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" A k=F6vetkez=F5 p=E1r napban legal=E1bb nyugodtan alszok! "
J=F3 neked, szerintem a csill.t=E1rsadalom t=F6bbs=E9ge most a legfesz=FClt=
ebb. (Aki
nem szereti a pesszimista k=F6zhangulatot, az a sokat id=E9zgetett
yahoo-=FCst=F6k=F6s-levlist=E1t ink=E1bb ne n=E9zze most meg.)
Egy nasa-oldalon megtal=E1lhat=F3, melyik szonda mikort=F3l l=E1tja az =FCs=
t=F6k=F6st =E9s
milyen poz=EDci=F3b=F3l, =EDgy =E9rdemes n=E9zni azoknak az oldalait is:
http://www.nasa.gov/content/goddard/nasas-solar-observing-fleet-to-watch-co=
met-isons-journey-around-the-sun/
(h=E1t a natgeos film az Ausztr=E1lia-m=E9ret=FB =FCst=F6k=F6ssel nekem sem=
j=F6tt be.
=DCss=FCnk =F6ssze valamit de gyorsan err=F5l az =E1jszon-cuccr=F3l, azt=E1=
n pipa ez is,
kb ennyi j=F6tt =E1t. )
"The dates of viewings by these observatories are as follows:
Nov 21-28: STEREO-A Heliospheric Imager
Nov 26-29: STEREO-B coronagraphs
Nov 27-30: SOHO coronagraphs
Nov 28-29: STEREO-A coronagraphs
Nov 28: SDO
Nov 28: Hinode
During the last week of its inbound trip, ISON will enter the fields of
view of several NASA Heliophysics observatories. Comet ISON will be viewed
first by the broad field of view seen by NASA´s Heliospheric Imager
instrument aboard its Solar Terrestrial Relations Observatory, or STEREO,
Next the comet will be seen in what´s called coronagraphs, images that
block the brighter view of the sun itself in order to focus on the solar
atmosphere, the corona. Such images will come both from STEREO and the
joint European Space Agency/NASA Solar and Heliospheric Observatory, or
SOHO. Then, NASA´s Solar Dynamics Observatory, or SDO, will view the comet
for a few hours during its closest approach to the sun, known as
perihelion. The X-Ray Telescope on the JAXA/NASA Hinode mission will also
be looking at Comet ISON for about 55 minutes during perihelion.
All of these observatories will have different views. STEREO-B will be the
only one that sees the comet transit across the face of the sun. In SDO´s
view, the comet will appear to travel above the sun, and the SDO
instruments will point away from the center of the sun to get a better view
for three hours on Nov. 28. In addition to learning more about the comet
itself, these observations can make use of the comet as a tracer to show
movement in the solar wind and solar atmosphere."
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During the last week of its inbound trip, ISON will enter the fields of vie=
w of several NASA Heliophysics observatories. Comet ISON will be viewed fir=
st by the broad field of view seen by NASA's Heliospheric Imager instru=
ment aboard its Solar Terrestrial Relations Observatory, or STEREO, Next th=
e comet will be seen in what's called coronagraphs, images that block t=
he brighter view of the sun itself in order to focus on the solar atmospher=
e, the corona. Such images will come both from STEREO and the joint Europea=
n Space Agency/NASA Solar and Heliospheric Observatory, or SOHO. Then, NASA=
's Solar Dynamics Observatory, or SDO, will view the comet for a few ho=
urs during its closest approach to the sun, known as perihelion. The X-Ray =
Telescope on the JAXA/NASA Hinode mission will also be looking at Comet ISO=
N for about 55 minutes during perihelion.
All of these observatories will have different views. STEREO-B will be =
the only one that sees the comet transit across the face of the sun. In SDO=
's view, the comet will appear to travel above the sun, and the SDO ins=
truments will point away from the center of the sun to get a better view fo=
r three hours on Nov. 28. In addition to learning more about the comet itse=
lf, these observations can make use of the comet as a tracer to show moveme=
nt in the solar wind and solar atmosphere."=C2=A0
lman.mcse.hu/mailman/listinfo/leonidak" target=3D"_blank">