llama2-7b-instruction-gen

Alpaca style Instruction generating

This model is used for creating the instructions, which we can then use to fine-tune the base model of Llama 2 to follow our instructions.

Prompt：

Use the Input below to create an instruction, which could have been used to generate the input using an LLM. 根据下面的文本输入生成一个指令，可以用来让大言语模型根据这条指令生成这段文本。

Examples：

1.

Input：监督学习是一种机器学习类型，其中标记过的数据用于创建可以对未标记数据进行预测的模型。在监督学习中，训练数据集由已经用正确的输出或目标值标记的数据组成。然后算法从这些标记数据中学习，并能够在新的、之前未见过的数据上做出预测。监督学习通常在图像识别，自然语言处理以及大多数机器学习任务中使用。

Response：解释什么是监督式机器学习

2.

Input：I see a lot of folks saying that minimum wage jobs are just intended for students. I wonder who they think makes their egg McMuffin at 8am or their chicken McNuggets at lunch? Folks who work a full-time job should be able to afford housing and food. It’s not that hard.

Response：回复以下评论，用不超过100个单词。 " Minimum wages are just for students."

3.

Input：Get ready for an anonymous cross-chain bridge coming to #MaxxChain courtesy of @BlockBlendIO! Transact with over 10 of the most prominent cryptocurrencies and receive #PWR through a single, untraceable transaction. Experience true DeFi freedom. Deployment slated for next week.

Response：发布一条推文，宣传新的加密货币桥。

4.

Input： Radial substructures have now been observed in a wide range of protoplanetary discs (PPDs), from young to old systems, however their formation is still an area of vigorous debate. Recent magnetohydrodynamic (MHD) simulations have shown that rings and gaps can form naturally in PPDs when non-ideal MHD effects are included. However these simulations employ ad-hoc approximations to the magnitudes of the magnetic diffusivities in order to facilitate ring growth. We replace the parametrisation of these terms with a simple chemical network and grain distribution model to calculate the non-ideal effects in a more self-consistent way. We use a range of grain distributions to simulate grain formation for different disc conditions. Including ambipolar diffusion, we find that large grain populations (> 1{\mu}m), and those including a population of very small polyaromatic hydrocarbons (PAHs) facilitate the growth of periodic, stable rings, while intermediate sized grains suppress ring formation. Including Ohmic diffusion removes the positive influence of PAHs, with only large grain populations still producing periodic ring and gap structures. These results relate closely to the degree of coupling between the magnetic field and the neutral disc material, quantified by the non-dimensional Elsasser number {\Lambda} (the ratio of magnetic forces to Coriolis force). For both the ambipolar-only and ambipolar-ohmic cases, if the total Elsasser number is initially of order unity along the disc mid-plane, ring and gap structures may develop.

Response：创建一篇关于行星盘中辐射结构的研究论文。