Expert-level radio astronomy covering radio telescopes, interferometry, VLBI, pulsars, spectral line observations, fast radio bursts, and aperture synthesis imaging.
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Single dish: large collecting area, resolution limited by diffraction. Parabolic reflector: focuses radio waves to receiver at prime or secondary focus. FAST: 500m dish in China, most sensitive single dish in the world. Receiver systems: LNA amplifiers, mixers, spectrometers, cryogenic cooling. System temperature: receiver noise plus sky background limits sensitivity.
Baseline: separation between two antennas, determines angular resolution. Visibility: complex number measured by each baseline, Fourier transform of sky. UV plane: spatial frequency coverage determines image quality. Aperture synthesis: Earth rotation fills UV plane over time. CLEAN algorithm: iterative deconvolution of dirty beam from dirty image.
Very long baseline interferometry: intercontinental baselines, microarcsecond resolution. Atomic clocks: GPS and hydrogen masers synchronize stations. EHT: global VLBI at 1.3mm imaged black hole shadows of M87 and Sgr A star. Space VLBI: RadioAstron satellite extended baselines beyond Earth diameter.
Pulsars: rotating neutron stars, stable rotation used as precise clocks. Pulsar timing arrays: gravitational wave background detection method. FRBs: fast radio bursts, millisecond transients, largely extragalactic origin. HI 21cm line: neutral hydrogen spin-flip transition traces galaxy structure. Molecular lines: CO, OH, NH3 probe cold gas in star-forming regions.
| Pitfall | Fix |
|---|---|
| RFI contamination | Flag affected data before imaging |
| Insufficient UV coverage | Observe at multiple hour angles or add more antennas |
| CLEAN divergence | Use appropriate CLEAN depth and mask region |
| Confusing flux density and luminosity | Always specify distance when quoting luminosity |
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概要と使いどころ
Expert-level abstract algebra knowledge. Use when working with groups, rings, fields, modules, Galois theory, representation theory, or algebraic structures. Also use when the user mentions 'group', 'ring', 'field', 'homomorphism', 'isomorphism', 'normal subgroup', 'quotient group', 'Sylow theorem', 'Galois theory', 'polynomial ring', 'ideal', 'module', 'vector space', or 'representation theory'.
日本語の概要は準備中です。原文の説明を表示しています。
Expert-level acoustics knowledge. Use when working with sound waves, acoustic propagation, resonance, standing waves, Doppler effect, room acoustics, ultrasound, noise control, musical acoustics, or architectural acoustics. Also use when the user mentions 'sound wave', 'decibel', 'frequency', 'resonance', 'standing wave', 'Doppler effect', 'acoustic impedance', 'reverberation', 'ultrasound', 'noise control', 'harmonics', or 'sound intensity'.
日本語の概要は準備中です。原文の説明を表示しています。
Expert-level aerodynamics covering subsonic and supersonic flow, lift and drag, airfoil theory, boundary layers, compressible flow, and CFD methods.
日本語の概要は準備中です。原文の説明を表示しています。
Expert-level air quality engineering covering pollutant sources, atmospheric dispersion, air quality standards, emission controls, and air quality modeling.
日本語の概要は準備中です。原文の説明を表示しています。
Expert-level aircraft structures covering structural design philosophy, wing and fuselage analysis, fatigue and damage tolerance, composite structures, and certification.
日本語の概要は準備中です。原文の説明を表示しています。
Expert-level algorithms and complexity theory covering sorting, searching, graph algorithms, dynamic programming, greedy algorithms, NP-completeness, and algorithm design paradigms.
日本語の概要は準備中です。原文の説明を表示しています。