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Dátum: 2012-07-12 11:10:52
Feladó: zoli kuli
Tárgy: Re: a Jupiteren forrong a NEB, kettévált az NTB!
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"Aki megteheti, keljen fel valamelyik hajnalon =E9s n=E9zze meg. Ne feledj=
=FCk,
szombat hajnalban k=E9t legyet =FCthet=FCnk egy csap=E1sra: a Jupiter-Hold =
fed=E9st
is megn=E9zhetj=FCk."

M=E1rmint vas=E1rnap hajnalban - miel=F5tt poty=E1ra felkelsz :)

=DCdv!



2012/7/12 =C1ron Kiss

> Kedves =C9szlel=F5k!
>
> A Jupiteren az =E9szaki egyenl=EDt=F5i z=F3na igen akt=EDvv=E1 v=E1lt, =
=E9s fel=E9ledt az
> NTB. A NEB-ben rengeteg apr=F3 csom=F3 =E9s kivet=FCl=E9s l=E1tszik, az N=
TB pedig
> kett=E9v=E1lt k=E9t komponensre!
> Aki megteheti, keljen fel valamelyik hajnalon =E9s n=E9zze meg. Ne feledj=
=FCk,
> szombat hajnalban k=E9t legyet =FCthet=FCnk egy csap=E1sra: a Jupiter-Hol=
d fed=E9st
> is megn=E9zhetj=FCk.
> N=E9zz=E9tek meg a k=E9peket, gy=F6ny=F6r=FBek!
> =DCdv=F6zlettel:
> Kiss =C1ron Keve
>
>   ----- Forwarded Message -----
> *From:* Stefan Buda
> *To:* Aron Keve Kiss
> *Sent:* Thursday, 12 July 2012, 10:19
> *Subject:* FW: Jupiter´s northern upheavals coming into focus
>
>
> Gondolom t=E9ged is =E9rdekel az al=E1bbi email.
>
> Stefan
>
>
> -----Original Message-----
> From: J.H. Rogers [mailto:jhr11@hermes.cam.ac.uk]On Behalf Of J.H.
> Rogers
> Sent: Wednesday, 11 July 2012 9:55 PM
> To: Paul Abel; Gianluigi Adamoli; Tomio Akutsu; Barry Adcock; David
> Arditti; Richard Baker; Bates.Don@corp.sysco.com; Lester Barnes; Charles
> Bell; Guillaume Bertrand; bernasconi@dollmar.com;
> Nicolas.Biver@obspm.fr; Richard Bosman; Stefan Buda; Rob Bullen; Fabio
> Carvalho; a.cidadao@fm.ul.pt; Daniel Chang; Rolando Chavez; Patrick
> Chevalley; Barry Clark; Ken Clark; Arthur Coombs; Brian Colville; Paulo
> Coelho; emilio1.colombo@telecomitalia.it; riccardo.cosenza@libero.it;
> bratislav.curcic@ericsson.com; Marc Delcroix; DIJON@chartreuse.cea.fr;
> Xavier Dupont; John Earl; PeterEdwards001@aol.com; Hideo Einaga;
> fattinnanzi.c@gmail.com; Mike FOULKES; Bernd Gaehrken; Sadegh
> Ghomizadeh; Chris Go; Ed Grafton; Guilherme Grassmann; Dave Graham;
> David Gray; fpguimaraes@globo.com; Paul Haese; Ian Hancock; Jason
> Hatton; Carlos Hernandez; Rick Hill; Kuniaki Horikawa; Phillip J.
> Hudson; Yuichi Iga; Toshihiko Ikemura; Michel Jacquesson; Rich Jakiel;
> Mark Justice; Manos Kardasis; john.kazanas@three.com.au; Thierry
> Legault; Paolo Lazzarotti; Pete Lawrence; martin.rlewis@virgin.net; Paul
> Marks; Paul Maxson; Lee Macdonald; Richard McKim; Frank J. Melillo;
> Antonello Medugno; Leonard Ellul Mercer; Hans-Joerg Mettig; Toshirou
> Mishina; Isao Miyazaki; Martin Mobberley; David M Moore; Richard
> Morisan; Andre Nikolai; Eric Ng; Dusko Novakovic;
> halloran@bermuda.ucd.ie; Tiziano Olivetti; Jordi-ortega@ono.com; Peter
> Parish; Donald C Parker; Timothy.J.Parker@jpl.nasa.gov; Damian Peach;
> chrispellier@sfr.fr; Jim Phillips; Elliott Porte;
> davidpretorius@precons.com; Jean-Pierre Prost; Terence Platt; Zac Pujic;
> Tom Richards; Mike Salway; jesus_sanluq@yahoo.es; David Scanlan; Richard
> Schmude; Clay Sherrod; John Smith; soldevilla@catalanadetelescopios.com;
> Ronald Stoyan; Paolo Tanga; Tan Wei Leong; Tang Siu kai; andrea
> tasselli; Martin Taylor; Larry Todd; Dave Tyler; Maurice Valimberti;
> Ralf Vandebergh; Marco Vedovato; Wynn Wacker; Matt Watson; Anthony
> Wesley; CKYan; Yu Gu
> Subject: Jupiter´s northern upheavals coming into focus
>
>
>
>
> Jupiter´s northern upheavals coming into focus
>
>
> Observers are now producing images of ever-improving quality as Jupiter
> moves higher in the morning sky. Attached is a compilation of colour imag=
es
> covering July 3-8, with some key features marked. (I can send an unlabell=
ed
> version, and a compilation of near-IR images, to anyone who would like
> them.)  Congratulations to all observers, and also thanks to the
> ALPO-Japan,
> from whose web site some of the best images are taken.
>
> The great upheavals on the NTB and NEB are now much better seen.  Revival=
s
> of both belts are indeed proceeding dramatically.  The whole region is ve=
ry
> complex, with disturbance spanning the NTropZ.
>
> The revived NTB(S) is a striking dark orange belt at most longitudes,
> although it is still weak from L1 ~ 40-120 (L2 ~ 60-150). (This sector
> seems
> to be moving with System I, although its boundaries are too indefinite fo=
r
> actual tracking.)  There is a separate dark grey NTB(N), everywhere excep=
t
> L2 =3D 60-106, with some darker sectors.
>
> The NTropZ is filled with pale fawn colour plus dark grey spots and
> streaks.
> (These are not as distinct as in June so it is not yet clear if they are
> the
> same ones.)
>
> The NEB is very complex at all longitudes, pale except for a narrow dark
> NEB(S), with much internal turbulence.  I can no longer identify any
> specifically disturbed sector as the source of disturbance.  On the NEBs
> edge, there are many diverse dark formations. I have numbered them for
> convenience, but cannot guarantee that these numbers match those used in
> June, as we have not yet tracked them. A closer study of the most active
> sector, L1 ~ 260-360, which was passing the most disturbed NEB sector in
> June, shows rapid changes: some ill-defined blue-grey streaks on NEBs
> crystallised into a chain of small projections at L1 <~295 (June 27, July
> 6), while the sector f. them is very disturbed, including bright white
> spots
> and very dark blue-grey spots erupting on the NEBs. The unusual brown
> sector
> of EZ(N), which enveloped dark features 13-14, disappeared as these spots
> intruded on it;  but reddish colour has spread from the NEB into the EZ(N=
)
> in other sectors, esp. around dark features 5-6.
>
> There is also an orange-brown Eq.Band at most longitudes, with some dark
> grey streaks in it. This seems to be the most distinct equatorial
> coloration
> event since 1989-91, and it could continue to grow.  The source of the
> reddish material is an outstanding puzzle: e.g., does it condense
> diffusely,
> or is it created in vigorous plumes/festoons from the NEBs disturbances?
>
> The southern hemisphere is mercifully normal by contrast.  The SEB has th=
e
> normal rifting f. the GRS.  The dark S.Trop.Band has now detached from th=
e
> p. end of the GRS.  The GRS is probably losing its dark S rim as a
> consequence and thus returning to the normal ´Voyager´ aspect, although i=
t
> is internally pale this year.  In contrast, oval BA (which is approaching
> the GRS) has reverted to a strong red colour.
>
> Finally, European observers, especially in England, don´t forget the
> occultation of Jupiter by the Moon this Sunday morning! A separate alert =
is
> going out about this.
>
> Best wishes,
> John
>
> _______________________________
>
> John H. Rogers, Ph.D.
> Jupiter Section Director,
> British Astronomical Association
>
>
> http://www.britastro.org/jupiter/
> _________________________________
>
>
>
>
> ________________________________________________________________________
>
> A csatolm=E1nyk=E9nt k=FCld=F6tt k=E9peket k=E9rj=FCk, m=E9retezd =E1t =
=FAgy, hogy a
> hosszabbik oldaluk legfeljebb 800 pixeles legyen! K=F6sz=F6nj=FCk!
>
> =C1ltal=E1nos inform=E1ci=F3k =E9s tan=E1csok a k=E9pbek=FCld=E9ssel kapc=
solatban:
>
> http://meteor.mcse.hu/digitalis_kepek.html
> ________________________________________________________________________
>
> Leonidak levelez=F5lista - =C9szlel=F5 amat=F5rcsillag=E1szok f=F3ruma
> Hozz=E1sz=F3l=E1sok: Leonidak@mcse.hu
> Listakezel=F5 utas=EDt=E1sok: Leonidak-request@mcse.hu
> Arch=EDvum, be=E1ll=EDt=E1sok: http://mailman.mcse.hu/mailman/listinfo/le=
onidak
>

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39;new york',times,serif;font-size:16px;background-color:rgb(255,255,25=
5)">"Aki megteheti, keljen fel valamelyik hajnalon =E9s n=E9zze meg. N=
e feledj=FCk, szombat hajnalban k=E9t legyet =FCthet=FCnk egy csap=E1sra: a=
Jupiter-Hold fed=E9st is megn=E9zhetj=FCk.
"


M=E1rmint vas=E1rnap hajnalban - miel=F5tt poty=E1ra felkels=
z :)

=DCdv!



class=3D"gmail_quote">2012/7/12 =C1ron Kiss < =3D"mailto:aronkevekiss@yahoo.co.uk" target=3D"_blank">aronkevekiss@yahoo.c=
o.uk
>


x #ccc solid;padding-left:1ex">
y:times new roman,new york,times,serif">
Kedves =C9szlel=F5k! an>


A Jupiteren az =E9szaki egyenl=EDt=F5i z=F3na igen akt=
=EDvv=E1 v=E1lt, =E9s fel=E9ledt az NTB. A NEB-ben rengeteg apr=F3 csom=F3 =
=E9s kivet=FCl=E9s l=E1tszik, az NTB pedig kett=E9v=E1lt k=E9t komponensre!=
Aki megteheti, keljen fel valamelyik hajnalon =E9s n=E9zze meg. =
Ne feledj=FCk, szombat hajnalban k=E9t legyet =FCthet=FCnk egy csap=E1sra: =
a Jupiter-Hold fed=E9st is megn=E9zhetj=FCk.

N=E9zz=E9tek meg a k=E9peket, gy=F6ny=F6r=FBek!
=DCdv=F6=
zlettel:
Kiss =C1ron Keve

 
"font-family:times new roman,new york,times,serif;font-size:12pt">
le=3D"font-family:times new roman,new york,times,serif;font-size:12pt">
----- Forwarded Message -----
=
From: Stefan Buda < ef=3D"mailto:beamtech@iprimus.com.au" target=3D"_blank">beamtech@iprimus.co=
m.au
>

To: Aron Keve Kiss < ref=3D"mailto:aronkevekiss@yahoo.co.uk" target=3D"_blank">aronkevekiss@yaho=
o.co.uk
>
Sent: T=
hursday, 12 July 2012, 10:19

Subject: FW: Jupiter's =
northern upheavals coming into focus


Gondolom t=
=E9ged is =E9rdekel az al=E1bbi email.

Stefan


-----Origin=
al Message-----

From: J.H. Rogers [mailto: =3D"_blank">jhr11@hermes.cam.ac.uk]On Behalf Of J.H.
Rogers
Sent:=
Wednesday, 11 July 2012 9:55 PM
To: Paul Abel; Gianluigi Adamoli; Tomio=
Akutsu; Barry Adcock; David

Arditti; Richard Baker; =3D"_blank">Bates.Don@corp.sysco.com; Lester Barnes; Charles
Bell;
Guillaume Bertrand; lank">bernasconi@dollmar.com;
fr" target=3D"_blank">Nicolas.Biver@obspm.fr; Richard Bosman; Stefan Bu=
da; Rob Bullen; Fabio

Carvalho; a.cidadao=
@fm.ul.pt
; Daniel Chang; Rolando Chavez; Patrick
Chevalley; Barry Cl=
ark; Ken Clark; Arthur Coombs; Brian Colville; Paulo
Coelho; mailto:emilio1.colombo@telecomitalia.it" target=3D"_blank">emilio1.colombo@=
telecomitalia.it
; =3D"_blank">riccardo.cosenza@libero.it;

bratisla=
v.curcic@ericsson.com
; Marc Delcroix; e.cea.fr" target=3D"_blank">DIJON@chartreuse.cea.fr;
Xavier Dupont; =
John Earl; Pet=
erEdwards001@aol.com
; Hideo Einaga;

fattinnanzi.c@=
gmail.com
; Mike FOULKES; Bernd Gaehrken; Sadegh
Ghomizadeh; Chris Go=
; Ed Grafton; Guilherme Grassmann; Dave Graham;
David Gray; ailto:fpguimaraes@globo.com" target=3D"_blank">fpguimaraes@globo.com; P=
aul Haese; Ian Hancock; Jason

Hatton; Carlos Hernandez; Rick Hill; Kuniaki Horikawa; Phillip J.
Hudson=
; Yuichi Iga; Toshihiko Ikemura; Michel Jacquesson; Rich Jakiel;
Mark Ju=
stice; Manos Kardasis; =3D"_blank">john.kazanas@three.com.au; Thierry

Legault; Paolo Lazzarotti; Pete Lawrence; irgin.net" target=3D"_blank">martin.rlewis@virgin.net; Paul
Marks; P=
aul Maxson; Lee Macdonald; Richard McKim; Frank J. Melillo;
Antonello Me=
dugno; Leonard Ellul Mercer; Hans-Joerg Mettig; Toshirou

Mishina; Isao Miyazaki; Martin Mobberley; David M Moore; Richard
Morisan=
; Andre Nikolai; Eric Ng; Dusko Novakovic;
rmuda.ucd.ie" target=3D"_blank">halloran@bermuda.ucd.ie; Tiziano Olivet=
ti; Jordi-ortega@=
ono.com
; Peter

Parish; Donald C Parker; arget=3D"_blank">Timothy.J.Parker@jpl.nasa.gov; Damian Peach;
f=3D"mailto:chrispellier@sfr.fr" target=3D"_blank">chrispellier@sfr.fr;=
Jim Phillips; Elliott Porte;

davidpretor=
ius@precons.com
; Jean-Pierre Prost; Terence Platt; Zac Pujic;
Tom Ri=
chards; Mike Salway; ank">jesus_sanluq@yahoo.es; David Scanlan; Richard

Schmude; Clay Sherrod; John Smith; elescopios.com" target=3D"_blank">soldevilla@catalanadetelescopios.com;=

Ronald Stoyan; Paolo Tanga; Tan Wei Leong; Tang Siu kai; andrea
tass=
elli; Martin Taylor; Larry Todd; Dave Tyler; Maurice Valimberti;

Ralf Vandebergh; Marco Vedovato; Wynn Wacker; Matt Watson; Anthony
Wesle=
y; CKYan; Yu Gu
Subject: Jupiter's northern upheavals coming into fo=
cus




Jupiter's northern upheavals coming into focus r>


Observers are now producing images of ever-improving quality as Jup=
iter
moves higher in
the morning sky. Attached is a compilation of colour images
covering Ju=
ly 3-8, with some key features marked. (I can send an unlabelled
version=
, and a compilation of near-IR images, to anyone who would like
them.)=
=A0 Congratulations to all observers, and also thanks to the ALPO-Japan, >
from whose web site some of the best images are taken.

The great uph=
eavals on the NTB and NEB are now much better seen.=A0 Revivals
of both =
belts are indeed proceeding dramatically.=A0 The whole region is very
co=
mplex, with disturbance spanning the NTropZ.


The revived NTB(S) is a striking dark orange belt at most longitudes, r>although it is still weak from L1 ~ 40-120 (L2 ~ 60-150). (This sector se=
ems
to be moving with System I, although its boundaries are too indefini=
te for

actual tracking.)=A0 There is a separate dark grey NTB(N), everywhere excep=
t
L2 =3D 60-106, with some darker sectors.

The NTropZ is filled
with pale fawn colour plus dark grey spots and streaks.
(These are not =
as distinct as in June so it is not yet clear if they are the
same ones.=
)

The NEB is very complex at all longitudes, pale except for a narro=
w dark

NEB(S), with much internal turbulence.=A0 I can no longer identify any
s=
pecifically disturbed sector as the source of disturbance.=A0 On the NEBs r>edge, there are many diverse dark formations. I have numbered them for >
convenience, but cannot guarantee that these numbers match those used in >June, as we have not yet tracked them. A closer study of the most active r>sector, L1 ~ 260-360, which was passing the most disturbed NEB sector in<=
br>
June, shows rapid changes: some ill-defined blue-grey streaks on NEBs
cr=
ystallised into a chain of small projections at L1 <~295 (June 27, July<=
br>6), while the sector f. them is very disturbed, including bright white s=
pots

and very dark blue-grey spots erupting
on the NEBs. The unusual brown sector
of EZ(N), which enveloped dark fe=
atures 13-14, disappeared as these spots
intruded on it;=A0 but reddish =
colour has spread from the NEB into the EZ(N)
in other sectors, esp. aro=
und dark features 5-6.


There is also an orange-brown Eq.Band at most longitudes, with some dar=
k
grey streaks in it. This seems to be the most distinct equatorial colo=
ration
event since 1989-91, and it could continue to grow.=A0 The source=
of the

reddish material is an outstanding puzzle: e.g., does it condense diffusely=
,
or is it created in vigorous plumes/festoons from the NEBs disturbance=
s?

The southern hemisphere is mercifully normal by contrast.=A0 The =
SEB has the

normal rifting f. the GRS.=A0 The dark S.Trop.Band has now detached from th=
e
p. end of the GRS.=A0 The GRS is probably losing its dark S rim as a r>consequence and thus returning to the normal 'Voyager' aspect, al=
though
it
is internally pale this year.=A0 In contrast, oval BA (which is appr=
oaching
the GRS) has reverted to a strong red colour.

Finally, Eu=
ropean observers, especially in England, don't forget the
occultatio=
n of Jupiter by the Moon this Sunday morning! A separate alert is

going out about this.

Best wishes,
John

__________________=
_____________

John H. Rogers, Ph.D.
Jupiter Section Director,
=
British Astronomical Association

< uk" target=3D"_blank">jhr11@cam.ac.uk>

http://www.=
britastro.org/jupiter/

_________________________________


=

 

_______________________________________=
_________________________________




A csatolm=E1nyk=E9nt k=FCld=F6tt k=E9peket k=E9rj=FCk, m=E9retezd =E1t =FAg=
y, hogy a

hosszabbik oldaluk legfeljebb 800 pixeles legyen! K=F6sz=F6nj=FCk!



=C1ltal=E1nos inform=E1ci=F3k =E9s tan=E1csok a k=E9pbek=FCld=E9ssel kapcso=
latban:



ht=
tp://meteor.mcse.hu/digitalis_kepek.html


________________________________________________________________________ >


Leonidak levelez=F5lista - =C9szlel=F5 amat=F5rcsillag=E1szok f=F3ruma

Hozz=E1sz=F3l=E1sok: Leonidak@mcse.hu a>

Listakezel=F5 utas=EDt=E1sok:
L=
eonidak-request@mcse.hu


Arch=EDvum, be=E1ll=EDt=E1sok: stinfo/leonidak" target=3D"_blank">http://mailman.mcse.hu/mailman/listinfo/=
leonidak




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________________________________________________________________________

A csatolmányként küldött képeket kérjük, méretezd át úgy, hogy a
hosszabbik oldaluk legfeljebb 800 pixeles legyen! Köszönjük!

Általános információk és tanácsok a képbeküldéssel kapcsolatban:

http://meteor.mcse.hu/digitalis_kepek.html
________________________________________________________________________

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