on the contributions that we have received by
then. Here is the registration link again:
https://www.mi.uni-hamburg.de/arts2024 .
Best wishes,
Stefan
On 30 Jan 2024, at 10:11, Stefan Buehler wrote:
> Dear all,
>
> summer 2024 is drawing closer, and so is the highlight of this summer, th
Dear all,
I would be very grateful if you could help spread this information. Our new
international master program is recruiting its second round of students now.
Amongst other things, it includes an advanced course on radiation and climate
that I am teaching, and that uses ARTS for the
ment to resolve this issue and get the registration form back online as
> quickly as possible.
>
> Sorry for the inconvenience.
>
> Cheers,
> Oliver
>
>> On 30. Jan 2024, at 10:11, Stefan Buehler
>> wrote:
>>
>> Dear all,
>>
>> summer 2024
Dear all,
summer 2024 is drawing closer, and so is the highlight of this summer, the ARTS
radiative transfer workshop at Kristineberg research station, on the Swedish
west coast.
The workshop will be on June 4-7, 2024 (from noon to noon). The target audience
are users and developers of the
thick atmospheres. We could look at using these
>> libraries, or at least techniques, but I'm not sure how intensive such a
>> restructuring of the code would be.
>>
>> Of course, the tricky piece here is finding someone with the time to do this
>> work. But, I think
Dear all,
I stumbled accross this interesting paper on an open C library for particularly
efficient MC calculations. Could this be the basis of ARTS 3D MC flux and
heating rate calculations? Using MC sampling also for the spectral dimension,
to be efficient, as in the second paper, which is
Dear all,
just a heads-up: we are planning a radiative transfer workshop next summer
(June 4-7, 2024, from noon to noon) in Kristineberg, at the Swedish west coast.
The target audience are users and developers of the atmospheric radiative
transfer simulator ARTS, and also anyone interested in
No problem, just great, that you answered him already! Stefan
> Am 21.03.2022 um 16:24 schrieb Patrick Eriksson
> :
>
> Hi,
>
> Sorry, I should have informed you. Kyle wrote to me on the side as well, and
> I there asked for more details and then answered separately.
>
> Not perfect. Next
And this one? - Stefan
> Anfang der weitergeleiteten Nachricht:
>
> Von: Sisma Samuel
> Betreff: [arts-users] sensitivity of SAPHIR frequencies (183.31GHZ)
> Datum: 15. März 2022 um 10:12:27 MEZ
> An: ARTS Users List
>
> Hi,
> I was trying to simulate the sensitivity of SAPHIR frequencies
Hi all, is there anyone that can take this? Stefan
> Anfang der weitergeleiteten Nachricht:
>
> Von: Kyle Johnson
> Betreff: [arts-users] ARTS ICI Cloud Simulations
> Datum: 13. März 2022 um 18:06:03 MEZ
> An: arts_users...@lists.uni-hamburg.de
> Antwort an: kyle.johnso...@colorado.edu
>
>
Focused on the solar spectral range, of course.
>> Stefan
>>> Anfang der weitergeleiteten Nachricht:
>>>
>>> *Von: *mailto:n...@eradiate.eu>>
>>> *Betreff: **Eradiate Workshop 2022*
>>> *Datum: *28. Februar 2022 um 16:58:41 MEZ
>>> *An: *mailto:st
> Von:
> Betreff: Eradiate Workshop 2022
> Datum: 28. Februar 2022 um 16:58:41 MEZ
> An:
>
> Dear Stefan Buehler,
>
> You are receiving this email because you were identified as a radiative
> transfer model user or developer. <>
> The development of Era
Dear Patrick,
I think we should put ARTS’ own line catalog in the center wherever possible
(which is based on converted current HITRAN). Use it, if you are happy with the
parameters there. If you want other parameters, and there is a good reason for
that, consider updating it. We have a
You are right, the cross dependence would still be there, and come through the
dry pressure, which gets smaller when there is more water vapor.
Overall, I also still like the option to rescale the VMRs better.
/Stefan
On 16 Sep 2021, at 21:34, Patrick Eriksson wrote:
> Stefan,
>
>>> For HSE
Hej igen,
> Yes, this puts some weight on the user. Hydrostatic equilibrium (HSE) is a
> similar case. Input profiles do not always fulfil HSE (this is the case for
> Fascod, if not a mater of geopotential vs geometric altitudes?).
Could this for Fascod also be due to the VMR definition,
Dear Stuart,
yes, exactly, thanks for pointing this out. :-) I had completely forgotten
about this.
This problem is related but slightly different: The VMR profile that we get as
input may be based on the convention that x = p_species/p_dry, rather than
p_species/p_total.
I just quickly
Hej,
> With our present definition of VMRs, we agree on that having 78% N2, 21% O2
> and e.g. 3% H2O is unphysical? That with a lot of H2O (or any other non-fixed
> gas) the standard values of the fixed gases should be scaled downwards. In
> the example above, with 0.97. Do you agree?
Yes, I
is the wet species when we go to other planets.
> Or maybe there are even planets with several wet species?
>
> That is, I would be in favour to define VMR with respect to dry air, if we
> can find a manner to handle other planets.
>
> Bye,
>
> Patrick
>
>
>
> On 202
Dear all,
Eli Mlawer brought up an interesting point in some other context:
> we recently had a LBLRTM user get confused on our vmr, which is amount_of_gas
> / amount_of_dry_air. They weren’t sure that dry air was the denominator
> instead of total air. I’m too lazy to look at the link above
Dear all,
I want to advertise this seminar in particular. An important topic!
Cheers
Stefan
Forwarded message:
From: Jimenez, Diego
To: mpi...@uni-hamburg.de
Subject: [Members.cen] [mpicen] TODAY 13:30h Special Virtual Joint
Seminar: Good Scientific Code - What, Why, How
Date: Wed, 9 Jun
Hi all,
could someone who knows answer him, please?
/Stefan
Forwarded message:
From: Thomas,Renish
To: Richard Larsson
Cc: Stefan Buehler ,
arts_users...@lists.uni-hamburg.de
Subject: Re: [arts-users] Calculated brightness temperature bias
causes.
Date: Wed, 21 Apr 2021 21:16:37 +
Hi again,
Viju pointed out that the pdf is difficult to get (damn Elsevier). Hier
is a preprint version:
https://www.dropbox.com/s/w302zg9u2mqe5d3/koshelev2020.pdf?dl=0
/Stefan
On 26 Apr 2021, at 12:52, Stefan Buehler wrote:
Hi all,
perhaps of interest for some of you:
Water vapor line
Hi all,
perhaps of interest for some of you:
Water vapor line profile at 183-GHz: Temperature dependence of
broadening, shifting, and speed-dependent shape parameters, Koshelev et
al., DOI: 10.1016/j.jqsrt.2020.107472
/Stefan
Forwarded message:
From: Baran, Anthony
To: Stefan Buehler
Subject: RE: Microwave retrieval paper
Date: Thu, 18 Feb 2021 08:54:53 +
Actually Stefan, the special issue is now remaining open for
submission of papers until 1st July - so your group could submit one.
There are two
hings this
way.
And I am not sure how easy it is to take Simon's idea and use it with
value-semantics.
With hope,
//Richard
Den mån 1 feb. 2021 kl 14:14 skrev Stefan Buehler <
stefan.bueh...@uni-hamburg.de>:
Dear Simon,
The handling of the constant data is completely up to the
implementation of t
Dear Simon,
The handling of the constant data is completely up to the
implementation of the specific scatterers.
For the ScatteringParticle class, for example, this is provided when
the object is constructed.
So when the ARTS user calls:
scattering_speciesAddScatteringHabit(...)
an object
of Stefan
Buehler
Sent: Friday, January 29, 2021 8:42:21 AM
To: Simon Pfreundschuh
Cc: ARTS Developers List
Subject: Re: Simon plans for scattering properties
Hej Simon,
can you help me understand it then, please? I do want to find the best
solution, not necessarily the quickest. (But simplicity
A controlfile example would perhaps help, as in the particle scattering
example in your concept doc.
On 29 Jan 2021, at 8:42, Stefan Buehler wrote:
Hej Simon,
can you help me understand it then, please? I do want to find the best
solution, not necessarily the quickest. (But simplicity
From: Stefan Buehler
Sent: Thursday, January 28, 2021 5:02:28 PM
To: Simon Pfreundschuh
Cc: ARTS Developers List
Subject: Re: Simon plans for scattering properties
Dear Simon,
thanks for the summary!
I think I understand more or less how this works now. A bit
unfortunate
that so much
...@mailman.rrz.uni-hamburg.de
on behalf of Stefan
Buehler
Sent: Monday, January 25, 2021 9:36:33 AM
To: ARTS Developers List
Subject: Simon plans for scattering properties
Dear all,
one thing I took home from the developer meeting on Friday is that I
would like to better understand Simon’s plans
Dear all,
one thing I took home from the developer meeting on Friday is that I
would like to better understand Simon’s plans for the scattering
properties. We need this to make a good decision on how to proceed with
the Rayleigh scattering (incorporate it into the existing scattering
data
Dear ARTS developers,
I got the pdf of his new book from Pao Wang. There is a lot of
interesting stuff about ice particles shapes and their fall behaviour:
https://www.dropbox.com/s/k5u8j40csr1kfr8/Wang_PK_Motions_of_Ice_Hydrometeors_2021.pdf?dl=0
He wrote it is ok to share among friends, so
Sorry, link was somehow messed up. Here is the right one:
https://twitter.com/hitran/status/1338929277128077313?s=20
It’s to a poster about the new CO2 line shape parameterisation.
/Stefan
On 16 Dec 2020, at 9:49, Stefan Buehler wrote:
HITRAN
@hitran
Check out
HITRAN
@hitran
Check out (Dec 16th) the #AGU2020 poster by @Robby22413232
about the new line shape parameterization of the CO2 transitions in
HITRAN2020
…20fallmeeting-agu.ipostersessions.com/Default.aspx?s…
15.12.20, 20:29
Die Twitter App downloaden
Dear ARTS friends,
there is an ARTS meeting in the calendar today. However, should we
perhaps skip it? My reason is egoistic, I have a too full todo list for
today. Also, Oliver is on vacation, so we would be a bit reduced anyhow.
Best wishes,
Stefan
Dear Stuart,
that’s great, thanks!
All the best,
Stefan
On 2 Jun 2020, at 11:52, Fox, Stuart wrote:
Hi ARTS developers,
I hope you are all well. Since next week was supposed to be the ARTS
workshop and I had some spare time when I was on holiday last week I
decided to develop syntax
Dear all,
perhaps this workshop is of interest to some of you.
Best wishes,
Stefan
> Begin forwarded message:
>
> From: Yves Govaerts
> Subject: Workshop on the development of a new open
> Date: 2. October 2019 at 16:46:00 CEST
> To: stefan.bueh...@uni-hamburg.de
>
> Dear Stefan,
>
> The
Dear all,
I started with Zenodo yesterday for another project, and it was very pleasant
to use actually. So I would suggest to put updates also there, it supports this
very well. (It automatically generates a special DOI that always points to the
latest version.) Then on the ARTS webpage just
Perhaps of interest for someone?Best wishes,StefanBegin forwarded message:From: "Imprs, Office" Subject: [Members.cen] [mpicen] Reminder: Summer School EaSyMS 2019Date: 24. June 2019 at 09:51:28 CESTTo: "Imprs, Office" Reminder – Reminder –
Dear Patrick,
an interesting mail!
Oliver and me both pondered your questions, and now had a brief discussion. We
think this kind of change is possible in principle.
Suggestions:
1. Hard to do this automatically, and perhaps dangerous. Perhaps we could add
the threshhold for considering a
Dear all,
here is a nice Mie scattering code in Python!
Best wishes,
Stefan
> Begin forwarded message:
>
> From: Bjorn Stevens
> Subject: Laser Photomedicine and Biomedical Optics at the Oregon Medical
> Laser Center
> Date: 12. February 2019 at 23:16:15 CET
> To: Stef
Dear all,
is anyone familiar with this?
Best wishes,
Stefan
> Begin forwarded message:
>
> From: "良亮"
> Subject: 回复: ARTS user
> Date: 29. June 2018 at 13:15:48 CEST
> To: "stefan.buehler"
>
> Dear Mr. Buehler
> Thank you for your reply.
>
> Yes, i want a benchmark result which simulate
Hello ARTS users,
I’m happy to announce that our new ARTS model description paper is published.
For the twitter users:
https://twitter.com/CENunihh/status/987275165938716672
If you use twitter, you would do me a great favour if you could like or retweet
this.
If you don’t and you just want
Dear all,
here is an ARTS challenge, not strictly important right now, but for my own
curiosity. Probably mostly to Patrick, but perhaps interesting also for others.
For exoplanet research, one observation technique provides the planet's transit
radius, that is, the tangent radius where the
Dear Patrick,
I think this is a move in the right direction. Good to have a clear strategy,
otherwise the complexity will quickly get out of control.
Cheers,
Stefan
> On 3. Dec 2017, at 13:52, Patrick Eriksson
> wrote:
>
> Hi Simon, Richard and all,
>
> I
Dear all,
does anyone want to reply to Sampo?
Best wishes,
Stefan
> Begin forwarded message:
>
> From: Sampo Salo
> Subject: [arts-users] Including clouds from the Chevallier_91L datasets to
> radio link simulation
> Date: 26. October 2017 at 11:07:45 GMT+2
> To:
Dear Richard,
> Ps. The cutoff is determined based on the negative frequency and not on the
> frequency of the line. Not sure if that is intentional or not, since I still
> have not read the papers on why the cutoff exists. This is not a big
> numerical issue but at most a potential mismatch
Dear Stuart, dear Richard,
Stuart, thanks for finding and reporting this. This is clearly a bug, due to an
oversight of mine at the time. For mirror lines, the shift should be such that
they continue to be at the mirror frequency of the original line. So, if the
original line shifts to higher
Hi Richard,
ok, I understand the problem. I’ll discuss with Oliver.
> (Alex ran into the former problem with the oxygen simulations yesterday. I
> guess he (or I) wanted to store O2 of LBLRTM to save reading speed but forgot
> to change the pseud-class index of the lines so all the line
Hi Simon,
really great! I look forward to learning more and discussing this in
Kristineberg.
Stefan
> On 22. Aug 2017, at 16:53, Simon Pfreundschuh
> wrote:
>
> Dear All,
>
> I just pushed a python interface for ARTS that I have been developing during
> the
Dear Xiaoying,
as Jana wrote, this does not work at the moment. However, by coincidence, we
are actually working on that right now. If all goes well, it may be usable by
the end of the year.
Best regards,
Stefan
> On 13. Jul 2017, at 15:46, Jana Mendrok wrote:
>
>
uter subroutine, due to L. D. Kaplan
> > and A. R. Curtis,
>
> M.A. Atwater: Comparison of Numerical Methods for Computing Radiative
> Temperature Changes in the Atmospheric Boundary Layer
> (http://dx.doi.org/10.1175/1520-0450(1966)005%3C0824:CONMFC%3E2.0.CO;2)
> [Flux ca
not described in further detail but all the equations are in
> the paper.
>
> Best wishes,
>
> Johannes
>
> -Ursprüngliche Nachricht-
> Von: John Burrows [mailto:burr...@iup.physik.uni-bremen.de]
> Gesendet: Mittwoch, 26. April 2017 12:02
> An: Stefan Bu
Sent from my iPhone
>
>
> John
>
>> On 26. Apr 2017, at 11:17, Stefan Buehler <stefan.bueh...@uni-hamburg.de>
>> wrote:
>>
>> Dear radiative transfer enthusiasts,
>>
>> here is a challenge for you: What is the earliest paper that de
Dear radiative transfer enthusiasts,
here is a challenge for you: What is the earliest paper that describes remote
sensing radiative transfer calculations on an electronic computer?
For energy flux calculations, there is for example the landmark paper by Manabe
and Möller from 1961. Funnily,
Dear Stuart,
it really should be included in continua.arts, I think.
All the best,
Stefan
> On 2 Feb 2017, at 17:30, Fox, Stuart wrote:
>
> Hi all,
>
> Is there a reason why the MPM89 complete H2O absorption model isn't included
> as an option in continua.arts?
Dear Ian,
yes, ok to commit also from my side. (Or we will sort out between Patrick,
Oliver, and me how to integrate the code you sent.)
This is really great. :-)
Best wishes,
Stefan
> On 22 Dec 2016, at 08:46, Patrick Eriksson
> wrote:
>
> Hi Ian,
>
> A
57 matches
Mail list logo