay\" radio report\u003c/a> online, as well as find additional links and resources.\u003c/span>\u003c/p>\n\u003cp>\u003cspan class=\"left\">\u003cimg src=\"http://ww2.kqed.org/quest/wp-content/uploads/sites/39/imp/icon_amys.jpg\" alt=\"\">\u003cem>\u003cstrong>Amy Standen\u003c/strong> is a Reporter for QUEST and \u003ca href=\"http://www.kqed.org/radio/\">Radio News\u003c/a> at KQED-FM.\u003c/em>\u003c/span>\u003c/p>\n\u003cp> \u003c/p>\n\u003cp class=\"geo\">latitude: \u003cspan class=\"latitude\">37.7631\u003c/span>, longitude: \u003cspan class=\"longitude\">-122.4093\u003c/span>\u003c/p>\n\u003cp>[ad fullwidth]\u003c/p>\u003cp>\u003c/p>\n",
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"info": "The MindShift podcast explores the innovations in education that are shaping how kids learn. Hosts Ki Sung and Katrina Schwartz introduce listeners to educators, researchers, parents and students who are developing effective ways to improve how kids learn. We cover topics like how fed-up administrators are developing surprising tactics to deal with classroom disruptions; how listening to podcasts are helping kids develop reading skills; the consequences of overparenting; and why interdisciplinary learning can engage students on all ends of the traditional achievement spectrum. This podcast is part of the MindShift education site, a division of KQED News. KQED is an NPR/PBS member station based in San Francisco. You can also visit the MindShift website for episodes and supplemental blog posts or tweet us \u003ca href=\"https://twitter.com/MindShiftKQED\">@MindShiftKQED\u003c/a> or visit us at \u003ca href=\"/mindshift\">MindShift.KQED.org\u003c/a>",
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