全力響應勞動部「防疫照顧假」
樂天市場開放同仁全薪居家辦公 兼具高效數位化工作品質與彈性
為配合中小學因防疫而延後開學,勞動部於2月3日公布特別措施「防疫照顧假」 ─ 凡2月11日至2月24日期間內,若有需照顧12歲以下學童之需求的家長,其中1人得向雇主申請「防疫照顧假」,此假是基於防疫需求而生的特別措施,不可歸責於勞工,因此雇主應予準假,且不可強迫請事假,亦不能據以扣全勤獎金或予以不利之處分,更不能作為解僱事由。
消息公布後,各知名國內外企業紛紛推出措施響應政令,台灣樂天市場亦宣布全力支持防疫行動,更早在1月31日,即針對曾與中國大陸籍親友共同居住、或身體不適,符合主管機關居家隔離條件的同仁,開放申請「居家工作」並提供全薪,只需備妥公司筆電並透過VPN連線,即可以居家辦公及進行全球各地的視訊會議。同時,關於「防疫照顧假」,樂天市場全力配合政府政策,凡有需要照顧12歲以下學童的家長皆可申請居家工作,同樣支付全薪。此外,由於樂天市場已將作業流程數位化,居家工作的同仁能擁有幾乎與辦公室一致的工作品質,同時可兼顧孩童家庭照顧,提升效率,也保有調度彈性。
台灣樂天市場人資部部長范君儀提到:「自從公司1月31日開放彈性在家上班到現在不滿一週,約一成符合條件的同仁申請彈性居家上班,來自基層同仁與主管的反應正面良好;台灣樂天市場全力支持政府的防疫措施,內部執行也以便利員工為主,兼顧勞雇雙方需求與彈性。」
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我也要這樣 安頓 處境時這樣吃吃吃 洪凱駖藥師~ Solving a long-standing mystery about the desert’s rock art canvas Petroglyphs are carved in a material called rock varnish, the origins of which have been debated for years. Now, scientists argue it’s the result of bacteria and an adaptation that protects them from the desert sun’s harsh rays. By Nathan Collins 5923141600_1bc3f25867_k.jpg Rock art featuring human and animal forms and handprints Petroglyphs at Mesa Verde National Park, Colorado (Christine Fry & Peter Russo) Wander around a desert most anywhere in the world, and eventually you’ll notice dark-stained rocks, especially where the sun shines most brightly and water trickles down or dew gathers. In some spots, if you’re lucky, you might stumble upon ancient art – petroglyphs – carved into the stain. For years, however, researchers have understood more about the petroglyphs than the mysterious dark stain, called rock varnish, in which they were drawn. In particular, science has yet to come to a conclusion about where rock varnish, which is unusually rich in manganese, comes from. Now, scientists at the California Institute of Technology, the Department of Energy’s SLAC National Accelerator Laboratory and elsewhere think they have an answer. According to a recent paper in Proceedings of the National Academy of Sciences, rock varnish is left behind by microbial communities that use manganese to defend against the punishing desert sun. The mystery of rock varnish is old, said Usha Lingappa, a graduate student at Caltech and the study’s lead author. “Charles Darwin wrote about it, Alexander von Humboldt wrote about it,” she said, and there is a long-standing debate about whether it has a biological or inorganic origin. But, Lingappa said, she and her colleagues didn’t actually set out to understand where rock varnish comes from. Instead, they were interested in how microbial ecosystems in the desert interact with rock varnish. To do so, they deployed as many techniques as they could come up with: DNA sequencing, mineralogical analyses, electron microscopy, and – aided by Stanford Synchroton Radiation Lightsource (SSRL) scientist Samuel Webb – advanced X-ray spectroscopy methods that could map different kinds of manganese and other elements within samples of rock varnish. “By combining these different perspectives, maybe we could draw a picture of this ecosystem and understand it in new ways,” Lingappa said. “That’s where we started, and then we just stumbled into this hypothesis” for rock varnish formation. Among the team’s key observations was that, while manganese in desert dust is usually in particle form, it was deposited in more continuous layers in varnish, a fact revealed by X-ray spectroscopy methods at SSRL that can tell not only what chemical compounds make up a sample but also how they are distributed, on a microscopic scale, throughout the sample. That same analysis showed that the kinds of manganese compounds in varnish were the result of ongoing chemical cycles, rather than being left out in the sun for millennia. That information, combined with the prevalence of bacteria called Chroococcidiopsis that use manganese to combat the oxidative effects of the harsh desert sun, led Lingappa and her team to conclude that rock varnish was left behind by those bacteria. For his part, Webb said that he always enjoys a manganese project – “I’ve been a mangaphile for a while now” – and that this project arrived at the perfect time, given advances in X-ray spectroscopy at SSRL. Improvements in X-ray beam size allowed the researchers to get a finer-grained picture of rock varnish, he said, and other improvements ensured that they could get a good look at their samples without the risk of damaging them. “We’re always tinkering and fine-tuning things, and I think it was the right time for a project that maybe 5 or 10 years ago wouldn’t really have been feasible.” The research was supported by the National Science Foundation, the National Institutes of Health and the National Aeronautics and Space Administration. SSRL is a DOE Office of Science user facility. Citation: Usha F. Lingappa et al., Proceedings of the National Academy of Sciences, 22 June 2021 (10.1073/pnas.2025188118) For questions or comments, contact the SLAC Office of Communications at communications@slac.stanford.edu. SLAC is a vibrant multiprogram laboratory that explores how the universe works at the biggest, smallest and fastest scales and invents powerful tools used by scientists around the globe. With research spanning particle physics, astrophysics and cosmology, materials, chemistry, bio- and energy sciences and scientific computing, we help solve real-world problems and advance the interests of the nation. SLAC is operated by Stanford University for the U.S. Department of Energy’s Office of Science. The Office of Science is the single largest supporter of basic research in the physical sciences in the United States and is working to address some of the most pressing challenges of our time. X-ray Science X-ray Spectroscopy Stanford Synchrotron Radiation Lightsource (SSRL)