This graduate-level course is really about how we *see* matter below the wavelength of visible light — the physics that sets resolution limits in each imaging modality, and the tricks (near-field probes, electron beams, superresolution fluorescence) used to push past them. You'll work through the optics math (Fourier imaging, PSFs, contrast transfer), study the mechanics of SPM and electron columns, and get hands-on lab time across AFM, STM, SEM, TEM, and confocal setups, with two open-book midterms, an open-book final, and weekly homework. It's a foundational methods course for MSN research — once you understand what each instrument actually measures and where it lies, you can read characterization sections of nanotech papers critically and pick the right tool for your own thesis work.
→ STARS müfredatı (resmi syllabus)
İlk dosyayı sen atarsan — not, slayt, geçmiş sınav, çözüm, cheat-sheet, ne varsa — defter ekibi öğrenci paylaşımlarından bu dersin notlarını yazar. Drive linki / PDF / ZIP, hepsi olur.
| Dönem | Course CPA | |
|---|---|---|
| 2025-2026 Fall | 3.33 | 1 sec · 6 öğr |
| 2024-2025 Spring | 3.18 | 1 sec · 13 öğr |
| 2023-2024 Spring | 3.22 | 1 sec · 13 öğr |
| 2022-2023 Spring | 3.50 | 1 sec · 9 öğr |
| 2021-2022 Spring | 3.33 | 1 sec · 12 öğr |
| 2020-2021 Spring | 3.18 | 1 sec · 13 öğr |
| 2019-2020 Spring | 3.27 | 1 sec · 17 öğr |
| 2018-2019 Spring | 3.15 | 1 sec · 13 öğr |
| 2017-2018 Spring | 3.29 | 1 sec · 11 öğr |
| 2015-2016 Spring | 3.69 | 1 sec · 27 öğr |
Aggregate course GPA — Bilkent STARS'tan public data. Hoca-bazlı per-section detayı için STARS evaluation report →. Öğrenci anket cevapları KVKK kapsamında defter'de tutulmaz.
75 percent attendance and having taken the midterm exams are required to take the final exam