{"id":19670,"date":"2026-06-18T16:40:43","date_gmt":"2026-06-18T08:40:43","guid":{"rendered":"https:\/\/www.es.ntnu.edu.tw\/?page_id=19670"},"modified":"2026-10-20T16:45:34","modified_gmt":"2026-10-20T08:45:34","slug":"academiclecture-115-1","status":"publish","type":"page","link":"https:\/\/www.es.ntnu.edu.tw\/index.php\/academiclecture-115-1\/","title":{"rendered":"\u5b78\u8853\u6f14\u8b1b 115-1"},"content":{"rendered":"\t\t
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\u5b78\u8853\u6f14\u8b1b Colloquium Schedule<\/h3>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t
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\u00a0\u4e00\u4e00\u4e94\u5b78\u5e74\u5ea6\u7b2c\u4e00\u5b78\u671f<\/p>

2026 Fall Semester<\/p>

Time: 02:20 pm every Tuesday<\/span><\/b><\/p>

Venue: Room S101<\/span><\/b>, 1F, Research Building<\/span><\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/10\/20 Dr. Yung-Hsin Liu (ASIES): The Early Solar System Evolution Inferred from Nucleosynthetic Isotope Anomalies in FUN Calcium-Aluminum-Rich Inclusions<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
Meteorites contain tiny remnants of dust grains that formed around earlier generations of stars that had survived the birth of the solar system. These presolar grains carry distinctive nucleosynthetic isotopic anomalies, which reflect their stellar origins. Although extensive mixing and processing in the protoplanetary disk largely homogenized these signatures, measurable anomalies are still preserved in meteorites and their components. These isotopic records provide important clues to the source materials of the solar system, the relationships among planetary bodies, and the transport and processing of matter in the early solar system.<\/div>
Calcium-aluminum-rich inclusions (CAIs) are the oldest known solids formed in the solar system. Condensed directly from hot gas near the proto-Sun, CAIs preserved a unique record of the chemical and isotopic environment that existed during the earliest stages of solar system formation. Their compositions were influenced by material inherited from multiple stellar sources, including supernovae that contributed short-lived radionuclides, such as 26 Al, neutron-rich isotopes, and r-process nuclides. A rare subgroup of CAIs, known as FUN (fractionation and unknown nuclear effects) CAIs, display unusual isotopic characteristics while sharing all the mineralogical and petrographic features as the \u201cnormal\u201d CAIs. Because FUN CAIs are extremely rare, their origin and significance remain poorly understood. In this study, we identified a new FUN CAI from the Allende CV3 chondrite using a laser-based Mg isotope analysis technique. By combining our results with previously published data, we find that many FUN CAIs show a unique characteristic of deficits in 26 Al and 30 Si, consistent with contributions from AGB stars. However, the supernovae related neutron-rich isotopes show either positive or negative anomalies. These observations support the idea that FUN CAIs represent a reservoir of stellar material inherited from the galaxy before the formation of our solar system, and subsequently isolated through thermal processing in the early protoplanetary disk. A key unresolved question is how FUN and normal CAIs are related and whether they formed in spatially distinct regions or at different times during the evolution of the early solar system.<\/div>
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Host: Yueh-Ning Lee<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/09\/22 2026 ESSSP Student Presentation II \u5730\u7403\u79d1\u5b78\u6691\u671f\u5b78\u751f\u5c08\u984c\u7814\u7a76\u8a08\u756b\u6210\u679c\u5831\u544a<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t

20min (incl. Q&A) per talk<\/b><\/p>

1.\u83ab\u62c9\u514b\u98b1\u98a8\u8207\u5b63\u5167\u9707\u76ea <\/strong><\/span>Typhoon Morakot and Intraseasonal Oscillations<\/b><\/p>

\u674e\u51a0\u5ef7<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb <\/span>LI, Kuan-Ting \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u66fe\u8389\u73ca\u6559\u6388<\/span> Prof. Li-Shan Tseng<\/p>

2. \u5730\u9707\u8207\u98b1\u98a8\u4f5c\u7528\u4e0b\u53f0\u5317 <\/span>101 \u5927\u6a13\u4e4b\u632f\u52d5\u8207\u6a21\u614b\u53cd\u61c9<\/span><\/strong> Vibration and Modal Responses of TAIPEI <\/b>101 to Earthquakes and Typhoons<\/b><\/p>

\u6c88\u5ead\u5b87<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb<\/span> SHEN, Ting-Yu \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u9673\u5349\u7444\u6559\u6388<\/span> Prof. Kate Hui-Hsuan Chen (\u53f0\u5e2b\u5927\u5730\u79d1\u7cfb <\/span>ES, NTNU)\u3001\u67ef\u4fca\u5b87\u6559\u6388<\/span> Prof. Chun-Yu Ke (\u53f0\u5927\u571f\u6728<\/span> CE, NTU)\u3001\u6797\u6b3d\u4ec1\u7814\u7a76\u6280\u5e2b <\/span>Dr. Chin-Jen Lin (\u4e2d\u7814\u9662\u5730\u79d1\u6240<\/span> IES, Academic Sinica)<\/p>

3. \u53f0\u5317 <\/span>101 \u5927\u6a13 <\/span>2022 \u5e74\u5168\u5e74\u632f\u52d5\u7279\u5fb5\uff1a\u74b0\u5883\u63a7\u5236\u8207\u6a21\u614b\u8b8a\u5316<\/span><\/strong> A Year of TAIPEI 101 Vibrations: <\/b>Environmental Controls and Modal Variations in 2022<\/b><\/p>

\u6c5f\u91c7\u9713<\/span> \/ \u967d\u660e\u4ea4\u5927\u767e\u5ddd\u5b78\u58eb\u5b78\u4f4d\u5b78\u7a0b<\/span> CHIANG, Tsai-Ni \/ Arete Honors Program, NYCU<\/p>

Supervisor<\/i>\uff1a \u9673\u5349\u7444\u6559\u6388<\/span> Prof. Kate Hui-Hsuan Chen (\u53f0\u5e2b\u5927\u5730\u79d1\u7cfb <\/span>ES, NTNU), \u67ef\u4fca\u5b87\u6559\u6388<\/span> Prof. Chun-Yu Ke (\u53f0\u5927\u571f\u6728<\/span> CE, NTU), \u6797\u6b3d\u4ec1\u7814\u7a76\u6280\u5e2b <\/span>Dr. Chin-Jen Lin (\u4e2d\u7814\u9662\u5730\u79d1\u6240<\/span> IES, Academic Sinica)<\/p>

4. \u53f0\u7063\u4e0a\u5347\u73ca\u745a\u53f0\u5730\u4e4b\u6c27\u540c\u4f4d\u7d20\u8207<\/span> Sr\/Ca \u53e4\u6c23\u5019\u5206\u6790\u7814\u7a76<\/span><\/strong> Oxygen Isotope and Sr\/Ca Analysis of <\/b>Uplifted Coral Terraces around Taiwan for Paleoclimate Reconstruction<\/b><\/p>

\u6f58\u6cd3\u5b87<\/span> \/ \u5e2b\u5927\u5730\u7406\u7cfb<\/span> PAN, Hong-Yu \/ NTNU Geography<\/p>

Supervisor<\/i>\uff1a \u8449\u5b5f\u5b9b\u6559\u6388\u3001\u7c73\u6cd3\u751f\u6559\u6388<\/span> Prof. Meng-Wan Yeh & Horng-Sheng Mii<\/p>

5. \u5927\u5c6f\u706b\u5c71\u4e5f\u6709\u9ed1\u66dc\u5ca9\uff1f\u713f\u5b50\u576a\u4f3c\u9ed1\u66dc\u5ca9\u5ca9\u77f3\u7814\u7a76<\/span><\/strong> Is obsidian present in the Tatun Volcano Group? <\/b>A study of obsidian-like rocks from Gengziping<\/b><\/p>

\u8a79\u5b87\u5d34<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb <\/span>JAN, Yu-Wei \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u8cf4\u6631\u9298\u6559\u6388<\/span> Prof. Yu-Ming Lai<\/p><\/div><\/div><\/div><\/div><\/div><\/div><\/div>

Host: Khushi<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/09\/08 2026 ESSSP Student Presentation I \u5730\u7403\u79d1\u5b78\u6691\u671f\u5b78\u751f\u5c08\u984c\u7814\u7a76\u8a08\u756b\u6210\u679c\u5831\u544a<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t

20min (incl. Q&A) per talk<\/b><\/p>

1.\u5927\u5c6f\u706b\u5c71\u7fa4\u84b8\u6c23\u5674\u767c\u7522\u7269\u4e4b\u7926\u7269\u5b78\u7814\u7a76<\/span><\/strong> Mineralogical study of phreatic eruption products from the <\/b>Tatun Volcano Group<\/b><\/p>

\u674e\u6046\u6bc5<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb<\/span> LEE, Harry Heng-Yi \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u8cf4\u6631\u9298\u6559\u6388 <\/span>Prof. Yu-Ming Lai<\/p>

2. \u7194\u7a4d\u5ca9\u7684\u7522\u72c0\u8207\u69cb\u9020\uff1a\u4ee5\u6d77\u5cb8\u5c71\u8108\u8207\u6f8e\u6e56\u70ba\u4f8b<\/strong><\/span> Occurrence and textures of peperites: examples <\/b>from the Coastal Range and Penghu Islands<\/b><\/p>

\u5468\u54f2\u5b87<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb <\/span>JHOU, Jhe-Yu \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u8cf4\u6631\u9298\u6559\u6388 <\/span>Prof. Yu-Ming Lai<\/p>

3. \u88c2\u9699\u788e\u5f62\u5e7e\u4f55\u5206\u6790\u53ca\u5176\u5c0d\u5ca9\u9ad4\u6ef2\u6d41\u7279\u6027\u4e4b\u610f\u6db5\u63a2\u8a0e<\/strong><\/span> Fractal Characterization of Rock Fracture <\/b>Networks and Its Implications for Permeability Anisotropy<\/b><\/p>

\u738b\u59ff\u8335<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb<\/span> WANG, Zi-Yin \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u8449\u6069\u8087\u6559\u6388<\/span> Prof. En-Chao Yeh<\/p>

4<\/strong>. \u73fe\u5730\u61c9\u529b\u975e\u5f48\u6027\u61c9\u8b8a\u56de\u5fa9\u6cd5\u4e4b\u7cbe\u5ea6\u5206\u6790\u8207\u6539\u9032<\/strong><\/span> Improvement of Anelastic Strain Recovery Method <\/b>for In-Situ Stress Assessment<\/b><\/p>

\u6d2a\u632f\u76ca<\/span> \/ \u5e2b\u5927\u5730\u79d1\u7cfb <\/span>ANG, Kim Joo \/ NTNUES<\/p>

Supervisor<\/i>\uff1a \u8449\u6069\u8087\u6559\u6388<\/span> Prof. En-Chao Yeh<\/p><\/div>

Host: Yu-Li Chen<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/09\/15 Charles University (Czech Republic) Visitors' Seminar<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
Prof. Vojt\u011bch Pato\u010dka<\/strong>: Reorientation of planets and more
Ond\u0159ej \u0160\u00e1dek<\/strong>: Ventilation of street canyons
V\u00edt Beran<\/strong>: Numerical modelling of a cooling magma chamber
J\u00e1chym \u0160ev\u010d\u00edk<\/strong>: ALADIN operative snow analysis & Microwave radiance data assimilation in ALADIN
Martin Hronek<\/strong>: Inverse dynamic rupture modeling of the 2016 Mw 6.1 Tottori earthquake
\u0160imon Barto\u0148<\/strong>: Instability of Internal Gravity Waves: Diagnosing the Transition to the Wave-Breaking Regime
Kl\u00e1ra Anna \u0160indlerov\u00e1<\/strong>: Topography of Saturn’s moon Enceladus as a record of thermal processes in the subsurface ocean<\/div>

Host: Wei-Ling Tseng\u00a0<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/09\/29 Prof. Jui-Lin Frank Li (NTU): How Falling-Ice Radiative Effects Shape Tropical Pacific Dynamics, ENSO, and Sea Level: A Satellite and Model-Based Assessment<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t

Falling ice particles \u2014 including ice crystals, snow, and other frozen hydrometeors \u2014 exert significant but long-underappreciated radiative effects on Earth’s energy budget. In contemporary general circulation models (GCMs), the treatment of ice-phase microphysics and their associated radiative properties remains a leading source of systematic bias, with downstream consequences for simulated tropical circulation, sea surface temperature (SST) variability, sea surface height (SSH) anomalies, and El Ni\u00f1o\u2013Southern Oscillation (ENSO). This talk synthesizes findings from a series of studies that used complementary satellite observations \u2014 including CloudSat, CALIPSO, MODIS, AIRS, Jason-1\/2, QuikSCAT, and CERES \u2014 alongside CMIP5 and CMIP6 multi-model ensembles to diagnose how falling ice radiative effects (FIRE) propagate through the coupled climate system. We demonstrate that FIRE warm the lower troposphere and cool the surface in the tropics, modulating surface wind stress, influence thermocline depth, and SSH anomalies in ways that bias the representation of Central-Pacific (CP) El Ni\u00f1o in models. We further show that CMIP3\/CMIP5\/CMIP6 models exhibit systematic shortwave and longwave radiation biases over tropical and subtropical oceans attributable to the parameterization of frozen hydrometeor optical properties, and that correcting or constraining these biases substantially alters projected Southern Ocean sea ice trajectories and CP-ENSO statistics under global warming. Taken together, these results highlight FIRE as a critical but underexplored physical mechanism linking cloud microphysics to large-scale ocean\u2013atmosphere variability, with implications for climate projection fidelity.<\/p>

\u00a0<\/div><\/div><\/div><\/div><\/div>

Host: Cheng-Ta Chen<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/10\/06 Prof. Chiung-Shen Johnson Ku (Department of Electrical Engineering, NTUT): Toward Indigenous SAR Capability in Taiwan: Polarimetric Simulation and X-Band UAV SAR Development<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t

Frequent cloud cover in Taiwan’s subtropical monsoon climate often limits optical remote sensing, while slope hazards, land subsidence, and maritime surveillance demand all-weather, day-and-night synthetic aperture radar (SAR) observation. SAR is an active microwave imaging system. Its range resolution is governed by signal bandwidth, and its azimuth resolution is determined by the synthetic aperture, independent of range. The retained phase further enables interferometric (InSAR), polarimetric (PolSAR), and tomographic (TomoSAR) applications. However, Taiwan’s first indigenous SAR mission, FORMOSAT-9, comprises two X-band active phased-array satellites (best resolution \u2264 1 m, maximum swath > 50 km), and its first launch is not scheduled until 2028, one year later than previously planned. Until then, domestic users remain reliant on foreign commercial SAR data.<\/p>

This talk begins with a review of SAR imaging geometry, resolution, and processing workflows, followed by a systematic overview of Taiwan\u2019s SAR research and development capabilities across industry, government, academia and domestic industry. The assessment indicates that domestic InSAR applications are internationally competitive, but it also identifies three structural gaps: (1) the absence of an indigenous data source before 2028; (2) the concentration of spaceborne payload integration in a single supplier, with transmit\/receive (T\/R) modules and GaN power amplifiers not yet space-qualified domestically; and (3) the lack of a shared validation infrastructure among the hardware, data, and algorithm communities. Accordingly, a three-phase roadmap toward indigenous capability is proposed, with the two FORMOSAT-9 launches as milestones. The first phase emphasizes pooled procurement of commercial data, calibration-site establishment, and airborne pathfinder validation. The second focuses on in-orbit calibration and a second payload supplier. The third targets a small SAR constellation and multi-baseline tomographic missions.<\/p>

Our group addresses these gaps from both the simulation and the system perspectives. On the simulation side, a GPU-accelerated, fully polarimetric shooting-and-bouncing-ray\/physical-optics (SBR\/PO) echo simulator has been developed. It models the polarimetric calibration chain using TerraSAR-X orbit and imaging geometry and incorporates a spherical-wave PO kernel for near-field airborne echoes. This enables imaging algorithms, radiometric calibration, and calibrator designs to be verified before measured data become available. On the system side, a dual-mode X-band (9.65 GHz) unmanned aerial vehicle (UAV) SAR has been designed for an operating altitude of 110 m. The High and Low modes use range bandwidths of 424 MHz and 212 MHz and provide ground swaths of approximately 100 m and 495 m, respectively. Under conservative assumptions, including an antenna efficiency of 0.4 and a system loss of 6 dB, the worst-case noise-equivalent sigma zero (NESZ) is \u221234.2 dB, exceeding the \u221230 dB requirement by about 4 dB. In the processing architecture, an RFSoC performs waveform generation, sampling, digital down-conversion, and range compression. An embedded system\u00a0 executes backprojection imaging, motion compensation, and phase gradient autofocus, with an estimated compute margin of 20\u201380\u00d7. Future work will complete hardware integration and conduct flight tests over a corner-reflector calibration site for cross-validation against simulation. Together, the simulator and the UAV SAR provide an airborne pathfinder for FORMOSAT-9 and help close the validation gap in Taiwan’s pursuit of indigenous SAR capability.<\/p>

Keywords:<\/strong> synthetic aperture radar (SAR); polarimetric simulation; SBR\/PO; UAV SAR; noise-equivalent sigma zero (NESZ); FORMOSAT-9<\/p><\/div>

Host: Yi-Jehng Kuan<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/10\/13 Prof. Yi-Leng Chen (University of Hawaii at M\u0101noa, Department of Atmospheric Sciences): Island-scale circulations over the Hawaiian Islands<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
\u00a0<\/div><\/div><\/div><\/div><\/div>

Host: Cheng-Ta Chen<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

\n\t\t\t\t\t
\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/10\/27 Prof. Pao-Shin Chu (University of Hawaii-Manoa): Impact of the El Nino-Southern Oscillation, the Pacific Meridional Mode, and the Pacific Decadal Oscillation on Hawaiian rainfall variability<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
\u00a0<\/div><\/div><\/div><\/div><\/div>

Host: Yong-Fu Lin<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/11\/03 Prof. Shih-Wei Fang (NCU): Past Climate and Cultural Impacts on Ancient Human Evolution<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
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Host: Cheng-Ta Chen<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/11\/10<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
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Host:\u00a0<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/11\/17 Dr. Chun-Yu Ke (NTU)<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
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Host: Kate Hui-Hsuen Chen<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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Host: Wei-Ling Tseng<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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Host: Yu-Ming-Lai<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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\n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/12\/08 Dr. Cheng-Hung Chen (ASIES)<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
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Host: Yu-Ming Lai<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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MSc student presentations \/\u00a0<\/span><\/b>\u78a9\u58eb\u73ed\u7814\u7a76\u751f\u5831\u544a<\/b>\u00a0(15min + 5min Q&A \/ talk)<\/span><\/b>\u00a0<\/span><\/b><\/div>
  1. \u674e\u627f\u6069 Li, Cheng-En<\/strong>: 2024\u5e74\u79cb\u5b63\u897f\u5317\u592a\u5e73\u6d0b\u516d\u500b\u98b1\u98a8\u4e4b\u767c\u5c55\u8207\u964d\u96e8\u5c0d\u4eba\u70ba\u6c23\u5019\u8b8a\u9077\u8a0a\u865f\u7684\u654f\u611f\u5ea6 Sensitivity of Typhoon Development and Rainfall to Anthropogenic Climate Change Signals: Six Western North Pacific Cases in Autumn 2024<\/li>
  2. \u9673\u548c\u9038 Chen\uff0cHo-Yi<\/strong>: 2022 \u5e74\u5c3c\u838e\u98b1\u98a8\u8207\u6771\u5317\u5b63\u98a8\u5171\u4f34\u964d\u96e8\u4e4b\u74b0\u5883\u5834\u4f4d\u79fb\u654f\u611f\u5ea6\u6a21\u64ec\u7814\u7a76 Sensitivity Simulation Study of Environmental Field Shifts in Typhoon Nesat\u2013Northeast Monsoon Interaction Rainfall in 2022<\/li>
  3. \u9ec3\u5049\u6d1b Wong Wai Lok<\/strong>: \u53f0\u7063\u590f\u5b63\u9ad8\u5c64\u51b7\u5fc3\u4f4e\u58d3\u8207\u5348\u5f8c\u5c0d\u6d41\u4e4b\u7279\u5fb5\u5206\u6790 Characteristics of Upper-Level Cold-Core Lows and Afternoon Convection over Taiwan during Summer<\/li><\/ol>
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    Host:\u00a0<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t

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    \n\t\t\t\t\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t<\/i><\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\t\t\t2026\/12\/22 Graduate Student Presentation II<\/a>\n\t\t\t\t\t<\/div>\n\t\t\t\t\t
    1. \u738b\u6615\u65c6 Wang, Hsin-Pei<\/strong>: \u5229\u7528\u5340\u57df\u6d77\u6d0b\u6a21\u5f0f\u6a21\u64ec\u6d77\u71d5\u98b1\u98a8\u66b4\u6f6e\uff1a\u9810\u5831\u80fd\u529b\u8207\u98b1\u98a8\u8def\u5f91\u8b8a\u5316\u4e4b\u5f71\u97ff Regional Ocean Modeling of Storm Surge during Super Typhoon Haiyan (2013): Predictability and Impacts of Track Variations<\/li>
    2. \u6797\u777f\u5bb8 Lin, Rui-chen<\/strong>: \u5c01\u9589\u5f0f\u5730\u6e90\u71b1\u6cf5\u7cfb\u7d71\u71b1\u3001\u6c34\u3001\u529b\u8026\u5408\u6548\u61c9\u4e4b\u7814\u7a76\uff1a\u71b1\u589e\u58d3\u8207\u4e95\u5b54\u5206\u96e2\u5c0d\u9577\u671f\u904b\u8f49\u7684\u5f71\u97ff Study on THM Coupling Effects in Closed-loop GSHP: Impacts of Thermal Pressurization and Borehole Decoupling on Long-term Operation<\/li>
    3. \u7ae5\u8b6f Tong, Yi<\/strong>: \u83f2\u5f8b\u8cd3\u5442\u5b8b\u5cf6\u6771\u5317\u90e8\u5361\u74dc\u706b\u5c71\u5ca9\u8c61\u5b78\u3001\u5730\u7403\u5316\u5b78\u8207\u5e74\u4ee3\u5b78 Petrology, Geochemistry, and Geochronology of Cagua Volcano, Northeastern Luzon Island<\/li><\/ol>
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      Host:\u00a0<\/p><\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t

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      \r\n Past Colloquium \u25be\r\n <\/div>\r\n\r\n \r\n
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      \r\n 114 \u5b78\u5e74\u5ea6 \u25be\r\n <\/div>\r\n \r\n
      \r\n 114-2<\/a>\r\n <\/div>\r\n <\/div>\r\n\r\n \r\n \r\n More\r\n <\/a>\r\n\r\n <\/div>\r\n<\/div>\r\n<\/div>\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t
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      \u5b78\u8853\u6f14\u8b1b Colloquium Schedule \u00a0\u4e00\u4e00\u4e94\u5b78\u5e74\u5ea6\u7b2c\u4e00\u5b78\u671f 2026 Fall Semester […]<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"ocean_front_end_style_editor":"no","ocean_post_layout":"","ocean_both_sidebars_style":"","ocean_both_sidebars_content_width":0,"ocean_both_sidebars_sidebars_width":0,"ocean_sidebar":"","ocean_second_sidebar":"","ocean_disable_margins":"enable","ocean_add_body_class":"","ocean_shortcode_before_top_bar":"","ocean_shortcode_after_top_bar":"","ocean_shortcode_before_header":"","ocean_shortcode_after_header":"","ocean_has_shortcode":"","ocean_shortcode_after_title":"","ocean_shortcode_before_footer_widgets":"","ocean_shortcode_after_footer_widgets":"","ocean_shortcode_before_footer_bottom":"","ocean_shortcode_after_footer_bottom":"","ocean_display_top_bar":"default","ocean_display_header":"default","ocean_header_style":"","ocean_center_header_left_menu":"","ocean_custom_header_template":"","ocean_custom_logo":0,"ocean_custom_retina_logo":0,"ocean_custom_logo_max_width":0,"ocean_custom_logo_tablet_max_width":0,"ocean_custom_logo_mobile_max_width":0,"ocean_custom_logo_max_height":0,"ocean_custom_logo_tablet_max_height":0,"ocean_custom_logo_mobile_max_height":0,"ocean_header_custom_menu":"","ocean_menu_typo_font_family":"","ocean_menu_typo_font_subset":"","ocean_menu_typo_font_size":0,"ocean_menu_typo_font_size_tablet":0,"ocean_menu_typo_font_size_mobile":0,"ocean_menu_typo_font_size_unit":"px","ocean_menu_typo_font_weight":"","ocean_menu_typo_font_weight_tablet":"","ocean_menu_typo_font_weight_mobile":"","ocean_menu_typo_transform":"","ocean_menu_typo_transform_tablet":"","ocean_menu_typo_transform_mobile":"","ocean_menu_typo_line_height":0,"ocean_menu_typo_line_height_tablet":0,"ocean_menu_typo_line_height_mobile":0,"ocean_menu_typo_line_height_unit":"","ocean_menu_typo_spacing":0,"ocean_menu_typo_spacing_tablet":0,"ocean_menu_typo_spacing_mobile":0,"ocean_menu_typo_spacing_unit":"","ocean_menu_link_color":"","ocean_menu_link_color_hover":"","ocean_menu_link_color_active":"","ocean_menu_link_background":"","ocean_menu_link_hover_background":"","ocean_menu_link_active_background":"","ocean_menu_social_links_bg":"","ocean_menu_social_hover_links_bg":"","ocean_menu_social_links_color":"","ocean_menu_social_hover_links_color":"","ocean_disable_title":"default","ocean_disable_heading":"default","ocean_post_title":"","ocean_post_subheading":"","ocean_post_title_style":"","ocean_post_title_background_color":"","ocean_post_title_background":0,"ocean_post_title_bg_image_position":"","ocean_post_title_bg_image_attachment":"","ocean_post_title_bg_image_repeat":"","ocean_post_title_bg_image_size":"","ocean_post_title_height":0,"ocean_post_title_bg_overlay":0.5,"ocean_post_title_bg_overlay_color":"","ocean_disable_breadcrumbs":"default","ocean_breadcrumbs_color":"","ocean_breadcrumbs_separator_color":"","ocean_breadcrumbs_links_color":"","ocean_breadcrumbs_links_hover_color":"","ocean_display_footer_widgets":"default","ocean_display_footer_bottom":"default","ocean_custom_footer_template":"","footnotes":""},"class_list":["post-19670","page","type-page","status-publish","hentry","entry"],"_links":{"self":[{"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/pages\/19670","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/comments?post=19670"}],"version-history":[{"count":125,"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/pages\/19670\/revisions"}],"predecessor-version":[{"id":20831,"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/pages\/19670\/revisions\/20831"}],"wp:attachment":[{"href":"https:\/\/www.es.ntnu.edu.tw\/index.php\/wp-json\/wp\/v2\/media?parent=19670"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}