學術演講 Colloquium Schedule

 一一五學年度第一學期

2026 Fall Semester

Time: 02:20 pm every Tuesday

Venue: Room S101, 1F, Research Building

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 ≤ 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.

This talk begins with a review of SAR imaging geometry, resolution, and processing workflows, followed by a systematic overview of Taiwan’s 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.

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 −34.2 dB, exceeding the −30 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  executes backprojection imaging, motion compensation, and phase gradient autofocus, with an estimated compute margin of 20–80×. 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.

Keywords: synthetic aperture radar (SAR); polarimetric simulation; SBR/PO; UAV SAR; noise-equivalent sigma zero (NESZ); FORMOSAT-9

Host: Yi-Jehng Kuan

20min (incl. Q&A) per talk

1.莫拉克颱風與季內震盪 Typhoon Morakot and Intraseasonal Oscillations

李冠廷 / 師大地科系 LI, Kuan-Ting / NTNUES

Supervisor: 曾莉珊教授 Prof. Li-Shan Tseng

2. 地震與颱風作用下台北 101 大樓之振動與模態反應 Vibration and Modal Responses of TAIPEI 101 to Earthquakes and Typhoons

沈庭宇 / 師大地科系 SHEN, Ting-Yu / NTNUES

Supervisor: 陳卉瑄教授 Prof. Kate Hui-Hsuan Chen (台師大地科系 ES, NTNU)、柯俊宇教授 Prof. Chun-Yu Ke (台大土木 CE, NTU)、林欽仁研究技師 Dr. Chin-Jen Lin (中研院地科所 IES, Academic Sinica)

3. 台北 101 大樓 2022 年全年振動特徵:環境控制與模態變化 A Year of TAIPEI 101 Vibrations: Environmental Controls and Modal Variations in 2022

江采霓 / 陽明交大百川學士學位學程 CHIANG, Tsai-Ni / Arete Honors Program, NYCU

Supervisor: 陳卉瑄教授 Prof. Kate Hui-Hsuan Chen (台師大地科系 ES, NTNU), 柯俊宇教授 Prof. Chun-Yu Ke (台大土木 CE, NTU), 林欽仁研究技師 Dr. Chin-Jen Lin (中研院地科所 IES, Academic Sinica)

4. 台灣上升珊瑚台地之氧同位素與 Sr/Ca 古氣候分析研究 Oxygen Isotope and Sr/Ca Analysis of Uplifted Coral Terraces around Taiwan for Paleoclimate Reconstruction

潘泓宇 / 師大地理系 PAN, Hong-Yu / NTNU Geography

Supervisor: 葉孟宛教授、米泓生教授 Prof. Meng-Wan Yeh & Horng-Sheng Mii

5. 大屯火山也有黑曜岩?焿子坪似黑曜岩岩石研究 Is obsidian present in the Tatun Volcano Group? A study of obsidian-like rocks from Gengziping

詹宇崴 / 師大地科系 JAN, Yu-Wei / NTNUES

Supervisor: 賴昱銘教授 Prof. Yu-Ming Lai

Host: Khushi

20min (incl. Q&A) per talk

1.大屯火山群蒸氣噴發產物之礦物學研究 Mineralogical study of phreatic eruption products from the Tatun Volcano Group

李恆毅 / 師大地科系 LEE, Harry Heng-Yi / NTNUES

Supervisor: 賴昱銘教授 Prof. Yu-Ming Lai

2. 熔積岩的產狀與構造:以海岸山脈與澎湖為例 Occurrence and textures of peperites: examples from the Coastal Range and Penghu Islands

周哲宇 / 師大地科系 JHOU, Jhe-Yu / NTNUES

Supervisor: 賴昱銘教授 Prof. Yu-Ming Lai

3. 裂隙碎形幾何分析及其對岩體滲流特性之意涵探討 Fractal Characterization of Rock Fracture Networks and Its Implications for Permeability Anisotropy

王姿茵 / 師大地科系 WANG, Zi-Yin / NTNUES

Supervisor: 葉恩肇教授 Prof. En-Chao Yeh

4. 現地應力非彈性應變回復法之精度分析與改進 Improvement of Anelastic Strain Recovery Method for In-Situ Stress Assessment

洪振益 / 師大地科系 ANG, Kim Joo / NTNUES

Supervisor: 葉恩肇教授 Prof. En-Chao Yeh

Host: Yu-Li Chen

Prof. Vojtěch Patočka: Reorientation of planets and more
Ondřej Šádek: Ventilation of street canyons
Vít Beran: Numerical modelling of a cooling magma chamber
Jáchym Ševčík: ALADIN operative snow analysis & Microwave radiance data assimilation in ALADIN
Martin Hronek: Inverse dynamic rupture modeling of the 2016 Mw 6.1 Tottori earthquake
Šimon Bartoň: Instability of Internal Gravity Waves: Diagnosing the Transition to the Wave-Breaking Regime
Klára Anna Šindlerová: Topography of Saturn’s moon Enceladus as a record of thermal processes in the subsurface ocean

Host: Wei-Ling Tseng 

Falling ice particles — including ice crystals, snow, and other frozen hydrometeors — 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 Niño–Southern Oscillation (ENSO). This talk synthesizes findings from a series of studies that used complementary satellite observations — including CloudSat, CALIPSO, MODIS, AIRS, Jason-1/2, QuikSCAT, and CERES — 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 Niño 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–atmosphere variability, with implications for climate projection fidelity.

 

Host: Cheng-Ta Chen

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.
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 “normal” 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.
 

Host: Yueh-Ning Lee

 
 

Host: Yong-Fu Lin

 
 

Host: 

 
 

Host: Kate Hui-Hsuen Chen

 
 

Host: Yu-Ming-Lai