[GH-ISSUE #5784] How to Deploy LLM Based on ollama in an offline environment? #65639

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GiteaMirror · 2026-05-03T21:59:09-05:00

GiteaMirror commented

2026-05-03 21:59:09 -05:00

Originally created by @RyanOvO on GitHub (Jul 19, 2024).
Original GitHub issue: https://github.com/ollama/ollama/issues/5784

ollama is now ready and I am deploying based on binary files. I have downloaded the GLM4 model file and the glm4 adaptation file for ollama. However, GLM4 does not provide guff at present. How can I deploy inference glm4 based on ollama in an offline environment?

Originally created by @RyanOvO on GitHub (Jul 19, 2024). Original GitHub issue: https://github.com/ollama/ollama/issues/5784 ollama is now ready and I am deploying based on binary files. I have downloaded the GLM4 model file and [the glm4 adaptation file for ollama](https://ollama.com/library/glm4:9b). However, GLM4 does not provide guff at present. How can I deploy inference glm4 based on ollama in an offline environment?

GiteaMirror closed this issue

2026-05-03 21:59:10 -05:00

GiteaMirror commented

2026-05-03 21:59:12 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

If you have downloaded the model with ollama pull glm4:9b, then all you need to do is ollama run glm4:9b to use the model from the command line. If you want API access, you can use the ollama python module:

#!/usr/bin/env python3

import ollama

client = ollama.Client()
print(client.generate(model="glm4:9b", prompt="why is the sky blue?"))

If you have a client that just talks HTTP, you can hit the API endpoint directly, eg with curl:

curl -s http://localhost:11434/api/generate -d '{"model": "glm4:9b", "prompt": "why is the sky blue?", "stream": false}'

@rick-github commented on GitHub (Jul 19, 2024): If you have downloaded the model with `ollama pull glm4:9b`, then all you need to do is `ollama run glm4:9b` to use the model from the command line. If you want API access, you can use the `ollama` python module: ``` #!/usr/bin/env python3 import ollama client = ollama.Client() print(client.generate(model="glm4:9b", prompt="why is the sky blue?")) ``` If you have a client that just talks HTTP, you can hit the API endpoint directly, eg with curl: ``` curl -s http://localhost:11434/api/generate -d '{"model": "glm4:9b", "prompt": "why is the sky blue?", "stream": false}' ```

GiteaMirror commented

2026-05-03 21:59:13 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

If you have downloaded the model with ollama pull glm4:9b, then all you need to do is ollama run glm4:9b to use the model from the command line. If you want API access, you can use the ollama python module:
#!/usr/bin/env python3

import ollama

client = ollama.Client()
print(client.generate(model="glm4:9b", prompt="why is the sky blue?"))
If you have a client that just talks HTTP, you can hit the API endpoint directly, eg with curl:
curl -s http://localhost:11434/api/generate -d '{"model": "glm4:9b", "prompt": "why is the sky blue?", "stream": false}'

thanks a lot！
Do you know where to download ollama run?

@RyanOvO commented on GitHub (Jul 19, 2024): > If you have downloaded the model with `ollama pull glm4:9b`, then all you need to do is `ollama run glm4:9b` to use the model from the command line. If you want API access, you can use the `ollama` python module: > > ``` > #!/usr/bin/env python3 > > import ollama > > client = ollama.Client() > print(client.generate(model="glm4:9b", prompt="why is the sky blue?")) > ``` > > If you have a client that just talks HTTP, you can hit the API endpoint directly, eg with curl: > > ``` > curl -s http://localhost:11434/api/generate -d '{"model": "glm4:9b", "prompt": "why is the sky blue?", "stream": false}' > ``` thanks a lot！ Do you know where to download ollama run?

GiteaMirror commented

2026-05-03 21:59:14 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

If you've installed ollama, ollama is a command that takes parameters to perform actions. run is an action, so just type ollama run glm4:9b to talk to the glm4:9b model.

@rick-github commented on GitHub (Jul 19, 2024): If you've installed ollama, `ollama` is a command that takes parameters to perform actions. `run` is an action, so just type `ollama run glm4:9b` to talk to the `glm4:9b` model.

GiteaMirror commented

2026-05-03 21:59:14 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

For example:

rick@z4070 ~ $ ollama run glm4:9b
>>> why is the sky blue?
The sky appears blue because of a phenomenon called Rayleigh scattering, which occurs when sunlight interacts with molecules and particles in Earth's atmosphere.

Here's a simplified explanation of how it happens:

1. **Sunlight Composition**: Sunlight is made up of all the colors of the visible spectrum (red, orange, yellow, green, blue, indigo, and violet), each with its own wavelength.

2. **Rayleigh Scattering**: When sunlight enters Earth's atmosphere, it encounters molecules such as nitrogen and oxygen. These molecules are much smaller than the wavelengths of visible light. When a 
photon (a particle of light) collides with an atom or molecule, the electron in the atom can briefly absorb some of the energy of the photon and then re-emit it.

3. **Frequency Dependency**: Rayleigh scattering is more effective for shorter wavelengths (blue and violet) than for longer wavelengths (red). This means that blue light is scattered more easily in the 
atmosphere than red light.

4. **Directional Scattering**: When the scattered light is directed towards an observer, that observer sees a sky with more of the scattered blue light than any other color. The scattering effect is more 
pronounced at shorter angles from the direction of sunlight (towards the horizon), which gives the sky its characteristic blue appearance during the day.

5. **Atmospheric Conditions**: Weather phenomena like raindrops and cloud particles can enhance Rayleigh scattering, making the sky appear brighter and more vibrant with a stronger blue color.

This is why on a clear, sunny day, when there are few particles in the atmosphere to scatter light, we see a very blue sky. Conversely, at sunrise and sunset, sunlight travels through more of the 
atmosphere before reaching our eyes, so it encounters more scattering. The red colors in the sunrise or sunset are due to Rayleigh scattering that preferentially scatters shorter blue wavelengths away from 
the sun, leaving behind longer-wavelength reds, oranges, and yellows.

>>> /bye
(base) rick@z4070 ~ $

@rick-github commented on GitHub (Jul 19, 2024): For example: ``` rick@z4070 ~ $ ollama run glm4:9b >>> why is the sky blue? The sky appears blue because of a phenomenon called Rayleigh scattering, which occurs when sunlight interacts with molecules and particles in Earth's atmosphere. Here's a simplified explanation of how it happens: 1. **Sunlight Composition**: Sunlight is made up of all the colors of the visible spectrum (red, orange, yellow, green, blue, indigo, and violet), each with its own wavelength. 2. **Rayleigh Scattering**: When sunlight enters Earth's atmosphere, it encounters molecules such as nitrogen and oxygen. These molecules are much smaller than the wavelengths of visible light. When a photon (a particle of light) collides with an atom or molecule, the electron in the atom can briefly absorb some of the energy of the photon and then re-emit it. 3. **Frequency Dependency**: Rayleigh scattering is more effective for shorter wavelengths (blue and violet) than for longer wavelengths (red). This means that blue light is scattered more easily in the atmosphere than red light. 4. **Directional Scattering**: When the scattered light is directed towards an observer, that observer sees a sky with more of the scattered blue light than any other color. The scattering effect is more pronounced at shorter angles from the direction of sunlight (towards the horizon), which gives the sky its characteristic blue appearance during the day. 5. **Atmospheric Conditions**: Weather phenomena like raindrops and cloud particles can enhance Rayleigh scattering, making the sky appear brighter and more vibrant with a stronger blue color. This is why on a clear, sunny day, when there are few particles in the atmosphere to scatter light, we see a very blue sky. Conversely, at sunrise and sunset, sunlight travels through more of the atmosphere before reaching our eyes, so it encounters more scattering. The red colors in the sunrise or sunset are due to Rayleigh scattering that preferentially scatters shorter blue wavelengths away from the sun, leaving behind longer-wavelength reds, oranges, and yellows. >>> /bye (base) rick@z4070 ~ $ ```

GiteaMirror commented

2026-05-03 21:59:15 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

If you've installed ollama, ollama is a command that takes parameters to perform actions. run is an action, so just type ollama run glm4:9b to talk to the glm4:9b model.

u are right.But now I find that I failed to download glm4:9b.My idea was to download glm4:9b on my virtual machine and copy it to an offline A10, but obviously I was wrong

@RyanOvO commented on GitHub (Jul 19, 2024): > If you've installed ollama, `ollama` is a command that takes parameters to perform actions. `run` is an action, so just type `ollama run glm4:9b` to talk to the `glm4:9b` model. u are right.But now I find that I failed to download glm4:9b.My idea was to download glm4:9b on my virtual machine and copy it to an offline A10, but obviously I was wrong

GiteaMirror commented

2026-05-03 21:59:16 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

For example:

rick@z4070 ~ $ ollama run glm4:9b
>>> why is the sky blue?
The sky appears blue because of a phenomenon called Rayleigh scattering, which occurs when sunlight interacts with molecules and particles in Earth's atmosphere.

Here's a simplified explanation of how it happens:

1. **Sunlight Composition**: Sunlight is made up of all the colors of the visible spectrum (red, orange, yellow, green, blue, indigo, and violet), each with its own wavelength.

2. **Rayleigh Scattering**: When sunlight enters Earth's atmosphere, it encounters molecules such as nitrogen and oxygen. These molecules are much smaller than the wavelengths of visible light. When a 
photon (a particle of light) collides with an atom or molecule, the electron in the atom can briefly absorb some of the energy of the photon and then re-emit it.

3. **Frequency Dependency**: Rayleigh scattering is more effective for shorter wavelengths (blue and violet) than for longer wavelengths (red). This means that blue light is scattered more easily in the 
atmosphere than red light.

4. **Directional Scattering**: When the scattered light is directed towards an observer, that observer sees a sky with more of the scattered blue light than any other color. The scattering effect is more 
pronounced at shorter angles from the direction of sunlight (towards the horizon), which gives the sky its characteristic blue appearance during the day.

5. **Atmospheric Conditions**: Weather phenomena like raindrops and cloud particles can enhance Rayleigh scattering, making the sky appear brighter and more vibrant with a stronger blue color.

This is why on a clear, sunny day, when there are few particles in the atmosphere to scatter light, we see a very blue sky. Conversely, at sunrise and sunset, sunlight travels through more of the 
atmosphere before reaching our eyes, so it encounters more scattering. The red colors in the sunrise or sunset are due to Rayleigh scattering that preferentially scatters shorter blue wavelengths away from 
the sun, leaving behind longer-wavelength reds, oranges, and yellows.

>>> /bye
(base) rick@z4070 ~ $

ok, Now I know how ollama works

@RyanOvO commented on GitHub (Jul 19, 2024): > For example: > > ``` > rick@z4070 ~ $ ollama run glm4:9b > >>> why is the sky blue? > The sky appears blue because of a phenomenon called Rayleigh scattering, which occurs when sunlight interacts with molecules and particles in Earth's atmosphere. > > Here's a simplified explanation of how it happens: > > 1. **Sunlight Composition**: Sunlight is made up of all the colors of the visible spectrum (red, orange, yellow, green, blue, indigo, and violet), each with its own wavelength. > > 2. **Rayleigh Scattering**: When sunlight enters Earth's atmosphere, it encounters molecules such as nitrogen and oxygen. These molecules are much smaller than the wavelengths of visible light. When a > photon (a particle of light) collides with an atom or molecule, the electron in the atom can briefly absorb some of the energy of the photon and then re-emit it. > > 3. **Frequency Dependency**: Rayleigh scattering is more effective for shorter wavelengths (blue and violet) than for longer wavelengths (red). This means that blue light is scattered more easily in the > atmosphere than red light. > > 4. **Directional Scattering**: When the scattered light is directed towards an observer, that observer sees a sky with more of the scattered blue light than any other color. The scattering effect is more > pronounced at shorter angles from the direction of sunlight (towards the horizon), which gives the sky its characteristic blue appearance during the day. > > 5. **Atmospheric Conditions**: Weather phenomena like raindrops and cloud particles can enhance Rayleigh scattering, making the sky appear brighter and more vibrant with a stronger blue color. > > This is why on a clear, sunny day, when there are few particles in the atmosphere to scatter light, we see a very blue sky. Conversely, at sunrise and sunset, sunlight travels through more of the > atmosphere before reaching our eyes, so it encounters more scattering. The red colors in the sunrise or sunset are due to Rayleigh scattering that preferentially scatters shorter blue wavelengths away from > the sun, leaving behind longer-wavelength reds, oranges, and yellows. > > >>> /bye > (base) rick@z4070 ~ $ > ``` ok, Now I know how ollama works

GiteaMirror commented

2026-05-03 21:59:17 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

The downloaded model is stored locally (see the faq based on your platform) so you should be able to copy the entire directory to the machine hosting the A10.

@rick-github commented on GitHub (Jul 19, 2024): The downloaded model is stored locally (see the [faq](https://github.com/ollama/ollama/blob/main/docs/faq.md#where-are-models-stored) based on your platform) so you should be able to copy the entire directory to the machine hosting the A10.

GiteaMirror commented

2026-05-03 21:59:18 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

thanks a lot ! again!

@RyanOvO commented on GitHub (Jul 19, 2024): thanks a lot ! again!

GiteaMirror commented

2026-05-03 21:59:19 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

The downloaded model is stored locally (see the faq based on your platform) so you should be able to copy the entire directory to the machine hosting the A10.

A10 上的ollama如何识别我拷贝过去的glm4:9b呢？

@RyanOvO commented on GitHub (Jul 19, 2024): > The downloaded model is stored locally (see the [faq](https://github.com/ollama/ollama/blob/main/docs/faq.md#where-are-models-stored) based on your platform) so you should be able to copy the entire directory to the machine hosting the A10. A10 上的ollama如何识别我拷贝过去的glm4:9b呢？

GiteaMirror commented

2026-05-03 21:59:21 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

You need to install ollama on the machine with the A10. Then copy the model from your virtual machine to the A10 machine. Then start ollama, ollama serve if it's not started as a system service. Then ollama run glm4:9b to talk to the model.

@rick-github commented on GitHub (Jul 19, 2024): You need to install ollama on the machine with the A10. Then copy the model from your virtual machine to the A10 machine. Then start ollama, `ollama serve` if it's not started as a system service. Then `ollama run glm4:9b` to talk to the model.

GiteaMirror commented

2026-05-03 21:59:22 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

You need to install ollama on the machine with the A10. Then copy the model from your virtual machine to the A10 machine. Then start ollama, ollama serve if it's not started as a system service. Then ollama run glm4:9b to talk to the model.

I have downloaded the ollama binary package on a10 and started ollama.
My problem is that I copy the glm4:9b downloaded from the VM to the default download path in ollama. ollama automatically recognizes that the model file exists in this path, and the download succeeds, right?

@RyanOvO commented on GitHub (Jul 19, 2024): > You need to install ollama on the machine with the A10. Then copy the model from your virtual machine to the A10 machine. Then start ollama, `ollama serve` if it's not started as a system service. Then `ollama run glm4:9b` to talk to the model. I have downloaded the ollama binary package on a10 and started ollama. My problem is that I copy the glm4:9b downloaded from the VM to the default download path in ollama. ollama automatically recognizes that the model file exists in this path, and the download succeeds, right?

GiteaMirror commented

2026-05-03 21:59:24 -05:00

@rick-github commented on GitHub (Jul 19, 2024):

Yes. Make that you have copied across the files in the models/blobs and the models/manifests directories. I don't think you need to restart the ollama service after copying, but try that if ollama list doesn't show the glm4:9b model.

@rick-github commented on GitHub (Jul 19, 2024): Yes. Make that you have copied across the files in the `models/blobs` and the `models/manifests` directories. I don't think you need to restart the ollama service after copying, but try that if `ollama list` doesn't show the glm4:9b model.

GiteaMirror commented

2026-05-03 21:59:25 -05:00

@RyanOvO commented on GitHub (Jul 19, 2024):

Yes. Make that you have copied across the files in the models/blobs and the models/manifests directories. I don't think you need to restart the ollama service after copying, but try that if ollama list doesn't show the glm4:9b model.

ok, u helped me a lot.
thanks bro !

@RyanOvO commented on GitHub (Jul 19, 2024): > Yes. Make that you have copied across the files in the `models/blobs` and the `models/manifests` directories. I don't think you need to restart the ollama service after copying, but try that if `ollama list` doesn't show the glm4:9b model. ok, u helped me a lot. thanks bro !

GiteaMirror commented

2026-05-03 21:59:26 -05:00

@Pyenb commented on GitHub (Aug 19, 2024):

Hey there, small update for anyone interested. Since this issue was still bothering me, I took matters into my own hands and created an Ollama model repository, where you can download the zipped official ollama models and import them to your offline machine or wherever.

Any feedback is appreciated 👍 More models will be coming soon.

@Pyenb commented on GitHub (Aug 19, 2024): Hey there, small update for anyone interested. Since this issue was still bothering me, I took matters into my own hands and created an [Ollama model repository](https://github.com/Pyenb/Ollama-models), where you can download the zipped official ollama models and import them to your offline machine or wherever. Any feedback is appreciated 👍 More models will be coming soon.

GiteaMirror commented

2026-05-03 21:59:29 -05:00

@RyanOvO commented on GitHub (Aug 20, 2024):

Hey there, small update for anyone interested. Since this issue was still bothering me, I took matters into my own hands and created an Ollama model repository, where you can download the zipped official ollama models and import them to your offline machine or wherever.

Any feedback is appreciated 👍 More models will be coming soon.

oh，that's great and an amazing work! I gave start

@RyanOvO commented on GitHub (Aug 20, 2024): > Hey there, small update for anyone interested. Since this issue was still bothering me, I took matters into my own hands and created an [Ollama model repository](https://github.com/Pyenb/Ollama-models), where you can download the zipped official ollama models and import them to your offline machine or wherever. > > Any feedback is appreciated 👍 More models will be coming soon. oh，that's great and an amazing work! I gave start

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parth/cmd-cleanup-SO

brucemacd/check-key-register-structured-err

parth/openai-stream-usage

parth/fix-referencing-so

stream-tools-stop

jmorganca/degin-1

brucemacd/install-path-clean

brucemacd/push-name-validation

brucemacd/browser-key-register

jmorganca/openai-fix-first-message

jmorganca/fix-proxy

jessegross/sample

parth/disallow-streaming-tools

dhiltgen/remove_submodule

jmorganca/ga

jmorganca/mllama

pdevine/newlines

pdevine/geems-2b

jmorganca/llama-bump

mxyng/modelname-7

mxyng/gin-slog

mxyng/modelname-6

jyan/convert-prog

jyan/quant5

paligemma-support

pdevine/import-docs

jmorganca/openai-context

jyan/paligemma

jyan/p2

jyan/palitest

bmizerany/embedspeedup

jmorganca/llama-vit

brucemacd/allow-ollama

royh/ep-methods

royh/whisper

mxyng/api-models

mxyng/fix-memory

jyan/q4_4/8

jyan/ollama-v

royh/stream-tools

roy-embed-parallel

bmizerany/hrm

revert-5963-revert-5924-mxyng/llama3.1-rope

royh/embed-viz

jyan/local2

jyan/auth

jyan/local

jyan/parse-temp

jmorganca/template-mistral

jyan/reord-g

royh-openai-suffixdocs

royh-imgembed

royh-embed-parallel

jyan/quant4

royh-precision

jyan/progress

pdevine/fix-template

jyan/quant3

pdevine/ggla

mxyng/update-registry-domain

jmorganca/ggml-static

mxyng/create-context

jyan/v0.146

mxyng/layers-from-files

build_dist

bmizerany/noseek

royh-ls

royh-name

timeout

mxyng/server-timestamp

bmizerany/nosillyggufslurps

royh-params

jmorganca/llama-cpp-7c26775

royh-openai-delete

royh-show-rigid

jmorganca/enable-fa

jmorganca/no-error-template

jyan/format

royh-testdelete

bmizerany/fastverify

language_support

pdevine/ps-glitches

brucemacd/tokenize

bruce/iq-quants

bmizerany/filepathwithcoloninhost

mxyng/split-bin

bmizerany/client-registry

jmorganca/if-none-match

native

jmorganca/native

jmorganca/batch-embeddings

jmorganca/initcmake

jmorganca/mm

pdevine/showggmlinfo

modenameenforcealphanum

bmizerany/modenameenforcealphanum

jmorganca/done-reason

jmorganca/llama-cpp-8960fe8

ollama.com

bmizerany/filepathnobuild

bmizerany/types/model/defaultfix

rmdisplaylong

nogogen

bmizerany/x

modelfile-readme

bmizerany/replacecolon

jmorganca/limit

jmorganca/execstack

jmorganca/replace-assets

mxyng/tune-concurrency

jmorganca/testing

whitespace-detection

jmorganca/options

upgrade-all

scratch

cuda-search

mattw/airenamer

mattw/allmodelsonhuggingface

mattw/quantcontext

mattw/whatneedstorun

brucemacd/llama-mem-calc

mattw/faq-context

mattw/communitylinks

mattw/noprune

mattw/python-functioncalling

rename

mxyng/install

pulse

remove-first

editor

mattw/selfqueryingretrieval

cgo

mattw/howtoquant

api

matt/streamingapi

format-config

mxyng/extra-args

shell

update-nous-hermes

cp-model

upload-progress

fix-unknown-model

fix-model-names

delete-fix

insecure-registry

ls

deletemodels

progressbar

readme-updates

license-layers

skip-list

list-models

modelpath

matt/examplemodelfiles

distribution

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Reference: github-starred/ollama#65639