从0到1快速入门TL;DR文档快速总结应用场景

• Introduce 简介
• setting 设置
• Prompt 提示
• Sample response 回复样本
• API request 接口请求
• • python接口请求示例
  • node.js接口请求示例
  • curl命令示例
  • json格式示例
• 其它资料下载

ChatGPT是目前最先进的AI聊天机器人，它能够理解图片和文字，生成流畅和有趣的回答。如果你想跟上AI时代的潮流，你一定要学会使用ChatGPT。如果你想了解OpenAI最新发布的GPT-4模型，以及它如何为ChatGPT聊天机器人带来更强大的功能，那么你一定不要错过OpenAI官网推荐的48种最佳应用场景，不管你是资深开发者、初学者，你都能够从0到1快速入门，并掌握他们。

TL;DR即，Too Long; Didn’t Read “太长;“没读过”，用来总结一篇很长的文本或文章。它通常用于互联网上，当人们想快速了解一篇文章的内容而不需要阅读所有内容时。ChatGPT强大的语言快速处理能力，就能为您完成这个需求。它不仅可以帮助您节省时间和精力，还可以帮助您更好地理解文章的内容。

Introduce 简介

TL;DR summarization TL;DR总结
Summarize text by adding a ‘tl;dr:’ to the end of a text passage. It shows that the API understands how to perform a number of tasks with no instructions.
通过添加’tl;dr：“到一段文字的结尾。它表明API理解如何在没有指令的情况下执行大量任务。

setting 设置

Engine：text-davinci-003
Max tokens：60
Temperature：0.7
Top p：1.0
Frequency penalty：0.0
Presence penalty：1.0

Prompt 提示

Sample response 回复样本

API request 接口请求

python接口请求示例

import os
import openaiopenai.api_key = os.getenv("OPENAI_API_KEY")response = openai.Completion.create(model="text-davinci-003",prompt="A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich.[1] Neutron stars are the smallest and densest stellar objects, excluding black holes and hypothetical white holes, quark stars, and strange stars.[2] Neutron stars have a radius on the order of 10 kilometres (6.2 mi) and a mass of about 1.4 solar masses.[3] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei.\n\nTl;dr",temperature=0.7,max_tokens=60,top_p=1.0,frequency_penalty=0.0,presence_penalty=1
)

node.js接口请求示例

const { Configuration, OpenAIApi } = require("openai");const configuration = new Configuration({apiKey: process.env.OPENAI_API_KEY,
});
const openai = new OpenAIApi(configuration);const response = await openai.createCompletion({model: "text-davinci-003",prompt: "A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich.[1] Neutron stars are the smallest and densest stellar objects, excluding black holes and hypothetical white holes, quark stars, and strange stars.[2] Neutron stars have a radius on the order of 10 kilometres (6.2 mi) and a mass of about 1.4 solar masses.[3] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei.\n\nTl;dr",temperature: 0.7,max_tokens: 60,top_p: 1.0,frequency_penalty: 0.0,presence_penalty: 1,
});

curl命令示例

curl https://api.openai.com/v1/completions \-H "Content-Type: application/json" \-H "Authorization: Bearer $OPENAI_API_KEY" \-d '{"model": "text-davinci-003","prompt": "A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich.[1] Neutron stars are the smallest and densest stellar objects, excluding black holes and hypothetical white holes, quark stars, and strange stars.[2] Neutron stars have a radius on the order of 10 kilometres (6.2 mi) and a mass of about 1.4 solar masses.[3] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei.\n\nTl;dr","temperature": 0.7,"max_tokens": 60,"top_p": 1.0,"frequency_penalty": 0.0,"presence_penalty": 1
}'

json格式示例

{"model": "text-davinci-003","prompt": "A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich.[1] Neutron stars are the smallest and densest stellar objects, excluding black holes and hypothetical white holes, quark stars, and strange stars.[2] Neutron stars have a radius on the order of 10 kilometres (6.2 mi) and a mass of about 1.4 solar masses.[3] They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density to that of atomic nuclei.\n\nTl;dr","temperature": 0.7,"max_tokens": 60,"top_p": 1.0,"frequency_penalty": 0.0,"presence_penalty": 1
}

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