diff --git a/.gitignore b/.gitignore index d1a9611..71fb614 100644 --- a/.gitignore +++ b/.gitignore @@ -1,29 +1,11 @@ -data/ -*.zen* -*.zenml -*.venv - - -private.env -*.pyc - -*.las -*.log -mlruns/ -mlflow.db - +*.venv* # Ignore specific environment files with secrets (.env is tracked with generic values) .devcontainer/.env .env* .copilot/ -*.zip - -# allow .env files in tests/ directories -!tests/**/.env* -!integration/**/.env* -!integration-tests/**/.env* - # Ignore Jupyter Notebook checkpoints -.ipynb_checkpoints/ \ No newline at end of file +.ipynb_checkpoints/ + +# __marimo__ \ No newline at end of file diff --git a/README.md b/README.md index b66b116..3da1d61 100644 --- a/README.md +++ b/README.md @@ -12,4 +12,9 @@ uv sync ```bash uv run marimo edit -``` \ No newline at end of file +``` + + +3. Save + Commit changes: + +Clos \ No newline at end of file diff --git a/__marimo__/session/VB_interviews_sandbox.py.json b/__marimo__/session/VB_interviews_sandbox.py.json deleted file mode 100644 index c7be9f3..0000000 --- a/__marimo__/session/VB_interviews_sandbox.py.json +++ /dev/null @@ -1,151 +0,0 @@ -{ - "version": "1", - "metadata": { - "marimo_version": "0.18.0" - }, - "cells": [ - { - "id": "AKra", - "code_hash": "1d0db38904205bec4d6f6f6a1f6cec3e", - "outputs": [ - { - "type": "data", - "data": { - "text/plain": "" - } - } - ], - "console": [] - }, - { - "id": "Hbol", - "code_hash": "d19d3437ab7e3f0171ea5eff9e1d0e12", - "outputs": [ - { - "type": "data", - "data": { - "text/plain": "" - } - } - ], - "console": [] - }, - { - "id": "GTQs", - "code_hash": "b2194e2e2f1bd697d641f1528cd29572", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "

Ollama Reference

\n

Ollama Web-UI: http://ollama-vb.tail44fa00.ts.net:3000

\nUse the UI to modify system prompts, custom models, etc...\n

Ollama Python

\nDocs: https://github.com/ollama/ollama-python\nUse the code below to programmatically interact with the models. E.g: create a small pipeline that loads a transcript and inserts it into the prompt. Helpful if we need to analyze 26 interviews...\nImportant Definitions:\n" - } - } - ], - "console": [] - }, - { - "id": "djDz", - "code_hash": "585f27cf56a471ec61aadf0913f6b2df", - "outputs": [ - { - "type": "data", - "data": { - "application/json": "[\"text/plain:model='deepseek-r1:32b-qwen-distill-q4_K_M' modified_at=datetime.datetime(2025, 11, 12, 20, 50, 50, 790607, tzinfo=TzInfo(0)) digest='edba8017331d15236e57480eb45406c0d721db77a4cdcf234df500fc2ad3960c' size=19851337809 details=ModelDetails(parent_model='', format='gguf', family='qwen2', families=['qwen2'], parameter_size='32.8B', quantization_level='Q4_K_M')\", \"text/plain:model='deepseek-r1:7b' modified_at=datetime.datetime(2025, 11, 12, 19, 43, 34, 449734, tzinfo=TzInfo(0)) digest='755ced02ce7befdb13b7ca74e1e4d08cddba4986afdb63a480f2c93d3140383f' size=4683075440 details=ModelDetails(parent_model='', format='gguf', family='qwen2', families=['qwen2'], parameter_size='7.6B', quantization_level='Q4_K_M')\"]" - } - } - ], - "console": [] - }, - { - "id": "oAuP", - "code_hash": "795fbe6629dfda7b3960fd48629439b7", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "

Sandbox Generate vs. Chat

" - } - } - ], - "console": [] - }, - { - "id": "zDBa", - "code_hash": "58afd2f3adf26cfb1dd38c7147318cee", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "

Chat

" - } - } - ], - "console": [] - }, - { - "id": "XdJn", - "code_hash": "3d0bcd5259dca1dd926cbfae6cacca6e", - "outputs": [ - { - "type": "data", - "data": { - "text/plain": "" - } - } - ], - "console": [] - }, - { - "id": "Jonk", - "code_hash": "43cb7d2f5707f6730908e4b19e972c16", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "The sky appears blue primarily due to a phenomenon known as Rayleigh scattering. Here's a step-by-step explanation:\n
    \n
  1. Light Composition: White light from the sun is composed of various colors, each corresponding to different wavelengths. Blue light has a shorter wavelength compared to red or orange.
    2. \n
  2. Atmospheric Interaction: As sunlight travels through Earth's atmosphere, it interacts with molecules and small particles (like water droplets in clouds). These interactions depend on the wavelength of the light.
    3. \n
  3. Scattering Mechanism: Smaller particles scatter light more effectively at shorter wavelengths than longer ones. This means blue light, with its shorter wavelength, is scattered more frequently by atmospheric gases like nitrogen and oxygen.
    4. \n
  4. Sky Color During the Day: During the day, when sunlight passes through a clear atmosphere overhead, blue light scatters uniformly in all directions. Our eyes perceive this scattered blue light as making the sky appear blue.
    5. \n
  5. Sunrise and Sunset: At these times, sunlight has to travel through a longer path of Earth's atmosphere. Longer wavelengths (like red and orange) are scattered out more effectively, leaving the redder colors visible during sunrise and sunset.
    6. \n
  6. Perception of Other Colors: Our eyes are more sensitive to blue and green light, which can amplify their presence even if they're not the most scattered. Additionally, atmospheric conditions like pollution or high altitude (which reduces scattering) can affect color perception.
    7. \n
  7. Atmospheric Density: In clearer atmospheres (e.g., at high altitudes), Rayleigh scattering is more pronounced for shorter wavelengths, keeping the sky blue even when looking through less atmosphere.
    8. \n
\nIn summary, the sky appears blue due to the scattering of shorter blue wavelengths by Earth's atmosphere, with other colors appearing during different times and conditions influenced by atmospheric density and light path length." - } - } - ], - "console": [] - }, - { - "id": "nhwf", - "code_hash": "8e002c6404579303afb3301e4db34a23", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "

Generate

" - } - } - ], - "console": [] - }, - { - "id": "DEGe", - "code_hash": "66676a30e32437a882c6b17859bd31aa", - "outputs": [ - { - "type": "data", - "data": { - "text/plain": "" - } - } - ], - "console": [] - }, - { - "id": "pSOw", - "code_hash": "23f528f8711dc173fa4f72f32677a2e8", - "outputs": [ - { - "type": "data", - "data": { - "text/markdown": "The sky appears blue primarily due to a phenomenon known as Rayleigh scattering. This occurs when sunlight passes through Earth's atmosphere, encountering gas molecules and small particles like ozone and water vapor. The scattering of light by these tiny particles is more effective at shorter wavelengths, which correspond to the color blue. \nOur eyes have evolved to be more sensitive to blue light, enhancing its visibility. During sunrise or sunset, the longer path of sunlight through the atmosphere scatters out the blue wavelengths more effectively, resulting in the hues of red and orange we observe.\nIn summary:\n" - } - } - ], - "console": [] - } - ] -} \ No newline at end of file