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1 Primary & Middle School Mathematics1–9 年级在线 2 High School Mathematics10–12 年级在线 3 University Mathematics — Year 1本科一年级在线 4 University Mathematics — Year 2本科二年级在线 5 University Mathematics — Year 3本科三年级在线

1 Primary & Middle School Physics1–9 年级在线 2 High School Physics10–12 年级在线 3 University Physics — Year 1本科一年级在线 4 University Physics — Year 2本科二年级在线 5 University Physics — Year 3本科三年级在线

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1 Markets I: The Ecosystem and Exchange-Traded Markets市场在线 2 Markets II: Rates, FX and Credit市场在线 3 Markets III: Commodities, Energy and Crypto市场在线 4 Quantitative Methods方法在线 5 Derivatives and Volatility衍生品在线 6 Rates, Credit, XVA and Risk利率、信用与风险在线 7 Research Craft: Predictors, Backtests, Measurement, Portfolios研究在线 8 Strategies I: Equities and Futures策略在线 9 Strategies II: Volatility, Relative Value, Macro and the Bank Desks策略在线 10 Microstructure and Execution交易执行在线 11 Market Making and High-Frequency Trading做市在线 12 Machine Learning for Markets机器学习在线 13 Low-Latency Software技术在线 14 Networks, Hardware and Trading Infrastructure技术在线 15 Research, Data and Risk Platforms技术在线 16 The Desk and the Firm公司运营在线 17 The Industry: Firms, Roles and Careers职业发展在线 18 Interviews I: Maths, Probability and Speed职业发展在线 19 Interviews II: Markets, Trading Games and the Final Round职业发展在线 20 Interviews III: Code职业发展在线

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Physics · 术语表

什么是 Continuous spectrum？

Definition 2.5 High School Physics · 第 2 章 — Light Spectra and the Message of Light

Dense, hot matter — the filament of a bulb, molten steel, the surface of a star — glows, and its light contains every wavelength over a wide range: an unbroken band of color with nothing missing. Such a spectrum is a continuous spectrum. It carries no trace of the chemical nature of the body: a white-hot iron bar and a white-hot copper bar glow alike. What it does encode — entirely — is the temperature.

示例

Example 2.9 (Taking the Sun’s temperature)

The Sun’s continuous spectrum is most intense near $\lambda_{\max} = 500\,\mathrm{nm}$ . Wien’s law gives its surface temperature:

T = \frac{2.90 \times 10^{-3}\,\mathrm{m}\,\mathrm{K}}{5.00 \times 10^{-7}\,\mathrm{m}} = 5800\,\mathrm{K},

about $5500{}^{\circ}\mathrm{C}$ — measured from $150$ million kilometers away, with a prism and a division.

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