The case study for the barycenter drivers of the solar cycle
Posted: 26.02.2018, 12:47
Would like to share a case study research for the barycenter drivers of the solar cycle, which was evaluated with the Clestia Planetarium.
In case the above link does not work with old Arcobat reader, you can open this link with another browser:
http://www.uvs-model.com/The case study for the b ... drivers of the solar cycle.pdf
Or access it from my website in a topic on "The solar cycle", then scroll down a bit and look for the link that was labelled as "The case study for the barycenter drivers of the solar cycle".
This is still a work in progress.
The plotting of barycenters of gas giants and drawing their alignments with the Sun and SSB for the major peaks and troughs of solar cycles were manually done, so it was very limiting and not productive. Nonetheless, as it was, its finding is already very assertive.
We hope to get advise from the community here on how to develop the add-ons to get this done systematically in the Celestia Planetarium like how we had done it manually. This would enable us to effective and easily evaluate the barycenter driver for every dip and spike of sunspot number in any solar cycle.
Any help is appreciated. Thanks in advance.
In case the above link does not work with old Arcobat reader, you can open this link with another browser:
http://www.uvs-model.com/The case study for the b ... drivers of the solar cycle.pdf
Or access it from my website in a topic on "The solar cycle", then scroll down a bit and look for the link that was labelled as "The case study for the barycenter drivers of the solar cycle".
This is still a work in progress.
The plotting of barycenters of gas giants and drawing their alignments with the Sun and SSB for the major peaks and troughs of solar cycles were manually done, so it was very limiting and not productive. Nonetheless, as it was, its finding is already very assertive.
We hope to get advise from the community here on how to develop the add-ons to get this done systematically in the Celestia Planetarium like how we had done it manually. This would enable us to effective and easily evaluate the barycenter driver for every dip and spike of sunspot number in any solar cycle.
![Help! :help:](./images/smilies/smile_help.gif)
Any help is appreciated. Thanks in advance.