RSS feed source: Volcano Discovery.com--Global earthquake monitor

Date and TimeMag
DepthDistanceLocationDetailsMap Jan 14, 02:44 pm (GMT +6)

4.2

10 km23 km (14 mi) to the SE Indian Ocean, 289 km southwest of Meulaboh, Indonesia InfoFeb 22, 2023 01:22 am (GMT +6)

5.0

10 km80 km (49 mi) to the SW Indian Ocean, 444 km south of Banda Aceh, Indonesia 2 reportsInfoJul 5, 2022 12:37 pm (GMT +6)

4.5

10 km25 km (16 mi) to the E Indian Ocean, 260 km southwest of Meulaboh, Indonesia InfoMar 3, 2022 07:07 am (GMT +6)

4.4

10 km44 km (28 mi) to the NWOff the West Coast of Northern Sumatra InfoFeb 17, 2022 06:25 am (GMT +6)

4.0

10 km90 km (56 mi) to the NW Indian Ocean, 307 km southwest of Banda Aceh, Indonesia InfoApr 9, 2020 05:15 am (GMT +6)

5.2

92 km69 km (43 mi) to the SW Indian Ocean, 211 km southwest of Pulau Salaut-besar Island, Indonesia InfoApr 18, 2019 03:17 am (GMT +6)

5.2

30 km54 km (34 mi) to the E Indian Ocean, 337 km south of Banda Aceh, Indonesia InfoJan 6, 2016 11:46 am (GMT +6)

5.1

10 km91 km (56 mi) to the SE Indian Ocean, 194 km west of Sinabang, Indonesia InfoMay 18, 2014 04:59 pm (GMT +6)

5.5

4.8 km88 km (55 mi) to the NW Indian Ocean, 312 km southwest of Banda Aceh, Indonesia InfoApr 29, 2012 02:09 pm (GMT +6)

5.7

14 km42 km (26 mi) to the NE Indian Ocean, 329 km south of Banda Aceh, Indonesia InfoApr 27, 2012 01:21 am (GMT +6)

5.6

7.9 km37 km (23 mi) to the NE Indian Ocean, 331 km south of Banda Aceh, Indonesia InfoApr 20, 2012 11:14

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A new study supported by the U.S. National Science Foundation shows, for the first time, how heat moves — or rather, doesn’t — between materials in a high-energy-density plasma state. The work is expected to provide a better understanding of inertial confinement fusion experiments, which aim to reliably achieve fusion ignition on Earth using lasers. How heat flows between a hot plasma and a material’s surface is also important in other technologies, including semiconductor etching and vehicles that fly at hypersonic speeds.

High-energy-density plasmas are produced only at extreme pressures and temperatures. The study shows that interfacial thermal resistance, a phenomenon known to impede heat transfer in less extreme conditions, also prevents heat flow between different materials in a dense, super-hot plasma state. The research is published in Nature Communications and was led by Thomas White, a physicist at the University of Nevada, Reno, and his former doctoral student, Cameron Allen. White is a recipient of an NSF Faculty Early Career Development grant.

“Understanding how energy flows across a boundary is a fundamental question, and this work provides us with new insights into how this happens in the exceptionally energy-dense environments that one finds inside of stars and planetary cores,” says Jeremiah Williams, a program director for the NSF Plasma Physics program.