[mesa-users] binary evolution(timestep controls)
吴优
youwu at ynao.ac.cn
Thu Jun 2 04:22:37 EDT 2016
Hi Rob
> So you need to change the "fr" variables. You allready said you tried "fr",
> what about:
>
> !### fr_limit
> fr_limit = 1d-2
>
> !### fr_dt_limit
> ! Minimum timestep limit allowed for the fr control in years.
> fr_dt_limit = 10d0
Thank you for your advice!
But i have tried to change those parameters("fr_limit=1d-2"and"fr_dt_limit=10d0"),it dose not seem to work as before.
timesteps ( log_dt ) stays about -3 for tens of thousands of steps,and look unlikely to go back to normal.
Many Thanks!
You Wu
> -----原始邮件-----
> 发件人: mesa-users-request at lists.sourceforge.net
> 发送时间: 2016年6月1日 星期三
> 收件人: mesa-users at lists.sourceforge.net
> 抄送:
> 主题: mesa-users Digest, Vol 81, Issue 14
>
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>
>
> Today's Topics:
>
> 1. Re: Question (Abel Schootemeijer)
> 2. Re: Question (Bill Paxton)
> 3. Re: Question (Aaron Dotter)
> 4. Re: Question (Max Katz)
> 5. Re: binary evolution(timestep controls) (Robert Farmer)
> 6. Re: Question (Bill Paxton)
>
>
> ----------------------------------------------------------------------
>
> Message: 1
> Date: Tue, 31 May 2016 16:22:15 +0200
> From: Abel Schootemeijer <schootemeijerabel at gmail.com>
> Subject: Re: [mesa-users] Question
> Cc: "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID:
> <CAF9o_j9ZCNO5eHUR0KsBHN8Nx5HmikA88hc8BfornSiHJ8iDnw at mail.gmail.com>
> Content-Type: text/plain; charset="utf-8"
>
> Hello,
>
> (Disclaimer: it is very well possible that I completely misunderstood the
> problem, in that case please accept my apologies :) )
>
>
> If the problem is that the output file is hard to read because a row with
> many elements continues on a new line (instead of a one row per line
> format), you can for example do
>
> :set nowrap
>
> if you are using vim, to display the file with one row per line, so the
> elements of one column are displayed right below one another.
>
> Kind regards,
> Abel
>
>
> 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
>
> > Hi,
> >
> > The final model file contains only the minimum information needed to
> > specify the structure and abundance.
> >
> > The final profile model will have the basics and much more. So you
> > probably should be getting the information you need from that.
> >
> > Most of the test cases have lines like the following in the inlist
> > &star_job section:
> >
> >
> > save_model_when_terminate = .true.
> > save_model_filename = 'final.mod'
> >
> > write_profile_when_terminate = .true.
> > filename_for_profile_when_terminate = 'final_profile.data'
> >
> > The "final.mod" has what is needed to start a new run.
> > The "final_profile.data" has lots of information about that model.
> >
> > Add to your "profile_columns.list" to add things to the profile.
> > See star/defaults/profile_columns.list for options you can add.
> > For things not built-in, use your run_star_extras to add your own.
> >
> > e.g., you might pick from these
> >
> > ! average charge from ionization module
> > !avg_charge_H
> > !avg_charge_He
> > !avg_charge_C
> > !avg_charge_N
> > !avg_charge_O
> > !avg_charge_Ne
> > !avg_charge_Mg
> > !avg_charge_Si
> > !avg_charge_Fe
> >
> > ! average neutral fraction from ionization module
> > !neutral_fraction_H
> > !neutral_fraction_He
> > !neutral_fraction_C
> > !neutral_fraction_N
> > !neutral_fraction_O
> > !neutral_fraction_Ne
> > !neutral_fraction_Mg
> > !neutral_fraction_Si
> > !neutral_fraction_Fe
> >
> >
> > b
> >
> >
> >
> >
> >
> >
> > On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
> >
> > > Sorry for my late reply. I need to extract the abundances and
> > ionizations of the several chemical elements from the final model. I am
> > trying to understand where it is saved and how it is organized. But am
> > unable to find it. I can't understand where one starts and the other ends.
> >
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and
> > traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols
> > are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> -------------- next part --------------
> An HTML attachment was scrubbed...
>
> ------------------------------
>
> Message: 2
> Date: Tue, 31 May 2016 09:02:42 -0700
> From: Bill Paxton <paxton at kitp.ucsb.edu>
> Subject: Re: [mesa-users] Question
> To: Abel Schootemeijer <schootemeijerabel at gmail.com>
> Cc: "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID: <6CCB23B0-A9F4-4C50-87FA-5D8B361D5BF0 at kitp.ucsb.edu>
> Content-Type: text/plain; charset="us-ascii"
>
> Hi Abel,
>
> > If the problem is that the output file is hard to read because a row with many elements continues on a new line
>
> Excellent new take on what might be the problem (I have to admit that I don't know what the actual problem is!). I didn't even think of that since I never look at the text files (I make plots plots and more plots). But in the rare cases where I do check something in the editor, I can set it so that it doesn't break lines of the file onto separate lines on the screen (same as your nowrap). Then I simply use horizontal scrolling. Or if I want to get several values from a row, I'll copy it to a separate file and replace spaces by CR's. then do the same for the line with the column names and match up names with values. It might be useful to have a script that would do that automatically, but I don't resort to doing it enough to be motivated to create such a script!
>
> Perhaps someone else has a trick for doing this. But unless you need many digits of output, making plots is the better solution in my experience.
>
> Cheers,
> Bill
>
>
>
>
>
>
> On May 31, 2016, at 7:22 AM, Abel Schootemeijer wrote:
>
> > Hello,
> >
> > (Disclaimer: it is very well possible that I completely misunderstood the problem, in that case please accept my apologies :) )
> >
> >
> > If the problem is that the output file is hard to read because a row with many elements continues on a new line (instead of a one row per line format), you can for example do
> >
> > :set nowrap
> >
> > if you are using vim, to display the file with one row per line, so the elements of one column are displayed right below one another.
> >
> > Kind regards,
> > Abel
> >
> >
> > 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
> > Hi,
> >
> > The final model file contains only the minimum information needed to specify the structure and abundance.
> >
> > The final profile model will have the basics and much more. So you probably should be getting the information you need from that.
> >
> > Most of the test cases have lines like the following in the inlist &star_job section:
> >
> >
> > save_model_when_terminate = .true.
> > save_model_filename = 'final.mod'
> >
> > write_profile_when_terminate = .true.
> > filename_for_profile_when_terminate = 'final_profile.data'
> >
> > The "final.mod" has what is needed to start a new run.
> > The "final_profile.data" has lots of information about that model.
> >
> > Add to your "profile_columns.list" to add things to the profile.
> > See star/defaults/profile_columns.list for options you can add.
> > For things not built-in, use your run_star_extras to add your own.
> >
> > e.g., you might pick from these
> >
> > ! average charge from ionization module
> > !avg_charge_H
> > !avg_charge_He
> > !avg_charge_C
> > !avg_charge_N
> > !avg_charge_O
> > !avg_charge_Ne
> > !avg_charge_Mg
> > !avg_charge_Si
> > !avg_charge_Fe
> >
> > ! average neutral fraction from ionization module
> > !neutral_fraction_H
> > !neutral_fraction_He
> > !neutral_fraction_C
> > !neutral_fraction_N
> > !neutral_fraction_O
> > !neutral_fraction_Ne
> > !neutral_fraction_Mg
> > !neutral_fraction_Si
> > !neutral_fraction_Fe
> >
> >
> > b
> >
> >
> >
> >
> >
> >
> > On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
> >
> > > Sorry for my late reply. I need to extract the abundances and ionizations of the several chemical elements from the final model. I am trying to understand where it is saved and how it is organized. But am unable to find it. I can't understand where one starts and the other ends.
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e_______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
>
> -------------- next part --------------
> An HTML attachment was scrubbed...
>
> ------------------------------
>
> Message: 3
> Date: Tue, 31 May 2016 13:16:51 -0400
> From: Aaron Dotter <aaron.dotter at gmail.com>
> Subject: Re: [mesa-users] Question
> To: Bill Paxton <paxton at kitp.ucsb.edu>
> Cc: "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID:
> <CAN5--jPSj_a8La_2KQ8hYKsu=xmkS0R5V7uvhuj4Xz3LFdVUzQ at mail.gmail.com>
> Content-Type: text/plain; charset="utf-8"
>
> The most useful single thing I've ever found for reading MESA history files
> and profiles in the terminal:
>
> less -S history.data
>
> from the less manual
>
> -S or --chop-long-lines
> Causes lines longer than the screen width to be chopped
> (trun?
> cated) rather than wrapped. That is, the portion of a long
> line
> that does not fit in the screen width is not shown. The
> default
> is to wrap long lines; that is, display the remainder on
> the
> next line.
>
> And from there you can use the arrow left and right keys to browse
> horizontally through the file. Changed my life!
>
> Aaron
>
>
> On Tue, May 31, 2016 at 12:02 PM, Bill Paxton <paxton at kitp.ucsb.edu> wrote:
>
> > Hi Abel,
> >
> > If the problem is that the output file is hard to read because a row with
> > many elements continues on a new line
> >
> >
> > Excellent new take on what might be the problem (I have to admit that I
> > don't know what the actual problem is!). I didn't even think of that
> > since I never look at the text files (I make plots plots and more plots).
> > But in the rare cases where I do check something in the editor, I can set
> > it so that it doesn't break lines of the file onto separate lines on the
> > screen (same as your nowrap). Then I simply use horizontal scrolling. Or
> > if I want to get several values from a row, I'll copy it to a separate file
> > and replace spaces by CR's. then do the same for the line with the column
> > names and match up names with values. It might be useful to have a script
> > that would do that automatically, but I don't resort to doing it enough to
> > be motivated to create such a script!
> >
> > Perhaps someone else has a trick for doing this. But unless you need many
> > digits of output, making plots is the better solution in my experience.
> >
> > Cheers,
> > Bill
> >
> >
> >
> >
> >
> >
> > On May 31, 2016, at 7:22 AM, Abel Schootemeijer wrote:
> >
> > Hello,
> >
> > (Disclaimer: it is very well possible that I completely misunderstood the
> > problem, in that case please accept my apologies :) )
> >
> >
> > If the problem is that the output file is hard to read because a row with
> > many elements continues on a new line (instead of a one row per line
> > format), you can for example do
> >
> > :set nowrap
> >
> > if you are using vim, to display the file with one row per line, so the
> > elements of one column are displayed right below one another.
> >
> > Kind regards,
> > Abel
> >
> >
> > 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
> >
> >> Hi,
> >>
> >> The final model file contains only the minimum information needed to
> >> specify the structure and abundance.
> >>
> >> The final profile model will have the basics and much more. So you
> >> probably should be getting the information you need from that.
> >>
> >> Most of the test cases have lines like the following in the inlist
> >> &star_job section:
> >>
> >>
> >> save_model_when_terminate = .true.
> >> save_model_filename = 'final.mod'
> >>
> >> write_profile_when_terminate = .true.
> >> filename_for_profile_when_terminate = 'final_profile.data'
> >>
> >> The "final.mod" has what is needed to start a new run.
> >> The "final_profile.data" has lots of information about that model.
> >>
> >> Add to your "profile_columns.list" to add things to the profile.
> >> See star/defaults/profile_columns.list for options you can add.
> >> For things not built-in, use your run_star_extras to add your own.
> >>
> >> e.g., you might pick from these
> >>
> >> ! average charge from ionization module
> >> !avg_charge_H
> >> !avg_charge_He
> >> !avg_charge_C
> >> !avg_charge_N
> >> !avg_charge_O
> >> !avg_charge_Ne
> >> !avg_charge_Mg
> >> !avg_charge_Si
> >> !avg_charge_Fe
> >>
> >> ! average neutral fraction from ionization module
> >> !neutral_fraction_H
> >> !neutral_fraction_He
> >> !neutral_fraction_C
> >> !neutral_fraction_N
> >> !neutral_fraction_O
> >> !neutral_fraction_Ne
> >> !neutral_fraction_Mg
> >> !neutral_fraction_Si
> >> !neutral_fraction_Fe
> >>
> >>
> >> b
> >>
> >>
> >>
> >>
> >>
> >>
> >> On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
> >>
> >> > Sorry for my late reply. I need to extract the abundances and
> >> ionizations of the several chemical elements from the final model. I am
> >> trying to understand where it is saved and how it is organized. But am
> >> unable to find it. I can't understand where one starts and the other ends.
> >>
> >>
> >>
> >> ------------------------------------------------------------------------------
> >> What NetFlow Analyzer can do for you? Monitors network bandwidth and
> >> traffic
> >> patterns at an interface-level. Reveals which users, apps, and protocols
> >> are
> >> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >> planning reports.
> >> https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> >> _______________________________________________
> >> mesa-users mailing list
> >> mesa-users at lists.sourceforge.net
> >> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >>
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and
> > traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols
> > are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports.
> > https://ad.doubleclick.net/ddm/clk/305295220;132659582;e_______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and
> > traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols
> > are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
> -------------- next part --------------
> An HTML attachment was scrubbed...
>
> ------------------------------
>
> Message: 4
> Date: Tue, 31 May 2016 13:36:30 -0400
> From: Max Katz <maxpkatz at gmail.com>
> Subject: Re: [mesa-users] Question
> To: Aaron Dotter <aaron.dotter at gmail.com>
> Cc: "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID:
> <CAACUSYnxk4k+g9meM_x2GNQjc8S8bh3h9Nz6KZgM767ha=DrVw at mail.gmail.com>
> Content-Type: text/plain; charset="utf-8"
>
> For emacs, you can do M-x toggle-truncate-lines. I have this assigned to a
> hotkey in my ~/.emacs file,
>
>
> (global-set-key (kbd "<f6>") 'toggle-truncate-lines)
>
>
> which allows me to press F6 on my keyboard and truncate lines (no text
> wrap) after opening a text file.
>
> Another fun trick I found after some searching relates to the problem of
> scrolling up and down in a column in emacs. By default, if you scroll down
> with your mouse or press Page Down, your cursor will reset to the beginning
> of the row, which makes it annoying to try and see how a given variable
> changes over time. The emacswiki tells you what to add to your .emacs file
> to get around this <https://www.emacswiki.org/emacs/Scrolling>,
>
> (defun sfp-page-down ()
> (interactive)
> (setq this-command 'next-line)
> (next-line
> (- (window-text-height)
> next-screen-context-lines)))
>
> (defun sfp-page-up ()
> (interactive)
> (setq this-command 'previous-line)
> (previous-line
> (- (window-text-height)
> next-screen-context-lines)))
>
> (global-set-key [next] 'sfp-page-down)
> (global-set-key [prior] 'sfp-page-up)
>
>
> Note also that in emacs you can do Ctrl+Left and Ctrl+Right to more quickly
> navigate across columns.
>
> (Cue everyone reporting in what their personal setup is...)
>
> Max Katz
> Ph.D. Candidate, Department of Physics and Astronomy
> Stony Brook University
> http://astro.sunysb.edu/mkatz/
>
> On Tue, May 31, 2016 at 1:16 PM, Aaron Dotter <aaron.dotter at gmail.com>
> wrote:
>
> > The most useful single thing I've ever found for reading MESA history
> > files and profiles in the terminal:
> >
> > less -S history.data
> >
> > from the less manual
> >
> > -S or --chop-long-lines
> > Causes lines longer than the screen width to be chopped
> > (trun?
> > cated) rather than wrapped. That is, the portion of a long
> > line
> > that does not fit in the screen width is not shown. The
> > default
> > is to wrap long lines; that is, display the remainder on
> > the
> > next line.
> >
> > And from there you can use the arrow left and right keys to browse
> > horizontally through the file. Changed my life!
> >
> > Aaron
> >
> >
> > On Tue, May 31, 2016 at 12:02 PM, Bill Paxton <paxton at kitp.ucsb.edu>
> > wrote:
> >
> >> Hi Abel,
> >>
> >> If the problem is that the output file is hard to read because a row with
> >> many elements continues on a new line
> >>
> >>
> >> Excellent new take on what might be the problem (I have to admit that I
> >> don't know what the actual problem is!). I didn't even think of that
> >> since I never look at the text files (I make plots plots and more plots).
> >> But in the rare cases where I do check something in the editor, I can set
> >> it so that it doesn't break lines of the file onto separate lines on the
> >> screen (same as your nowrap). Then I simply use horizontal scrolling. Or
> >> if I want to get several values from a row, I'll copy it to a separate file
> >> and replace spaces by CR's. then do the same for the line with the column
> >> names and match up names with values. It might be useful to have a script
> >> that would do that automatically, but I don't resort to doing it enough to
> >> be motivated to create such a script!
> >>
> >> Perhaps someone else has a trick for doing this. But unless you need
> >> many digits of output, making plots is the better solution in my experience.
> >>
> >> Cheers,
> >> Bill
> >>
> >>
> >>
> >>
> >>
> >>
> >> On May 31, 2016, at 7:22 AM, Abel Schootemeijer wrote:
> >>
> >> Hello,
> >>
> >> (Disclaimer: it is very well possible that I completely misunderstood the
> >> problem, in that case please accept my apologies :) )
> >>
> >>
> >> If the problem is that the output file is hard to read because a row with
> >> many elements continues on a new line (instead of a one row per line
> >> format), you can for example do
> >>
> >> :set nowrap
> >>
> >> if you are using vim, to display the file with one row per line, so the
> >> elements of one column are displayed right below one another.
> >>
> >> Kind regards,
> >> Abel
> >>
> >>
> >> 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
> >>
> >>> Hi,
> >>>
> >>> The final model file contains only the minimum information needed to
> >>> specify the structure and abundance.
> >>>
> >>> The final profile model will have the basics and much more. So you
> >>> probably should be getting the information you need from that.
> >>>
> >>> Most of the test cases have lines like the following in the inlist
> >>> &star_job section:
> >>>
> >>>
> >>> save_model_when_terminate = .true.
> >>> save_model_filename = 'final.mod'
> >>>
> >>> write_profile_when_terminate = .true.
> >>> filename_for_profile_when_terminate = 'final_profile.data'
> >>>
> >>> The "final.mod" has what is needed to start a new run.
> >>> The "final_profile.data" has lots of information about that model.
> >>>
> >>> Add to your "profile_columns.list" to add things to the profile.
> >>> See star/defaults/profile_columns.list for options you can add.
> >>> For things not built-in, use your run_star_extras to add your own.
> >>>
> >>> e.g., you might pick from these
> >>>
> >>> ! average charge from ionization module
> >>> !avg_charge_H
> >>> !avg_charge_He
> >>> !avg_charge_C
> >>> !avg_charge_N
> >>> !avg_charge_O
> >>> !avg_charge_Ne
> >>> !avg_charge_Mg
> >>> !avg_charge_Si
> >>> !avg_charge_Fe
> >>>
> >>> ! average neutral fraction from ionization module
> >>> !neutral_fraction_H
> >>> !neutral_fraction_He
> >>> !neutral_fraction_C
> >>> !neutral_fraction_N
> >>> !neutral_fraction_O
> >>> !neutral_fraction_Ne
> >>> !neutral_fraction_Mg
> >>> !neutral_fraction_Si
> >>> !neutral_fraction_Fe
> >>>
> >>>
> >>> b
> >>>
> >>>
> >>>
> >>>
> >>>
> >>>
> >>> On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
> >>>
> >>> > Sorry for my late reply. I need to extract the abundances and
> >>> ionizations of the several chemical elements from the final model. I am
> >>> trying to understand where it is saved and how it is organized. But am
> >>> unable to find it. I can't understand where one starts and the other ends.
> >>>
> >>>
> >>>
> >>> ------------------------------------------------------------------------------
> >>> What NetFlow Analyzer can do for you? Monitors network bandwidth and
> >>> traffic
> >>> patterns at an interface-level. Reveals which users, apps, and protocols
> >>> are
> >>> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >>> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >>> planning reports.
> >>> https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> >>> _______________________________________________
> >>> mesa-users mailing list
> >>> mesa-users at lists.sourceforge.net
> >>> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >>>
> >>
> >>
> >> ------------------------------------------------------------------------------
> >> What NetFlow Analyzer can do for you? Monitors network bandwidth and
> >> traffic
> >> patterns at an interface-level. Reveals which users, apps, and protocols
> >> are
> >> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >> planning reports.
> >> https://ad.doubleclick.net/ddm/clk/305295220;132659582;e_______________________________________________
> >> mesa-users mailing list
> >> mesa-users at lists.sourceforge.net
> >> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >>
> >>
> >>
> >>
> >> ------------------------------------------------------------------------------
> >> What NetFlow Analyzer can do for you? Monitors network bandwidth and
> >> traffic
> >> patterns at an interface-level. Reveals which users, apps, and protocols
> >> are
> >> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >> planning reports.
> >> https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> >> _______________________________________________
> >> mesa-users mailing list
> >> mesa-users at lists.sourceforge.net
> >> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >>
> >>
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and
> > traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols
> > are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
> -------------- next part --------------
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> ------------------------------
>
> Message: 5
> Date: Tue, 31 May 2016 10:52:54 -0700
> From: Robert Farmer <rjfarmer at asu.edu>
> Subject: Re: [mesa-users] binary evolution(timestep controls)
> To: ?? <youwu at ynao.ac.cn>, "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID:
> <CAJ4VsmNdhx8ZT06YVkbUW-RTkUBLuj_LSXbN5OjXFPMsNgLXcQ at mail.gmail.com>
> Content-Type: text/plain; charset="utf-8"
>
> Hi
> Please keep replies on list, other may find the information useful.
>
> > I have changed these parameters
> ("fr"?"fm","fj","varcontrol_target"and"max_tries_to_achieve"),adjust them
> to large or small.
> Good
>
> >"Max increase" limiting the timestep in the terminal output.
> So running your inlists, firstly you should probably set terminal_cnt = 1
> so you can see every step in the output. In this case your timestep limiter
> is b_RL, so take that and search the binary_controls.defaults you find:
>
> !# timestep controls
> 'b_RL' fr
>
> So you need to change the "fr" variables. You allready said you tried "fr",
> what about:
>
> !### fr_limit
> fr_limit = 1d-2
>
> !### fr_dt_limit
> ! Minimum timestep limit allowed for the fr control in years.
> fr_dt_limit = 10d0
>
> However, as you being limited by the relative change in radius-roche lobe
> radius, and your mass transfer rate is quite high, you may simply not be
> able to evolve with a larger timestep and have physically meaningful
> results.
>
> Rob
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>
> Message: 6
> Date: Tue, 31 May 2016 11:00:30 -0700
> From: Bill Paxton <paxton at kitp.ucsb.edu>
> Subject: Re: [mesa-users] Question
> To: Max Katz <maxpkatz at gmail.com>, Aaron Dotter
> <aaron.dotter at gmail.com>
> Cc: "mesa-users at lists.sourceforge.net users"
> <mesa-users at lists.sourceforge.net>
> Message-ID: <55D1C4A2-A6DC-4BC5-BC4D-3C850E376C7C at kitp.ucsb.edu>
> Content-Type: text/plain; charset="utf-8"
>
> Thanks! This makes me think there should be a place on the website for users to share "how to" ideas for viewing histories and profiles -- perhaps including simple scripts for some of the popular plotting options. Would that be useful? at least to folks just getting started? We should make it easy for new users to make plots instead of digging into text files.
>
> bill
>
>
> On May 31, 2016, at 10:36 AM, Max Katz wrote:
>
> > For emacs, you can do M-x toggle-truncate-lines. I have this assigned to a hotkey in my ~/.emacs file,
> >
> > (global-set-key (kbd "<f6>") 'toggle-truncate-lines)
> >
> > which allows me to press F6 on my keyboard and truncate lines (no text wrap) after opening a text file.
> >
> > Another fun trick I found after some searching relates to the problem of scrolling up and down in a column in emacs. By default, if you scroll down with your mouse or press Page Down, your cursor will reset to the beginning of the row, which makes it annoying to try and see how a given variable changes over time. The emacswiki tells you what to add to your .emacs file to get around this,
> >
> > (defun sfp-page-down ()
> > (interactive)
> > (setq this-command 'next-line)
> > (next-line
> > (- (window-text-height)
> > next-screen-context-lines)))
> >
> > (defun sfp-page-up ()
> > (interactive)
> > (setq this-command 'previous-line)
> > (previous-line
> > (- (window-text-height)
> > next-screen-context-lines)))
> >
> > (global-set-key [next] 'sfp-page-down)
> > (global-set-key [prior] 'sfp-page-up)
> >
> > Note also that in emacs you can do Ctrl+Left and Ctrl+Right to more quickly navigate across columns.
> >
> > (Cue everyone reporting in what their personal setup is...)
> >
> > Max Katz
> > Ph.D. Candidate, Department of Physics and Astronomy
> > Stony Brook University
> > http://astro.sunysb.edu/mkatz/
> >
> > On Tue, May 31, 2016 at 1:16 PM, Aaron Dotter <aaron.dotter at gmail.com> wrote:
> > The most useful single thing I've ever found for reading MESA history files and profiles in the terminal:
> >
> > less -S history.data
> >
> > from the less manual
> >
> > -S or --chop-long-lines
> > Causes lines longer than the screen width to be chopped (trun?
> > cated) rather than wrapped. That is, the portion of a long line
> > that does not fit in the screen width is not shown. The default
> > is to wrap long lines; that is, display the remainder on the
> > next line.
> >
> > And from there you can use the arrow left and right keys to browse horizontally through the file. Changed my life!
> >
> > Aaron
> >
> >
> > On Tue, May 31, 2016 at 12:02 PM, Bill Paxton <paxton at kitp.ucsb.edu> wrote:
> > Hi Abel,
> >
> >> If the problem is that the output file is hard to read because a row with many elements continues on a new line
> >
> > Excellent new take on what might be the problem (I have to admit that I don't know what the actual problem is!). I didn't even think of that since I never look at the text files (I make plots plots and more plots). But in the rare cases where I do check something in the editor, I can set it so that it doesn't break lines of the file onto separate lines on the screen (same as your nowrap). Then I simply use horizontal scrolling. Or if I want to get several values from a row, I'll copy it to a separate file and replace spaces by CR's. then do the same for the line with the column names and match up names with values. It might be useful to have a script that would do that automatically, but I don't resort to doing it enough to be motivated to create such a script!
> >
> > Perhaps someone else has a trick for doing this. But unless you need many digits of output, making plots is the better solution in my experience.
> >
> > Cheers,
> > Bill
> >
> >
> >
> >
> >
> >
> > On May 31, 2016, at 7:22 AM, Abel Schootemeijer wrote:
> >
> >> Hello,
> >>
> >> (Disclaimer: it is very well possible that I completely misunderstood the problem, in that case please accept my apologies :) )
> >>
> >>
> >> If the problem is that the output file is hard to read because a row with many elements continues on a new line (instead of a one row per line format), you can for example do
> >>
> >> :set nowrap
> >>
> >> if you are using vim, to display the file with one row per line, so the elements of one column are displayed right below one another.
> >>
> >> Kind regards,
> >> Abel
> >>
> >>
> >> 2016-05-30 18:05 GMT+02:00 Bill Paxton <paxton at kitp.ucsb.edu>:
> >> Hi,
> >>
> >> The final model file contains only the minimum information needed to specify the structure and abundance.
> >>
> >> The final profile model will have the basics and much more. So you probably should be getting the information you need from that.
> >>
> >> Most of the test cases have lines like the following in the inlist &star_job section:
> >>
> >>
> >> save_model_when_terminate = .true.
> >> save_model_filename = 'final.mod'
> >>
> >> write_profile_when_terminate = .true.
> >> filename_for_profile_when_terminate = 'final_profile.data'
> >>
> >> The "final.mod" has what is needed to start a new run.
> >> The "final_profile.data" has lots of information about that model.
> >>
> >> Add to your "profile_columns.list" to add things to the profile.
> >> See star/defaults/profile_columns.list for options you can add.
> >> For things not built-in, use your run_star_extras to add your own.
> >>
> >> e.g., you might pick from these
> >>
> >> ! average charge from ionization module
> >> !avg_charge_H
> >> !avg_charge_He
> >> !avg_charge_C
> >> !avg_charge_N
> >> !avg_charge_O
> >> !avg_charge_Ne
> >> !avg_charge_Mg
> >> !avg_charge_Si
> >> !avg_charge_Fe
> >>
> >> ! average neutral fraction from ionization module
> >> !neutral_fraction_H
> >> !neutral_fraction_He
> >> !neutral_fraction_C
> >> !neutral_fraction_N
> >> !neutral_fraction_O
> >> !neutral_fraction_Ne
> >> !neutral_fraction_Mg
> >> !neutral_fraction_Si
> >> !neutral_fraction_Fe
> >>
> >>
> >> b
> >>
> >>
> >>
> >>
> >>
> >>
> >> On May 29, 2016, at 11:22 PM, Liliana Novais wrote:
> >>
> >> > Sorry for my late reply. I need to extract the abundances and ionizations of the several chemical elements from the final model. I am trying to understand where it is saved and how it is organized. But am unable to find it. I can't understand where one starts and the other ends.
> >>
> >>
> >> ------------------------------------------------------------------------------
> >> What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> >> patterns at an interface-level. Reveals which users, apps, and protocols are
> >> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >> planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> >> _______________________________________________
> >> mesa-users mailing list
> >> mesa-users at lists.sourceforge.net
> >> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >>
> >> ------------------------------------------------------------------------------
> >> What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> >> patterns at an interface-level. Reveals which users, apps, and protocols are
> >> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> >> J-Flow, sFlow and other flows. Make informed decisions using capacity
> >> planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e_______________________________________________
> >> mesa-users mailing list
> >> mesa-users at lists.sourceforge.net
> >> https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
> >
> > ------------------------------------------------------------------------------
> > What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> > patterns at an interface-level. Reveals which users, apps, and protocols are
> > consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> > J-Flow, sFlow and other flows. Make informed decisions using capacity
> > planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
> > _______________________________________________
> > mesa-users mailing list
> > mesa-users at lists.sourceforge.net
> > https://lists.sourceforge.net/lists/listinfo/mesa-users
> >
> >
>
> -------------- next part --------------
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> ------------------------------
>
> ------------------------------------------------------------------------------
> What NetFlow Analyzer can do for you? Monitors network bandwidth and traffic
> patterns at an interface-level. Reveals which users, apps, and protocols are
> consuming the most bandwidth. Provides multi-vendor support for NetFlow,
> J-Flow, sFlow and other flows. Make informed decisions using capacity
> planning reports. https://ad.doubleclick.net/ddm/clk/305295220;132659582;e
>
> ------------------------------
>
> _______________________________________________
> mesa-users mailing list
> mesa-users at lists.sourceforge.net
> https://lists.sourceforge.net/lists/listinfo/mesa-users
>
>
> End of mesa-users Digest, Vol 81, Issue 14
> ******************************************
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